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1. Overview of the Medium and High Frequency Telescopes of the LiteBIRD Satellite Mission

Author: L. Montier, B. Mot, P. de Bernardis, B. Maffei, G. Pisano, F. Columbro, J. E. Gudmundsson, S. Henrot-Versillé, L. Lamagna, J. Montgomery, T. Prouvé, M. Russell, G. Savini, S. Stever, K. L. Thompson, M. Tsujimoto, C. Tucker, B. Westbrook, P. A.R. Ade, A. Adler, E. Allys, K. Arnold, D. Auguste, J. Aumont, R. Aurlien, J. Austermann, C. Baccigalupi, A. J. Banda, R. Banerji, R. B. Barreiro, S. Basak, J. Beall, D. Beck, S. Beckman, J. Bermejo, M. Bersanelli, J. Bonis, J. Borrill, F. Boulanger, S. Bounissou, M. Brilenkov, M. Brown, M. Bucher, E. Calabrese, P. Campeti, A. Carones, F. J. Casas, A. Challinor, V. Chan, K. Cheung, Y. Chinone, J. F. Cliché, L. Colombo, J. Cubas, A. Cukierman, D. Curtis, G. D’Alessandro, N. Dachlythra, M. De Petris, C. Dickinson, P. Diego-Palazuelos, M. Dobbs, T. Dotani, L. Duband, S. Duff, J. M. Duval, K. Ebisawa, T. Elleflot, H. K. Eriksen, J. Errard, T. Essinger-Hileman, F. Finelli, R. Flauger, C. Franceschet, U. Fuskeland, M. Galloway, K. Ganga, J. R. Gao, R. Genova-Santos, M. Gerbino, M. Gervasi, T. Ghigna, E. Gjerløw, M. L. Gradziel, J. Grain, F. Grupp, A. Gruppuso, T. de Haan, N. W. Halverson, P. Hargrave, T. Hasebe, M. Hasegawa, M. Hattori, M. Hazumi, D. Herman, D. Herranz, C. A. Hill, G. Hilton, Y. Hirota, E. Hivon, R. A. Hlozek, Y. Hoshino, E. de la Hoz, J. Hubmayr, K. Ichiki, T. Iida, H. Imada, K. Ishimura, H. Ishino, G. Jaehnig, T. Kaga, S. Kashima, N. Katayama, A. Kato, T. Kawasaki, R. Keskitalo, T. Kisner, Y. Kobayashi, N. Kogiso, A. Kogut, K. Kohri, E. Komatsu, K. Komatsu, K. Konishi, N. Krachmalnicoff, I. Kreykenbohm, C. L. Kuo, A. Kushino, J. V. Lanen, M. Lattanzi, A.T. Lee, C. Leloup, F. Levrier, E. Linder, T. Louis, G. Luzzi, T. Maciaszek, D. Maino, M. Maki, S. Mandelli, E. Martinez-Gonzalez, S. Masi, T. Matsumura, A. Mennella, M. Migliaccio, Y. Minami, K. Mitsuda, G. Morgante, Y. Murata, J. A. Murphy, M. Nagai, Y. Nagano, T. Nagasaki, R. Nagata, S. Nakamura, T. Namikawa, P. Natoli, S. Nerval, T. Nishibori, H. Nishino, C. O’Sullivan, H. Ogawa, S. Oguri, H. Ohsaki, I. S. Ohta, N. Okada, L. Pagano, A. Paiella, D. Paoletti, G. Patanchon, J. Peloton, F. Piacentini, G. Polenta, D. Poletti, G. Puglisi, D. Rambaud, C. Raum, S. Realini, M. Reinecke, M. Remazeilles, A. Ritacco, G. Roudil, J. A. Rubino-Martin, H. Sakurai, Y. Sakurai, M. Sandri, M. Sasaki, D. Scott, J. Seibert, Y. Sekimoto, B. Sherwin, K. Shinozaki, M. Shiraishi, P. J. Shirron, G. Signorelli, G. Smecher, R. Stompor, H. Sugai, S. Sugiyama, A. Suzuki, J. Suzuki, T. L. Svalheim, E. Switzer, R. Takaku, H. Takakura, S. Takakura, Y. Takase, Y. Takeda, A. Tartari, E. Taylor, Y. Terao, H. Thommesen, B. Thorne, T. Toda, M. Tomasi, M. Tominaga, N. Trappe, M. Tristram, M. Tsuji, J. Ullom, G. Vermeulen, P. Vielva, F. Villa, M. Vissers, N. Vittorio, I. Wehus, J. Weller, J. Wilms, B. Winter, E. J. Wollack, N. Y. Yamasaki, T. Yoshida, J. Yumoto, M. Zannoni, and A. Zonca
Subjects: Instrumentation And Photography, Astrophysics
Abstract: LiteBIRD is a JAXA-led Strategic Large-Class mission designed to search for the existence of the primordial gravitational waves produced during the inflationary phase of the Universe, through the measurements of their imprint onto the polarization of the cosmic microwave background (CMB). These measurements, requiring unprecedented sensitivity, will be performed over the full sky, at large angular scales, and over 15 frequency bands from 34 GHz to 448 GHz. The LiteBIRD instruments consist of three telescopes, namely the Low-, Medium- and High-Frequency Telescope (respectively LFT, MFT and HFT). We present in this paper an overview of the design of the Medium-Frequency Telescope (89–224 GHz) and the High-Frequency Telescope (166–448 GHz), the so-called MHFT, under European responsibility, which are two cryogenic refractive telescopes cooled down to 5 K. They include a continuous rotating half-wave plate as the first optical element, two high-density polyethylene (HDPE) lenses and more than three thousand transition-edge sensor (TES) detectors cooled to 100 mK. We provide an overview of the concept design and the remaining specific challenges that we have to face in order to achieve the scientific goals of LiteBIRD.
Published: 2020
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2. Two-dimensional echocardiographic scoring system of the left ventricular filling pressure and clinical outcomes in heart failure with preserved ejection fraction

Author: M Murayama, H Iwano, M Obokata, T Harada, K Omote, S Tsujinaga, Y Chiba, S Ishizaka, K Motoi, M Nakabachi, H Nishino, S Yokoyama, M Nishida, M Kurabayashi, and T Anzai
Subjects: Radiology, Nuclear Medicine and imaging, General Medicine, Cardiology and Cardiovascular Medicine
Abstract: Funding Acknowledgements Type of funding sources: Public Institution(s). Main funding source(s): Japan Society for the Promotion of Science (JSPS) Introduction Elevated left ventricular (LV) filling pressure in non-decompensated state is a powerful indicator of worse clinical outcomes in heart failure regardless of LV ejection fraction. However, its detection is often challenging in heart failure with preserved ejection fraction (HFpEF). Purpose This study aimed to elucidate the predictive value of recently proposed echocardiographic parameter of LV filling pressure, Visually assessed time difference between the Mitral valve and Tricuspid valve opening (VMT) score in HFpEF. Methods We retrospectively analyzed 310 well-differentiated HFpEF patients in stable conditions. Using two-dimensional echocardiographic images, time sequence of opening of mitral valve and tricuspid valve was visually assessed in the apical four-chamber view and scored to 0 to 2 (0: tricuspid valve first, 1: simultaneous, 2: mitral valve first). When the inferior vena cava diameter was dilated, 1 point was added and VMT score was calculated as four grades from 0 to 3. Based on the previous study, VMT≥2 was regarded as a sign of elevated LV filling pressure (Figure 1). LV diastolic function was graded according to the guidelines. The primary endpoint was defined as a composite of cardiac death and heart failure hospitalisation during the two years after echocardiographic examination. Results During the follow-up period, 55 events (18%) occurred, including four cardiac deaths and 51 heart failure hospitalisations. Kaplan-Meier curves demonstrated that VMT≥2 (n = 54) was associated with worse outcomes compared to patients showing VMT ≤ 1 (n = 256) (log-rank test P Conclusions In patients with HFpEF, the VMT score was independently and incrementally associated with adverse clinical outcomes. Moreover, it discriminated worse clinical outcome even in HFpEF patients with atrial fibrillation. Abstract Figure. VMT scoring Abstract Figure. Kaplan-Meier analysis
Published: 2022
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3. Pathophysiological mechanism of worsened clinical outcome by lowered left ventricular cardiac power output in heart failure

Author: H Aoyagi, S Tsujinaga, H Iwano, S Ishizaka, Y Tamaki, K Motoi, Y Chiba, M Murayama, M Nakabachi, H Nishino, S Yokoyama, T Sato, S Kaga, T Nagai, and T Anzai
Subjects: Radiology, Nuclear Medicine and imaging, General Medicine, Cardiology and Cardiovascular Medicine
Abstract: Funding Acknowledgements Type of funding sources: None. Background Cardiac power output (CPO) is a measure of cardiac pumping function, and CPO during exercise is known to be a powerful prognostic marker of heart failure. Despite its prognostic significance, pathophysiological mechanism of the association between reduced CPO and worse clinical outcome is unknown. We hypothesized that reduced CPO is associated with worse outcome through the reduced exercise capacity and enhanced ventilatory response. Methods Cardiopulmonary exercise testing and exercise stress echocardiography were performed in consecutive 64 patients with chronic heart failure who admitted to our department for the management of heart failure [60 ± 14 years old, left ventricular (LV) ejection fraction 39 ± 16%, ischemic etiology 16%, brain natriuretic peptide 124 pg/ml (51-313)]. Peak oxygen uptake (peak VO2) and the lowest minute ventilation / carbon dioxide production ratio (VE/VCO2) were measured as a parameter of exercise tolerance and that of ventilatory response, respectively. LV ejection fraction was measured by disk summation method at peak exercise. By using Doppler images, E/e" at peak exercise was measured as a marker of LV filling pressure, and CPO normalized by LV mass was obtained as 0.222 × cardiac output × mean blood pressure / LV mass [W/100 g]. Cardiac events defined as hospitalization for heart failure, cardiac death, or implantation of a LV assist device after the examinations were recorded. Results CPO at rest was weakly correlated with peak VO2 (r = 0.25, p = 0.046) but not with VE/VCO2. In contrast, CPO at peak exercise was positively correlated with peak VO2 (r = 0.50, p Conclusions In patients with chronic heart failure, CPO during exercise was associated with prognosis of heart failure through the reduced exercise capacity and enhanced ventilatory response.
Published: 2022
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4. Optical Characterization of OMT-Coupled TES Bolometers for LiteBIRD

Author: J. Hubmayr, P. A. R. Ade, A. Adler, E. Allys, D. Alonso, K. Arnold, D. Auguste, J. Aumont, R. Aurlien, J. E. Austermann, S. Azzoni, C. Baccigalupi, A. J. Banday, R. Banerji, R. B. Barreiro, N. Bartolo, S. Basak, E. Battistelli, L. Bautista, J. A. Beall, D. Beck, S. Beckman, K. Benabed, J. Bermejo-Ballesteros, M. Bersanelli, J. Bonis, J. Borrill, F. Bouchet, F. Boulanger, S. Bounissou, M. Brilenkov, M. L. Brown, M. Bucher, E. Calabrese, M. Calvo, P. Campeti, A. Carones, F. J. Casas, A. Catalano, A. Challinor, V. Chan, K. Cheung, Y. Chinone, C. Chiocchetta, S. E. Clark, L. Clermont, S. Clesse, J. Cliche, F. Columbro, J. A. Connors, A. Coppolecchia, W. Coulton, J. Cubas, A. Cukierman, D. Curtis, F. Cuttaia, G. D’Alessandro, K. Dachlythra, P. de Bernardis, T. de Haan, E. de la Hoz, M. De Petris, S. Della Torre, J. J. Daz Garca, C. Dickinson, P. Diego-Palazuelos, M. Dobbs, T. Dotani, D. Douillet, E. Doumayrou, L. Duband, A. Ducout, S. M. Duff, J. M. Duval, K. Ebisawa, T. Elleflot, H. K. Eriksen, J. Errard, T. Essinger-Hileman, S. Farrens, F. Finelli, R. Flauger, K. Fleury-Frenette, C. Franceschet, U. Fuskeland, L. Galli, S. Galli, M. Galloway, K. Ganga, J. R. Gao, R. T. Genova-Santos, M. Georges, M. Gerbino, M. Gervasi, T. Ghigna, S. Giardiello, E. Gjerlw, R. Gonzlez Gonzles, M. L. Gradziel, J. Grain, L. Grandsire, F. Grupp, A. Gruppuso, J. E. Gudmundsson, N. W. Halverson, J. Hamilton, P. Hargrave, T. Hasebe, M. Hasegawa, M. Hattori, M. Hazumi, S. Henrot-Versill, B. Hensley, D. Herman, D. Herranz, G. C. Hilton, E. Hivon, R. A. Hlozek, D. Hoang, A. L. Hornsby, Y. Hoshino, K. Ichiki, T. Iida, T. Ikemoto, H. Imada, K. Ishimura, H. Ishino, G. Jaehnig, M. Jones, T. Kaga, S. Kashima, N. Katayama, A. Kato, T. Kawasaki, R. Keskitalo, C. Kintziger, T. Kisner, Y. Kobayashi, N. Kogiso, A. Kogut, K. Kohri, E. Komatsu, K. Komatsu, K. Konishi, N. Krachmalnicoff, I. Kreykenbohm, C. L. Kuo, A. Kushino, L. Lamagna, J. V. Lanen, G. Laquaniello, M. Lattanzi, A. T. Lee, C. Leloup, F. Levrier, E. Linder, M. J. Link, A. I. Lonappan, T. Louis, G. Luzzi, J. Macias-Perez, T. Maciaszek, B. Maffei, D. Maino, M. Maki, S. Mandelli, M. Maris, B. Marquet, E. Martnez-Gonzlez, F. A. Martire, S. Masi, M. Massa, M. Masuzawa, S. Matarrese, F. T. Matsuda, T. Matsumura, L. Mele, A. Mennella, M. Migliaccio, Y. Minami, K. Mitsuda, A. Moggi, M. Monelli, A. Monfardini, J. Montgomery, L. Montier, G. Morgante, B. Mot, Y. Murata, J. A. Murphy, M. Nagai, Y. Nagano, T. Nagasaki, R. Nagata, S. Nakamura, R. Nakano, T. Namikawa, F. Nati, P. Natoli, S. Nerval, N. Neto Godry Farias, T. Nishibori, H. Nishino, F. Noviello, G. C. O’Neil, C. O’Sullivan, K. Odagiri, H. Ochi, H. Ogawa, S. Oguri, H. Ohsaki, I. S. Ohta, N. Okada, L. Pagano, A. Paiella, D. Paoletti, G. Pascual Cisneros, A. Passerini, G. Patanchon, V. Pelgrim, J. Peloton, V. Pettorino, F. Piacentini, M. Piat, G. Piccirilli, F. Pinsard, G. Pisano, J. Plesseria, G. Polenta, D. Poletti, T. Prouv, G. Puglisi, D. Rambaud, C. Raum, S. Realini, M. Reinecke, C. D. Reintsema, M. Remazeilles, A. Ritacco, P. Rosier, G. Roudil, J. Rubino-Martin, M. Russell, H. Sakurai, Y. Sakurai, M. Sandri, M. Sasaki, G. Savini, D. Scott, J. Seibert, Y. Sekimoto, B. Sherwin, K. Shinozaki, M. Shiraishi, P. Shirron, A. Shitvov, G. Signorelli, G. Smecher, F. Spinella, J. Starck, S. Stever, R. Stompor, R. Sudiwala, S. Sugiyama, R. Sullivan, A. Suzuki, J. Suzuki, T. Suzuki, T. L. Svalheim, E. Switzer, R. Takaku, H. Takakura, S. Takakura, Y. Takase, Y. Takeda, A. Tartari, D. Tavagnacco, A. Taylor, E. Taylor, Y. Terao, L. Terenzi, J. Thermeau, H. Thommesen, K. L. Thompson, B. Thorne, T. Toda, M. Tomasi, M. Tominaga, N. Trappe, M. Tristram, M. Tsuji, M. Tsujimoto, C. Tucker, R. Ueki, J. N. Ullom, K. Umemori, L. Vacher, J. Van Lanen, G. Vermeulen, P. Vielva, F. Villa, M. R. Vissers, N. Vittorio, B. Wandelt, W. Wang, I. K. Wehus, J. Weller, B. Westbrook, G. Weymann-Despres, J. Wilms, B. Winter, E. J. Wollack, N. Y. Yamasaki, T. Yoshida, J. Yumoto, K. Watanuki, A. Zacchei, M. Zannoni, A. Zonca, Hubmayr, J, Ade, P, Adler, A, Allys, E, Alonso, D, Arnold, K, Auguste, D, Aumont, J, Aurlien, R, Austermann, J, Azzoni, S, Baccigalupi, C, Banday, A, Banerji, R, Barreiro, R, Bartolo, N, Basak, S, Battistelli, E, Bautista, L, Beall, J, Beck, D, Beckman, S, Benabed, K, Bermejo-Ballesteros, J, Bersanelli, M, Bonis, J, Borrill, J, Bouchet, F, Boulanger, F, Bounissou, S, Brilenkov, M, Brown, M, Bucher, M, Calabrese, E, Calvo, M, Campeti, P, Carones, A, Casas, F, Catalano, A, Challinor, A, Chan, V, Cheung, K, Chinone, Y, Chiocchetta, C, Clark, S, Clermont, L, Clesse, S, Cliche, J, Columbro, F, Connors, J, Coppolecchia, A, Coulton, W, Cubas, J, Cukierman, A, Curtis, D, Cuttaia, F, D’Alessandro, G, Dachlythra, K, de Bernardis, P, de Haan, T, de la Hoz, E, De Petris, M, Della Torre, S, Daz Garca, J, Dickinson, C, Diego-Palazuelos, P, Dobbs, M, Dotani, T, Douillet, D, Doumayrou, E, Duband, L, Ducout, A, Duff, S, Duval, J, Ebisawa, K, Elleflot, T, Eriksen, H, Errard, J, Essinger-Hileman, T, Farrens, S, Finelli, F, Flauger, R, Fleury-Frenette, K, Franceschet, C, Fuskeland, U, Galli, L, Galli, S, Galloway, M, Ganga, K, Gao, J, Genova-Santos, R, Georges, M, Gerbino, M, Gervasi, M, Ghigna, T, Giardiello, S, Gjerlw, E, Gonzles, R, Gradziel, M, Grain, J, Grandsire, L, Grupp, F, Gruppuso, A, Gudmundsson, J, Halverson, N, Hamilton, J, Hargrave, P, Hasebe, T, Hasegawa, M, Hattori, M, Hazumi, M, Henrot-Versill, S, Hensley, B, Herman, D, Herranz, D, Hilton, G, Hivon, E, Hlozek, R, Hoang, D, Hornsby, A, Hoshino, Y, Ichiki, K, Iida, T, Ikemoto, T, Imada, H, Ishimura, K, Ishino, H, Jaehnig, G, Jones, M, Kaga, T, Kashima, S, Katayama, N, Kato, A, Kawasaki, T, Keskitalo, R, Kintziger, C, Kisner, T, Kobayashi, Y, Kogiso, N, Kogut, A, Kohri, K, Komatsu, E, Komatsu, K, Konishi, K, Krachmalnicoff, N, Kreykenbohm, I, Kuo, C, Kushino, A, Lamagna, L, Lanen, J, Laquaniello, G, Lattanzi, M, Lee, A, Leloup, C, Levrier, F, Linder, E, Link, M, Lonappan, A, Louis, T, Luzzi, G, Macias-Perez, J, Maciaszek, T, Maffei, B, Maino, D, Maki, M, Mandelli, S, Maris, M, Marquet, B, Martnez-Gonzlez, E, Martire, F, Masi, S, Massa, M, Masuzawa, M, Matarrese, S, Matsuda, F, Matsumura, T, Mele, L, Mennella, A, Migliaccio, M, Minami, Y, Mitsuda, K, Moggi, A, Monelli, M, Monfardini, A, Montgomery, J, Montier, L, Morgante, G, Mot, B, Murata, Y, Murphy, J, Nagai, M, Nagano, Y, Nagasaki, T, Nagata, R, Nakamura, S, Nakano, R, Namikawa, T, Nati, F, Natoli, P, Nerval, S, Neto Godry Farias, N, Nishibori, T, Nishino, H, Noviello, F, O’Neil, G, O’Sullivan, C, Odagiri, K, Ochi, H, Ogawa, H, Oguri, S, Ohsaki, H, Ohta, I, Okada, N, Pagano, L, Paiella, A, Paoletti, D, Pascual Cisneros, G, Passerini, A, Patanchon, G, Pelgrim, V, Peloton, J, Pettorino, V, Piacentini, F, Piat, M, Piccirilli, G, Pinsard, F, Pisano, G, Plesseria, J, Polenta, G, Poletti, D, Prouv, T, Puglisi, G, Rambaud, D, Raum, C, Realini, S, Reinecke, M, Reintsema, C, Remazeilles, M, Ritacco, A, Rosier, P, Roudil, G, Rubino-Martin, J, Russell, M, Sakurai, H, Sakurai, Y, Sandri, M, Sasaki, M, Savini, G, Scott, D, Seibert, J, Sekimoto, Y, Sherwin, B, Shinozaki, K, Shiraishi, M, Shirron, P, Shitvov, A, Signorelli, G, Smecher, G, Spinella, F, Starck, J, Stever, S, Stompor, R, Sudiwala, R, Sugiyama, S, Sullivan, R, Suzuki, A, Suzuki, J, Suzuki, T, Svalheim, T, Switzer, E, Takaku, R, Takakura, H, Takakura, S, Takase, Y, Takeda, Y, Tartari, A, Tavagnacco, D, Taylor, A, Taylor, E, Terao, Y, Terenzi, L, Thermeau, J, Thommesen, H, Thompson, K, Thorne, B, Toda, T, Tomasi, M, Tominaga, M, Trappe, N, Tristram, M, Tsuji, M, Tsujimoto, M, Tucker, C, Ueki, R, Ullom, J, Umemori, K, Vacher, L, Van Lanen, J, Vermeulen, G, Vielva, P, Villa, F, Vissers, M, Vittorio, N, Wandelt, B, Wang, W, Wehus, I, Weller, J, Westbrook, B, Weymann-Despres, G, Wilms, J, Winter, B, Wollack, E, Yamasaki, N, Yoshida, T, Yumoto, J, Watanuki, K, Zacchei, A, Zannoni, M, Zonca, A, and National Aeronautics and Space Administration (US)
Subjects: CMB, TES, OMT, Low temperature detector, Bolometer, FIS/05 - ASTRONOMIA E ASTROFISICA, Settore FIS/05 - Astronomia e Astrofisica, General Materials Science, Condensed Matter Physics, CMB, TES, OMT, Low temperature detector, Bolometer, Atomic and Molecular Physics, and Optics
Abstract: et al., Feedhorn- and orthomode transducer- (OMT) coupled transition edge sensor (TES) bolometers have been designed and micro-fabricated to meet the optical specifications of the LiteBIRD high frequency telescope (HFT) focal plane. We discuss the design and optical characterization of two LiteBIRD HFT detector types: dual-polarization, dual-frequency-band pixels with 195/280 GHz and 235/337 GHz band centers. Results show well-matched passbands between orthogonal polarization channels and frequency centers within 3% of the design values. The optical efficiency of each frequency channel is conservatively reported to be within the range 0.64−0.72, determined from the response to a cryogenic, temperature-controlled thermal source. These values are in good agreement with expectations and either exceed or are within 10% of the values used in the LiteBIRD sensitivity forecast. Lastly, we report a measurement of loss in Nb/SiNx/Nb microstrip at 100 mK and over the frequency range 200–350 GHz, which is comparable to values previously reported in the literature., This work is supported by NASA under grant no. 80NSSC18K0132.
Published: 2022

5. Abstract 4117: Clinicopathologic and molecular characterization of KRASG12D lung cancers

Author: Jia Luo, Biagio Ricciuti, Joao V. Alessi, Xinan Wang, Victor Vaz, Federica Pecci, Tom Nguyen, James Lindsay, Bijaya Sharma, Kristen D. Felt, Scott J. Rodig, Mizuki H. Nishino, Lynette M. Sholl, David A. Barbie, Pasi A. Jänne, and Mark M. Awad
Subjects: Cancer Research, Oncology
Abstract: Introduction: Allele-specific KRAS inhibitors are an emerging class of cancer therapies. KRASmut non-small cell lung cancers (NSCLCs) exhibit heterogenous outcomes, driven by differences in underlying biology shaped by co-mutations. In contrast to KRASG12C NSCLC, KRASG12D NSCLC is associated with low/never smoking status and has not been characterized in depth. Methods: We examined characteristics of patients with advanced KRASmut NSCLC seen at a single center. RECISTv1.1 and Cox-proportional hazards models adjusting for line of therapy and performance status were used to compare outcomes to immunotherapy. Benjamini-Hochberg corrected q-values were used for genomic comparisons. Results: Of 1,823 patients with KRASmut NSCLC, 16% (n=283) harbored KRASG12D which was mutually exclusive from other targetable alterations. Among these, the median age was 66 (range 20-92), 0.7% had squamous histology, 30% had a never/light smoking history ( Conclusions: KRASG12D lung cancers harbor distinct clinical, genomic, and immunologic features compared to other KRAS mutated lung cancers and numerically worse outcomes to PD-(L)1 blockade-based therapies. Drug development for KRASG12D lung cancers will have to take these differences into account. Citation Format: Jia Luo, Biagio Ricciuti, Joao V. Alessi, Xinan Wang, Victor Vaz, Federica Pecci, Tom Nguyen, James Lindsay, Bijaya Sharma, Kristen D. Felt, Scott J. Rodig, Mizuki H. Nishino, Lynette M. Sholl, David A. Barbie, Pasi A. Jänne, Mark M. Awad. Clinicopathologic and molecular characterization of KRASG12D lung cancers [abstract]. In: Proceedings of the American Association for Cancer Research Annual Meeting 2022; 2022 Apr 8-13. Philadelphia (PA): AACR; Cancer Res 2022;82(12_Suppl):Abstract nr 4117.
Published: 2022
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6. Data acquisition and management system for the CMB polarization experiment: Simons Array

Author: Theodore Kisner, P. Siritanasak, Nathan Whitehorn, Kevin T. Crowley, Y. Zhou, Daisuke Kaneko, Tucker Elleflot, Akito Kusaka, Benjamin Westbrook, Alexandra S. Rahlin, S. Takakura, L. Howe, Haruaki Hirose, H. Nishino, John Groh, Joshua Montgomery, Masashi Hazumi, Masaya Hasegawa, Darcy Barron, S. Kikuchi, A. Zahn, Charles A. Hill, D. Tanabe, S. Takatori, Graeme Smecher, Amy N. Bender, and Yuji Chinone
Subjects: Data acquisition, business.industry, Observatory, Computer science, Data management, Cosmic microwave background, Real-time computing, Bandwidth (signal processing), Management system, business, Data rate, Raw data
Abstract: The Simons Array upgrades the POLARBEAR experiment, which measures the cosmic microwave background from the Atacama Desert in Chile, with three newly developed receivers. Each receiver has 7,588 transition-edge sensor bolometers with a raw data rate of approximately 20 MB/s. This significantly increased data rate required us to develop a new data-acquisition (DAQ) and data-management system. As the network bandwidth from our observatory to our data-storage sites outside Chile is not high enough to send all the raw data, we compress the raw data on-site. The expected yearly compressed data rate is approximately 60 TB from each receiver. We have also developed a new housekeeping DAQ system. The new housekeeping DAQ system is a distributed system to handle the various newly added monitoring systems and to better understand our instruments and environments. Those data can also be fetched by another module for real-time monitoring of our instrument from all over the world with latencies on the order of minutes. We deployed the first receiver in late 2018 and started the commissioning of the DAQ system. The DAQ system has been working without significant problems and already accumulates a considerable amount of the new receiver data from the commissioning observations. In this presentation, we summarize and report the status of the new systems.
Published: 2020
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7. Results of gravitational lensing and primordial gravitational waves from the POLARBEAR experiment

Author: Peter A. R. Ade, Davide Poletti, C. Verges, Shunsuke Adachi, Kam Arnold, Yuji Chinone, A. Suzuki, Yuto Minami, Chang Feng, J. Peloton, Nathan Whitehorn, Oliver Jeong, N. W. Halverson, Yuki Inoue, T. Hamada, Akito Kusaka, Y. Zhou, A. Zahn, A. Cukierman, M. Aguilar, Carole Tucker, D. Beck, Nicoletta Krachmalnicoff, Rolando Dünner, Brian Keating, Paul L. Richards, Stephen M. Feeney, J. C. Groh, Julian Borrill, C. Tsai, Joshua Montgomery, Darcy Barron, Theodore Kisner, R. Stompor, G. Hall, D. Boettger, Tucker Elleflot, Josquin Errard, Frederick Matsuda, L. N. Lowry, D. Leon, Takayuki Tomaru, Reijo Keskitalo, Benjamin Westbrook, M. Navaroli, D. Kaneko, K. Cheung, Osamu Tajima, A. T. P. Pham, Eric V. Linder, Giulio Fabbian, A. J. Gilbert, L. Howe, Neil Goeckner-Wald, H. El-Bouhargani, Max Silva-Feaver, Hans P. Paar, M. A. Dobbs, S. Takatori, Federico Bianchini, Colin Ross, Christian L. Reichardt, John Groh, Praween Siritanasak, Julien Carron, Tomotake Matsumura, T. Fujino, Y. Akiba, H. Nishino, G. Jaehnig, Giuseppe Puglisi, Charles A. Hill, D. Tanabe, Andrew H. Jaffe, Masashi Hazumi, Nicholas Galitzki, Blake D. Sherwin, S. Kikuchi, Carlo Baccigalupi, E. M. Leitch, S. Beckman, N. Katayama, Grant Teply, A. Ducout, Aashrita Mangu, M. LeJeune, Adrian T. Lee, Nathan Stebor, Masaya Hasegawa, S. Takakura, Y. Segawa, Scott Chapman, Kevin T. Crowley, Chinone, Y, Adachi, S, Ade, P, Aguilar, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Beckman, S, Bianchini, F, Boettger, D, Borrill, J, Elbouhargani, H, Carron, J, Chapman, S, Cheung, K, Crowley, K, Cukierman, A, Dunner, R, Dobbs, M, Ducout, A, Elleflot, T, Errard, J, Fabbian, G, Feeney, S, Feng, C, Fujino, T, Galitzki, N, Gilbert, A, Goeckner-Wald, N, Groh, J, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hazumi, M, Hill, C, Howe, L, Inoue, Y, Jaehnig, G, Jaffe, A, Jeong, O, Lejeune, M, Kaneko, D, Katayama, N, Keating, B, Keskitalo, R, Kikuchi, S, Kisner, T, Krachmalnicoff, N, Kusaka, A, Lee, A, Leitch, E, Leon, D, Linder, E, Lowry, L, Mangu, A, Matsuda, F, Matsumura, T, Minami, Y, Montgomery, J, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Pham, A, Poletti, D, Puglisi, G, Reichardt, C, Richards, P, Ross, C, Segawa, Y, Sherwin, B, Silva-Feaver, M, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Takatori, S, Tanabe, D, Teply, G, Tomaru, T, Tsai, C, Tucker, C, Verges, C, Westbrook, B, Whitehorn, N, Zahn, A, Zhou, Y, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), POLARBEAR, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: History, satellite: Planck, Cosmic microwave background, gravitational lensing, cosmic background radiation: polarization, detector: noise, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravity waves, power spectrum, 01 natural sciences, Education, Primary mirror, symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, gravitation: lens, Polarization, 0103 physical sciences, Planck, mirror, 010303 astronomy & astrophysics, Physics, COSMIC cancer database, 010308 nuclear & particles physics, Gravitational wave, Settore FIS/05, POLARBEAR experiment, Gravitational effects, gravitational radiation: primordial, Astrophysics::Instrumentation and Methods for Astrophysics, Polarization (waves), Galaxy, Computer Science Applications, Gravitational lens, B-mode, symbols, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], galaxy
Abstract: POLARBEAR is a Cosmic Microwave Background radiation (CMB) polarization experiment that is located in the Atacama Desert in Chile. The scientific goals of the experiment are to characterize the B-mode signal from gravitational lensing, as well as to search for B-mode signals created by primordial gravitational waves (PGWs). Polarbear started observations in 2012 and has published a series of results. These include the first measurement of a nonzero B-mode angular auto-power spectrum at sub-degree scales where the dominant signal is gravitational lensing of the CMB. In addition, we have achieved the first measurement of crosscorrelation between the lensing potential, which was reconstructed from the CMB polarization data alone by Polarbear, and the cosmic shear field from galaxy shapes by the Subaru Hyper Suprime-Cam (HSC) survey. In 2014, we installed a continuously rotating half-wave plate (CRHWP) at the focus of the primary mirror to search for PGWs and demonstrated the control of low-frequency noise. We have found that the low-frequency B-mode power in the combined dataset with the Planck high-frequency maps is consistent with Galactic dust foreground, thus placing an upper limit on the tensor-to-scalar ratio of r < 0.90 at the 95% confidence level after marginalizing over the foregrounds.
Published: 2020
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8. Design and Assembly of SPT-3G Cold Readout Hardware

Author: Amy N. Bender, A. Cukierman, D. Dutcher, E. V. Denison, V. G. Yefremenko, C. M. Posada, W. B. Everett, Trupti Khaire, John E. Carlstrom, K. L. Thompson, Joaquin Vieira, Q. Y. Tang, Carole Tucker, Joshua Montgomery, A. E. Lowitz, Z. Pan, Alexandra S. Rahlin, Jason E. Austermann, K. W. Yoon, Graeme Smecher, R. Basu Thakur, Chihway Chang, Valentine Novosad, J. E. Ruhl, Faustin Carter, Leila R. Vale, Y. Hori, K. M. Rotermund, K. Vanderlinde, M. A. Dobbs, Peter A. R. Ade, S. E. Kuhlmann, Junjia Ding, K. T. Story, Oliver Jeong, J. F. Cliche, Kent D. Irwin, Gene C. Hilton, W. L. Holzapfel, M. Korman, A. A. Stark, R. N. Gannon, M. R. Young, Donna Kubik, John E. Pearson, Kaori Hattori, T. Natoli, Gensheng Wang, M. Jonas, Aritoki Suzuki, John Groh, A. J. Gilbert, Jason W. Henning, Tucker Elleflot, C. L. Kuo, A. Foster, Adam Anderson, Zeeshan Ahmed, Thomas Cecil, N. W. Halverson, T. de Haan, L. J. Saunders, J. A. Sobrin, H. Nguyen, Jessica Avva, Nathan Whitehorn, S. S. Meyer, Stephen Padin, Masaya Hasegawa, H. Nishino, A. M. Kofman, I. Shirley, Andrew Nadolski, A. H. Harke-Hosemann, G. I. Noble, Aaron Lee, Erik Shirokoff, N. Huang, J. T. Sayre, D. Barron, N. L. Harrington, and Bradford Benson
Subjects: 010302 applied physics, Physics, business.industry, Detector, Condensed Matter Physics, 01 natural sciences, Atomic and Molecular Physics, and Optics, Resonator, Upgrade, Thermal conductivity, South Pole Telescope, Planar, 0103 physical sciences, Optoelectronics, General Materials Science, 010306 general physics, business, Electrical impedance, Stripline
Abstract: The third-generation upgrade to the receiver on the South Pole Telescope, SPT-3G, was installed at the South Pole during the 2016–2017 austral summer to measure the polarization of the cosmic microwave background. Increasing the number of detectors by a factor of 10 to ∼16,000 \ud ∼16,000\ud required the multiplexing factor to increase to 68 and the bandwidth of the frequency-division readout electronics to span 1.6–5.2 MHz. This increase necessitates low-thermal conductance, low-inductance cryogenic wiring. Our cold readout system consists of planar thin-film aluminum inductive–capacitive resonators, wired in series with the detectors, summed together, and connected to 4K SQUIDs by 10−μm \ud 10−μm\ud -thick niobium–titanium (NbTi) broadside-coupled striplines. Here, we present an overview of the cold readout electronics for SPT-3G, including assembly details and characterization of electrical and thermal properties of the system. We report, for the NbTi striplines, values of R≤10 −4 Ω \ud R≤10−4Ω\ud , L=21±1 nH \ud L=21±1 nH\ud , and C=1.47±.02 nF \ud C=1.47±.02 nF\ud . Additionally, the striplines’ thermal conductivity is described by kA=6.0±0.3 T 0.92±0.04 μW mm K −1 \ud kA=6.0±0.3 T0.92±0.04 μW mm K−1\ud . Finally, we provide projections for cross talk induced by parasitic impedances from the stripline and find that the median value of percentage cross talk from leakage current is 0.22 and 0.09% \ud 0.09%\ud from wiring impedance.
Published: 2018
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9. Preoperative Diagnosis of Histological Lymph Node Metastasis of Resected Perihilar Cholangiocarcinoma Using Diffusion-Weighted Magnetic Resonance Imaging

Author: I. Hosokawa, K. Hayano, K. Furukawa, T. Takayashiki, S. Kuboki, S. Takano, D. Suzuki, N. Sakai, T. Mishima, T. Konishi, H. Nishino, and M. Ohtsuka
Subjects: Hepatology, Gastroenterology
Published: 2022
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10. Abstract PD2-07: Real-time navigation for sentinel lymph node biopsy in breast cancer patients using projection mapping with indocyanine green fluorescence

Author: Megumi Takeuchi, N Sakita-Kawaguchi, H Nishino, Etsuro Hatano, Masakazu Toi, T Okuda, Masae Torii, Yoshihide Matsumoto, Eiji Suzuki, Masahiro Takada, Fumiaki Sato, S Seo, and Y Nakayama
Subjects: Cancer Research, medicine.diagnostic_test, business.industry, Sentinel lymph node, Cancer, Body movement, medicine.disease, Breast cancer, Oncology, Biopsy, medicine, Medical imaging, Median body, Nuclear medicine, business, Indocyanine green fluorescence
Abstract: Background) Sentinel lymph node (SLN) biopsy using indocyanine green fluorescence (fICG) method showed equal or better identification rate compared with blue dye or radioisotope (RI) method. In the fICG method, lymphatic vessels which drain into the SLNs can be seen through skin or subcutaneous tissue using near infrared camera (Photodynamic Eye®: PDE), and we can easily find the SLNs. However, whenever we observe the fluorescence images, we have to hold the PDE, turn off the operating light, and look at a monitor because fluorescence images cannot be seen directly. Medical imaging projection system (MIPS) is a new device which detects fluorescent emission from the organ and projects their images on the location of the fluorescence emission (Panasonic Connected Solutions Company, Japan). Projected images can be adjusted following the body movement or deformation of the organ. Therefore, MIPS could provide an option for real-time navigation for the SLN biopsy. The aim of this study was to evaluate the clinical utility of the MIPS. Patients and methods) Patients with clinically node-negative primary breast cancer underwent the fICG SLN biopsy using MIPS. Primary endpoint was identification rate of the fICG method using MIPS. At first, the study was conducted as an interventional study because the MIPS was the unapproved medical device. After approval of the MIPS, this study was conducted as an observational study. The study protocol was approved by the institutional review board at Kyoto University Hospital. All patients provided informed consent to participate in this study. Results) Between March 2016 and May 2017, 39 patients (40 procedures) underwent the fICG method SLN biopsy using MIPS. The median age was 55 years (range 32–74 years), and the median body mass index was 20.4 kg/m2 (range 17.7–27.7 kg/m2). About half had tumor stage T1 (58%) and 8 (20.0%) had DCIS. 8 procedures (20%) were performed after preoperative systemic therapy (PST). As MIPS itself can illuminate the operating field, SLN biopsy using MIPS was successfully performed without operating light in all procedures. At least one SLN was detected using MIPS for all procedures and the identification rate was 100% (95% CI: 91–100%). Median number of SLNs detected by MIPS was 3 (range 1–9) for all procedures, and 3 (range 2–8) for procedures after PST. Two pathologically positive SLNs and one SLN which included isolated tumor cells were detected by MIPS. In 25 procedures, RI was also used. 62 of 97 SLNs detected by MIPS (64%) were also detected by RI. However, no SLNs were detected only by RI. Conclusions) Although we still may not be able to avoid RI method because 25/40 (62.5%) procedures required the combined use of RI method, the fICG methods SLN biopsy using MIPS, which showed comparable identification rate of SLN with the conventional methods, could be useful tool with a view of allowing us to perform a real-time navigation surgery. Acknowledgements) This study was supported by Acceleration Transformative research for Medical innovation, Japan Agency for Medical Research and Development (AMED). Citation Format: Takada M, Takeuchi M, Suzuki E, Sato F, Matsumoto Y, Torii M, Sakita-Kawaguchi N, Nakayama Y, Okuda T, Nishino H, Seo S, Hatano E, Toi M. Real-time navigation for sentinel lymph node biopsy in breast cancer patients using projection mapping with indocyanine green fluorescence [abstract]. In: Proceedings of the 2017 San Antonio Breast Cancer Symposium; 2017 Dec 5-9; San Antonio, TX. Philadelphia (PA): AACR; Cancer Res 2018;78(4 Suppl):Abstract nr PD2-07.
Published: 2018
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11. Melatonin-Secreting Pineal Gland: A Novel Tissue Source for Neural Transplantation Therapy in Stroke

Author: C. V. Borlongan, I. Sumaya, D. Moss, M. Kumazaki, T. Sakurai, H. Hida, and H. Nishino
Subjects: Medicine
Published: 2003
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12. Updated design of the CMB polarization experiment satellite LiteBIRD

Author: H. Sugai, P. A. R. Ade, Y. Akiba, D. Alonso, K. Arnold, J. Aumont, J. Austermann, C. Baccigalupi, A. J. Banday, R. Banerji, R. B. Barreiro, S. Basak, J. Beall, S. Beckman, M. Bersanelli, J. Borrill, F. Boulanger, M. L. Brown, M. Bucher, A. Buzzelli, E. Calabrese, F. J. Casas, A. Challinor, V. Chan, Y. Chinone, J.-F. Cliche, F. Columbro, A. Cukierman, D. Curtis, P. Danto, P. de Bernardis, T. de Haan, M. De Petris, C. Dickinson, M. Dobbs, T. Dotani, L. Duband, A. Ducout, S. Duff, A. Duivenvoorden, J.-M. Duval, K. Ebisawa, T. Elleflot, H. Enokida, H. K. Eriksen, J. Errard, T. Essinger-Hileman, F. Finelli, R. Flauger, C. Franceschet, U. Fuskeland, K. Ganga, J.-R. Gao, R. Génova-Santos, T. Ghigna, A. Gomez, M. L. Gradziel, J. Grain, F. Grupp, A. Gruppuso, J. E. Gudmundsson, N. W. Halverson, P. Hargrave, T. Hasebe, M. Hasegawa, M. Hattori, M. Hazumi, S. Henrot-Versille, D. Herranz, C. Hill, G. Hilton, Y. Hirota, E. Hivon, R. Hlozek, D.-T. Hoang, J. Hubmayr, K. Ichiki, T. Iida, H. Imada, K. Ishimura, H. Ishino, G. C. Jaehnig, M. Jones, T. Kaga, S. Kashima, Y. Kataoka, N. Katayama, T. Kawasaki, R. Keskitalo, A. Kibayashi, T. Kikuchi, K. Kimura, T. Kisner, Y. Kobayashi, N. Kogiso, A. Kogut, K. Kohri, E. Komatsu, K. Komatsu, K. Konishi, N. Krachmalnicoff, C. L. Kuo, N. Kurinsky, A. Kushino, M. Kuwata-Gonokami, L. Lamagna, M. Lattanzi, A. T. Lee, E. Linder, B. Maffei, D. Maino, M. Maki, A. Mangilli, E. Martínez-González, S. Masi, R. Mathon, T. Matsumura, A. Mennella, M. Migliaccio, Y. Minami, K. Mistuda, D. Molinari, L. Montier, G. Morgante, B. Mot, Y. Murata, J. A. Murphy, M. Nagai, R. Nagata, S. Nakamura, T. Namikawa, P. Natoli, S. Nerval, T. Nishibori, H. Nishino, Y. Nomura, F. Noviello, C. O’Sullivan, H. Ochi, H. Ogawa, H. Ohsaki, I. Ohta, N. Okada, L. Pagano, A. Paiella, D. Paoletti, G. Patanchon, F. Piacentini, G. Pisano, G. Polenta, D. Poletti, T. Prouvé, G. Puglisi, D. Rambaud, C. Raum, S. Realini, M. Remazeilles, G. Roudil, J. A. Rubiño-Martín, M. Russell, H. Sakurai, Y. Sakurai, M. Sandri, G. Savini, D. Scott, Y. Sekimoto, B. D. Sherwin, K. Shinozaki, M. Shiraishi, P. Shirron, G. Signorelli, G. Smecher, P. Spizzi, S. L. Stever, R. Stompor, S. Sugiyama, A. Suzuki, J. Suzuki, E. Switzer, R. Takaku, H. Takakura, S. Takakura, Y. Takeda, A. Taylor, E. Taylor, Y. Terao, K. L. Thompson, B. Thorne, M. Tomasi, H. Tomida, N. Trappe, M. Tristram, M. Tsuji, M. Tsujimoto, C. Tucker, J. Ullom, S. Uozumi, S. Utsunomiya, J. Van Lanen, G. Vermeulen, P. Vielva, F. Villa, M. Vissers, N. Vittorio, F. Voisin, I. Walker, N. Watanabe, I. Wehus, J. Weller, B. Westbrook, B. Winter, E. Wollack, R. Yamamoto, N. Y. Yamasaki, M. Yanagisawa, T. Yoshida, J. Yumoto, M. Zannoni, A. Zonca, Sugai, H, Ade, P, Akiba, Y, Alonso, D, Arnold, K, Aumont, J, Austermann, J, Baccigalupi, C, Banday, A, Banerji, R, Barreiro, R, Basak, S, Beall, J, Beckman, S, Bersanelli, M, Borrill, J, Boulanger, F, Brown, M, Bucher, M, Buzzelli, A, Calabrese, E, Casas, F, Challinor, A, Chan, V, Chinone, Y, Cliche, J, Columbro, F, Cukierman, A, Curtis, D, Danto, P, de Bernardis, P, de Haan, T, De Petris, M, Dickinson, C, Dobbs, M, Dotani, T, Duband, L, Ducout, A, Duff, S, Duivenvoorden, A, Duval, J, Ebisawa, K, Elleflot, T, Enokida, H, Eriksen, H, Errard, J, Essinger-Hileman, T, Finelli, F, Flauger, R, Franceschet, C, Fuskeland, U, Ganga, K, Gao, J, Génova-Santos, R, Ghigna, T, Gomez, A, Gradziel, M, Grain, J, Grupp, F, Gruppuso, A, Gudmundsson, J, Halverson, N, Hargrave, P, Hasebe, T, Hasegawa, M, Hattori, M, Hazumi, M, Henrot-Versille, S, Herranz, D, Hill, C, Hilton, G, Hirota, Y, Hivon, E, Hlozek, R, Hoang, D, Hubmayr, J, Ichiki, K, Iida, T, Imada, H, Ishimura, K, Ishino, H, Jaehnig, G, Jones, M, Kaga, T, Kashima, S, Kataoka, Y, Katayama, N, Kawasaki, T, Keskitalo, R, Kibayashi, A, Kikuchi, T, Kimura, K, Kisner, T, Kobayashi, Y, Kogiso, N, Kogut, A, Kohri, K, Komatsu, E, Komatsu, K, Konishi, K, Krachmalnicoff, N, Kuo, C, Kurinsky, N, Kushino, A, Kuwata-Gonokami, M, Lamagna, L, Lattanzi, M, Lee, A, Linder, E, Maffei, B, Maino, D, Maki, M, Mangilli, A, Martínez-González, E, Masi, S, Mathon, R, Matsumura, T, Mennella, A, Migliaccio, M, Minami, Y, Mistuda, K, Molinari, D, Montier, L, Morgante, G, Mot, B, Murata, Y, Murphy, J, Nagai, M, Nagata, R, Nakamura, S, Namikawa, T, Natoli, P, Nerval, S, Nishibori, T, Nishino, H, Nomura, Y, Noviello, F, O’Sullivan, C, Ochi, H, Ogawa, H, Ohsaki, H, Ohta, I, Okada, N, Pagano, L, Paiella, A, Paoletti, D, Patanchon, G, Piacentini, F, Pisano, G, Polenta, G, Poletti, D, Prouvé, T, Puglisi, G, Rambaud, D, Raum, C, Realini, S, Remazeilles, M, Roudil, G, Rubiño-Martín, J, Russell, M, Sakurai, H, Sakurai, Y, Sandri, M, Savini, G, Scott, D, Sekimoto, Y, Sherwin, B, Shinozaki, K, Shiraishi, M, Shirron, P, Signorelli, G, Smecher, G, Spizzi, P, Stever, S, Stompor, R, Sugiyama, S, Suzuki, A, Suzuki, J, Switzer, E, Takaku, R, Takakura, H, Takakura, S, Takeda, Y, Taylor, A, Taylor, E, Terao, Y, Thompson, K, Thorne, B, Tomasi, M, Tomida, H, Trappe, N, Tristram, M, Tsuji, M, Tsujimoto, M, Tucker, C, Ullom, J, Uozumi, S, Utsunomiya, S, Van Lanen, J, Vermeulen, G, Vielva, P, Villa, F, Vissers, M, Vittorio, N, Voisin, F, Walker, I, Watanabe, N, Wehus, I, Weller, J, Westbrook, B, Winter, B, Wollack, E, Yamamoto, R, Yamasaki, N, Yanagisawa, M, Yoshida, T, Yumoto, J, Zannoni, M, Zonca, A, World Premier International Research Center (Japan), Japan Society for the Promotion of Science, Ministry of Education, Culture, Sports, Science and Technology (Japan), Agenzia Spaziale Italiana, Istituto Nazionale di Fisica Nucleare, Centre National D'Etudes Spatiales (France), Centre National de la Recherche Scientifique (France), Commissariat à l'Ènergie Atomique et aux Ènergies Alternatives (France), European Space Agency, Canadian Space Agency, National Aeronautics and Space Administration (US), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National d’Études Spatiales [Paris] (CNES), Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Néel (NEEL), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Sugai, H. [0000-0001-6501-3871], and Apollo - University of Cambridge Repository
Subjects: Passive cooling, Cosmic Microwave Background, Cosmology, Polarimetry, Instrumentation, Inflation, Cosmic microwave background, cosmic background radiation: polarization, 7. Clean energy, 01 natural sciences, Polarization, General Materials Science, 010303 astronomy & astrophysics, media_common, Physics, Settore FIS/01, Settore FIS/05, Astrophysics::Instrumentation and Methods for Astrophysics, suppression, Condensed Matter Physics, Polarization (waves), Atomic and Molecular Physics, and Optics, Infation, adiabatic, Astrophysics - Instrumentation and Methods for Astrophysics, signature, Astrophysics and Astronomy, media_common.quotation_subject, Lagrangian point, Inflation, Primordial gravitational wave, Satellite, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Noise (electronics), Article, NO, FIS/05 - ASTRONOMIA E ASTROFISICA, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, noise: thermal, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), 010308 nuclear & particles physics, Gravitational wave, PE9_14, beam: width, gravitational radiation: primordial, Astronomy, 13. Climate action, Sky, spectral, galaxy, astro-ph.IM
Abstract: H. Sugai, et al., Recent developments of transition-edge sensors (TESs), based on extensive experience in ground-based experiments, have been making the sensor techniques mature enough for their application on future satellite cosmic microwave background (CMB) polarization experiments. LiteBIRD is in the most advanced phase among such future satellites, targeting its launch in Japanese Fiscal Year 2027 (2027FY) with JAXA’s H3 rocket. It will accommodate more than 4000 TESs in focal planes of reflective low-frequency and refractive medium-and-high-frequency telescopes in order to detect a signature imprinted on the CMB by the primordial gravitational waves predicted in cosmic inflation. The total wide frequency coverage between 34 and 448 GHz enables us to extract such weak spiral polarization patterns through the precise subtraction of our Galaxy’s foreground emission by using spectral differences among CMB and foreground signals. Telescopes are cooled down to 5 K for suppressing thermal noise and contain polarization modulators with transmissive half-wave plates at individual apertures for separating sky polarization signals from artificial polarization and for mitigating from instrumental 1/f noise. Passive cooling by using V-grooves supports active cooling with mechanical coolers as well as adiabatic demagnetization refrigerators. Sky observations from the second Sun–Earth Lagrangian point, L2, are planned for 3 years. An international collaboration between Japan, the USA, Canada, and Europe is sharing various roles. In May 2019, the Institute of Space and Astronautical Science, JAXA, selected LiteBIRD as the strategic large mission No. 2., This work was supported by World Premier International Research Center Initiative (WPI), MEXT, Japan, by JSPS Core-to-Core Program, A. Advanced Research Networks, and by JSPS KAKENHI Grant Numbers JP15H05891, JP17H01115, and JP17H01125. The Italian contribution to the LiteBIRD phase A is supported by the Italian Space Agency (ASI Grant No. 2016-24- H.1-2018) and the National Institute for Nuclear Physics (INFN). The French contribution to the LiteBIRD phase A is supported by the Centre National d’Etudes Spatiale (CNES), by the Centre National de la Recherche Scientifque (CNRS), and by the Commissariat à l’Energie Atomique (CEA). A Concurrent Design Facility study focused on the MHFT and Sub-Kelvin coolers has been led by the European Space Agency (ESA). The Canadian contribution to LiteBIRD is supported by the Canadian Space Agency. The US contribution is supported by NASA Grant no. 80NSSC18K0132
Published: 2020
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13. Internal delensing of cosmic microwave background polarization B-modes with the POLARBEAR experiment

Author: Kam Arnold, Grant Teply, D. Leon, R. Stompor, Neil Goeckner-Wald, Yuji Chinone, D. Beck, J. Borrill, H. El Bouhargani, Kevin T. Crowley, S. Takatori, Toshiya Namikawa, M. A. O. Aguilar Faúndez, Max Silva-Feaver, M. Navaroli, Christian L. Reichardt, J. Peloton, Tucker Elleflot, Josquin Errard, Darcy Barron, Davide Poletti, Osamu Tajima, K. Cheung, C. Verges, L. N. Lowry, N. Katayama, Federico Bianchini, Eric V. Linder, Giulio Fabbian, Praween Siritanasak, Yuto Minami, Brian Keating, Julien Carron, L. Howe, Shunsuke Adachi, Tomotake Matsumura, A. T. P. Pham, Y. Segawa, Carlo Baccigalupi, Aamir Ali, Akito Kusaka, Masaya Hasegawa, Frederick Matsuda, Aaron Lee, Chang Feng, Giuseppe Puglisi, Charles A. Hill, T. Fujino, Y. Akiba, D. Tanabe, S. Kikuchi, H. Nishino, Masashi Hazumi, Blake D. Sherwin, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), POLARBEAR, Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Adachi, S, Aguilar Faundez, M, Akiba, Y, Ali, A, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Bianchini, F, Borrill, J, Carron, J, Cheung, K, Chinone, Y, Crowley, K, El Bouhargani, H, Elleflot, T, Errard, J, Fabbian, G, Feng, C, Fujino, T, Goeckner-Wald, N, Hasegawa, M, Hazumi, M, Hill, C, Howe, L, Katayama, N, Keating, B, Kikuchi, S, Kusaka, A, Lee, A, Leon, D, Linder, E, Lowry, L, Matsuda, F, Matsumura, T, Minami, Y, Namikawa, T, Navaroli, M, Nishino, H, Peloton, J, Pham, A, Poletti, D, Puglisi, G, Reichardt, C, Segawa, Y, Sherwin, B, Silva-Feaver, M, Siritanasak, P, Stompor, R, Tajima, O, Takatori, S, Tanabe, D, Teply, G, Verges, C, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), APC - Cosmologie, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmic Microwave Background Polarization, Cosmic microwave background, FOS: Physical sciences, General Physics and Astronomy, cosmic background radiation: polarization, General Relativity and Quantum Cosmology (gr-qc), Gravitation and Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, B-mode: primordial, Settore FIS/05 - Astronomia e Astrofisica, QB0980, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), QC, QB, Physics, Settore FIS/05, Polarization (waves), inflation: model, Computational physics, POLARBEAR Experiment, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Instrumentation and Methods for Astrophysics, Variance reduction, Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Using only cosmic microwave background polarization data from the POLARBEAR experiment, we measure $B$-mode polarization delensing on subdegree scales at more than $5\sigma$ significance. We achieve a 14% $B$-mode power variance reduction, the highest to date for internal delensing, and improve this result to 2% by applying for the first time an iterative maximum a posteriori delensing method. Our analysis demonstrates the capability of internal delensing as a means of improving constraints on inflationary models, paving the way for the optimal analysis of next-generation primordial $B$-mode experiments., Comment: Matches version published in Physical Review Letters
Published: 2019
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14. Deployment of Polarbear-2A

Author: Chang Feng, Radek Stompor, Takayuki Tomaru, Rolando Dünner, Josquin Errard, D. Tanabe, Praween Siritanasak, N. Stebor, Julien Carron, D. Leon, Davide Poletti, K. Cheung, C. Tsai, S. Takakura, Grant Teply, Yuto Minami, Yuki Inoue, Stephen M. Feeney, Yuji Chinone, Frederick Matsuda, D. Beck, Akito Kusaka, Y. Akiba, A. Suzuki, Nicoletta Krachmalnicoff, Adrian T. Lee, M. Aguilar Faúndez, J. Peloton, Colin Ross, Osamu Tajima, D. Boettger, B. Westbrook, A. T. P. Pham, M. Navaroli, N. W. Halverson, Y. Zhou, Federico Bianchini, A. Cukierman, Aashrita Mangu, Nobuhiko Katayama, T. Hamada, Tucker Elleflot, Y. Segawa, Masaya Hasegawa, G. Hall, Julian Borrill, Peter A. R. Ade, Eric V. Linder, Giulio Fabbian, H. Nishino, G. Jaehnig, Giuseppe Puglisi, Charles A. Hill, Shunsuke Adachi, S. Takatori, L. Howe, A. J. Gilbert, H. El-Bouhargani, Christian L. Reichardt, Kam Arnold, John Groh, Masashi Hazumi, Neil Goeckner-Wald, Nicholas Galitzki, S. Beckman, Brian Keating, M. A. Dobbs, Carlo Baccigalupi, Clara Vergès, Theodore Kisner, Reijo Keskitalo, Daisuke Kaneko, T. Fujino, S. Kikuchi, Darcy Barron, L. N. Lowry, Scott Chapman, Maximiliano Silva-Feaver, Oliver Jeong, Kevin T. Crowley, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Kaneko, D, Adachi, S, Ade, P, Aguilar Faundez, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Beckman, S, Bianchini, F, Boettger, D, Borrill, J, Carron, J, Chapman, S, Cheung, K, Chinone, Y, Crowley, K, Cukierman, A, Dobbs, M, Dunner, R, El-Bouhargani, H, Elleflot, T, Errard, J, Fabbian, G, Feeney, S, Feng, C, Fujino, T, Galitzki, N, Gilbert, A, Goeckner-Wald, N, Groh, J, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hazumi, M, Hill, C, Howe, L, Inoue, Y, Jaehnig, G, Jeong, O, Katayama, N, Keating, B, Keskitalo, R, Kikuchi, S, Kisner, T, Krachmalnicoff, N, Kusaka, A, Lee, A, Leon, D, Linder, E, Lowry, L, Mangu, A, Matsuda, F, Minami, Y, Navaroli, M, Nishino, H, Peloton, J, Pham, A, Poletti, D, Puglisi, G, Reichardt, C, Ross, C, Segawa, Y, Silva-Feaver, M, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Takatori, S, Tanabe, D, Teply, G, Tomaru, T, Tsai, C, Verges, C, Westbrook, B, Zhou, Y, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: [PHYS]Physics [physics], Settore FIS/05, Gravitational wave, Cosmic microwave background, Millimeter wave, First light, CMB, Condensed Matter Physics, 7. Clean energy, 01 natural sciences, Atomic and Molecular Physics, and Optics, 010305 fluids & plasmas, Microwave emission, Settore FIS/05 - Astronomia e Astrofisica, TES bolometer, Planet, Software deployment, 0103 physical sciences, Extremely high frequency, B-mode polarization, General Materials Science, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Remote sensing
Abstract: International audience; Polarbear-2A is the first of three receivers in the Simons array, a cosmic microwave background experiment located on the Atacama Plateau in Chile. Polarbear-2A was deployed and achieved the first light in January 2019 by mapping the microwave emission from planet observations. Commissioning work is underway to prepare the receiver for science observations.
Published: 2019
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15. LiteBIRD: A Satellite for the Studies of B-Mode Polarization and Inflation from Cosmic Background Radiation Detection

Author: Josquin Errard, Kent D. Irwin, Ingunn Kathrine Wehus, Kazunori Kohri, Kam Arnold, Atsushi Okamoto, Osamu Tajima, T. Tomida, Hirokazu Ishino, L. Montier, T. Kawasaki, M. Willer, Ryo Yamamoto, Nobuhiko Katayama, B. Thorne, Eiichiro Komatsu, Takayuki Tomaru, Benjamin Westbrook, Toshiaki Iida, Tadayasu Dotani, Yuki Inoue, T. Funaki, Chiko Otani, Bruno Maffei, L. Hayes, Charles A. Hill, F. Vansyngel, T. Nagasaki, L. Duband, Tucker Elleflot, H. Imada, Johannes Hubmayr, A. Cukierman, M. Nakajima, T. Hasebe, Paul Turin, A. Dominjon, Eric V. Linder, S. Takatori, Toshifumi Shimizu, Yuto Minami, Shin Utsunomiya, Y. Sato, Yoshinori Uzawa, D. Tanabe, J. M. Duval, F. Boulanger, Takahiro Okamura, Jo Dunkley, Hiroyuki Sugita, Masato Naruse, Julian Borrill, Makoto Hattori, Theodore Kisner, Yuji Chinone, Tom Nitta, Dale Li, Mathieu Remazeilles, K. Ganga, Hideo Ogawa, Reijo Keskitalo, Masashi Hazumi, Giampaolo Pisano, E. Taylor, S. Takakura, H. Kanai, Jun-ichi Suzuki, N. Sato, Masahiro Tsujimoto, Yutaro Sekimoto, Shin-ichiro Sakai, Kimihiro Kimura, M. Nagai, N. W. Halverson, Anna Mangilli, Seongjae Cho, M. Tristram, S. A. Kernasovskiy, Jonathan Aumont, Blake D. Sherwin, Carole Tucker, Tomotake Matsumura, Kiyotomo Ichiki, Satoru Mima, T. de Haan, T. Hamada, N. Tomita, G. Patanchon, K. Komatsu, Shuji Matsuura, J. Grain, Paul L. Richards, Norio Okada, N. Hidehira, Kazuhisa Mitsuda, Soumen Basak, Yasuhiro Yamada, Aritoki Suzuki, H. K. Eriksen, Hajime Sugai, Shogo Nakamura, Peter A. R. Ade, Alex Lazarian, T. Fujino, Y. Akiba, Gabriel M. Rebeiz, H. Nishino, Nathan Whitehorn, Martin Bucher, R. Stompor, Shingo Kashima, A. Kibayashi, Y. Kida, Noah Kurinsky, D. W. Curtis, M. Inoue, Masaya Hasegawa, Adrian T. Lee, Shugo Oguri, Y. Segawa, David Alonso, A. Ducout, Carlo Baccigalupi, U. Fuskeland, S. Beckman, Uroš Seljak, R. Nagata, J. Fischer, Mitsuhiro Yoshida, K. L. Thompson, Darcy Barron, Gene C. Hilton, Noriko Y. Yamasaki, Erminia Calabrese, Neil Goeckner-Wald, R. Takaku, Suguru Takada, M. A. Dobbs, Oliver Jeong, Toshiya Namikawa, Yuki Sakurai, Chao-Lin Kuo, Kaori Hattori, Keisuke Shinozaki, D. Meilhan, M. Maki, Makoto Sawada, D. Kaneko, T. Yamashita, S. Uozumi, Takashi Noguchi, Akito Kusaka, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Service des Basses Températures (SBT ), Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire des Cryoréfrigérateurs et Cryogénie Spatiale (LCCS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: detector: cryogenics, Cosmic microwave background, Cosmic background radiation, cosmic background radiation: polarization, Lagrangian point, B-mode polarization, Cosmic inflation, Primordial gravitational wave, Quantum gravity, Satellite, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, 010305 fluids & plasmas, law.invention, Telescope, Settore FIS/05 - Astronomia e Astrofisica, bolometer, law, 0103 physical sciences, General Materials Science, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], detector: optical, 010306 general physics, Physics, Bolometer, gravitational radiation: primordial, Astrophysics::Instrumentation and Methods for Astrophysics, Condensed Matter Physics, Polarization (waves), inflation: model, Atomic and Molecular Physics, and Optics, detector: sensitivity, modulation, Cardinal point, B-mode, angular resolution, moment: multipole, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Multipole expansion
Abstract: 著者人数: 152名(所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 羽澄, 昌史; 堂谷, 忠靖; 長谷部, 孝; 今田, 大皓; 満田, 和久; 坂井, 真一郎; 関本, 裕太郎; Tomida, T.; 辻本, 匡弘; Yamamoto, R.; 山崎, 典子), Accepted: 2019-01-18, 資料番号: SA1180402000
Published: 2019
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16. Reducing inspection time of active thermographic non-destructive testing based on thermal wave theory

Author: M. Ishikawa, M. Koyama, H. Kasano, R. Fukui, H. Hatta, S. Utsunomiya, and H. Nishino
Published: 2019
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17. A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND B-MODE POLARIZATION WITH POLARBEAR

Author: X. Meng, N. W. Halverson, P. Hyland, M. J. Myers, Nathan Miller, Daniel Flanigan, M. Atlas, A. E. Anthony, Josquin Errard, D. Poletti, Kam Arnold, M. Navaroli, R. Keskitalo, Zigmund Kermish, A. J. Gilbert, J. Borrill, Masashi Hazumi, M. A. Dobbs, Hans P. Paar, T. Matsumura, Yuji Chinone, E. Quealy, G. Fabbian, H. Morii, Peter A. R. Ade, M. Le Jeune, Brian Keating, Y. Akiba, Jonathon Howard, Scott Chapman, Tucker Elleflot, S. Moyerman, William F. Grainger, W. L. Holzapfel, Gabriel M. Rebeiz, Masaya Hasegawa, J. Peloton, Eric V. Linder, Theodore Kisner, Kaori Hattori, E. M. Leitch, Marius Lungu, Frederick Matsuda, Y. Hori, Angelo Orlando, Darcy Barron, Yuki Inoue, H. Nishino, A. T. Lee, G. Jaehnig, Chang Feng, Andrew H. Jaffe, and D. Boettger
Subjects: Physics, Gravitational wave, Bolometer, Cosmic microwave background, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic background radiation, Astronomy, Spectral density, Astrophysics::Cosmology and Extragalactic Astrophysics, General Medicine, Astrophysics, Polarization (waves), law.invention, Gravitational lens, law, Transition edge sensor
Abstract: Polarbear is a ground-based experiment located in the Atacama desert of northern Chile. The experiment is designed to measure the Cosmic Microwave Background B-mode polarization at several arcminute resolution. The CMB B-mode polarization on degree angular scales is a unique signature of primordial gravitational waves from cosmic inflation and B-mode signal on sub-degree scales is induced by the gravitational lensing from large-scale structure. Science observations began in early 2012 with an array of 1, 274 polarization sensitive antenna-couple Transition Edge Sensor (TES) bolometers at 150 GHz. We published the first CMB-only measurement of the B-mode polarization on sub-degree scales induced by gravitational lensing in December 2013 followed by the first measurement of the B-mode power spectrum on those scales in March 2014. In this proceedings, we review the physics of CMB B-modes and then describe the Polarbear experiment, observations, and recent results.
Published: 2015
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18. Concept design of the LiteBIRD satellite for CMB B-mode polarization

Author: A. Cukierman, Makoto Hattori, Alessandro Gruppuso, Y. Kataoka, D. T. Hoang, Kam Arnold, Tucker Elleflot, Benjamin Westbrook, Eric V. Linder, Johannes Hubmayr, Toshiyuki Nishibori, Christopher Raum, T. Kikuchi, Luca Lamagna, S. Takakura, Shingo Kashima, Ryota Takaku, Ken Ganga, N. Katayama, Masahiro Tsujimoto, Yutaro Sekimoto, A. Kibayashi, Hajime Sugai, H. K. Eriksen, Noah Kurinsky, F. Columbro, Gianluca Morgante, Toshiya Namikawa, Yuki Sakurai, B. Mot, E. Martínez-González, H. Nishino, G. Jaehnig, Hiroyuki Ohsaki, Shogo Nakamura, Peter A. R. Ade, L. Montier, T. Kawasaki, Giuseppe Puglisi, Charles A. Hill, H. Takakura, Masaaki Nagai, Anna Murphy, D. W. Curtis, M. Tristram, Adrian T. Lee, J. Grain, S. Realini, H. Ochi, Peter Charles Hargrave, Theodore Kisner, Maresuke Shiraishi, F. Boulanger, Y. Kobayashi, M. Tomasi, G. Signorelli, Y. Hirota, M. Tsuji, Graeme Smecher, F. Piacentini, K. Ebisawa, S. Beckman, Carlo Baccigalupi, E. Hivon, K. Mistuda, Haruyuki Sakurai, Soumen Basak, C. L. Kuo, G. Patanchon, Ingunn Kathrine Wehus, Masashi Hazumi, J. Aumont, Berend Winter, I. S. Ohta, Reijo Keskitalo, Bruno Maffei, Ryo Yamamoto, Marco Bersanelli, Mario Zannoni, P. Natoli, Junji Yumoto, Andrea Zonca, Erminia Calabrese, A. Ducout, Blake D. Sherwin, N. Trappe, U. Fuskeland, Nicoletta Krachmalnicoff, K. L. Thompson, M. A. Dobbs, F. Noviello, Anna Mangilli, Jun-ichi Suzuki, A. Kushino, Tadayasu Dotani, S. Sugiyama, H. Kanai, T. Yoshida, Silvia Masi, G. Polenta, M. Yanagisawa, N. Watanabe, R. Nagata, J. Austermann, Keisuke Shinozaki, Yasunori Terao, Davide Poletti, Cristian Franceschet, Michael L. Brown, Anthony Challinor, M. De Petris, Masaya Hasegawa, Yuto Minami, Noriko Y. Yamasaki, L. Duband, Créidhe O'Sullivan, Yasuhiro Murata, J. R. Gao, B. Thorne, Eiichiro Komatsu, P. de Bernardis, Kazunori Kohri, Hirokazu Ishino, Kuniaki Konishi, A. J. Banday, N. W. Halverson, A. Mennella, Kiyotomo Ichiki, T. Hasebe, Giorgio Savini, Julian Borrill, Yuji Chinone, Mathieu Remazeilles, Giampaolo Pisano, D. Molinari, Radek Stompor, M. Maki, H. Tomida, N. Okada, H. Imada, S. Uozumi, Nozomu Kogiso, R. Banerji, Tomotake Matsumura, Raphael Flauger, T. Ghigna, Josquin Errard, Shin Utsunomiya, M. Bucher, K. Komatsu, Hideo Ogawa, E. Taylor, Kimihiro Kimura, Sophie Henrot-Versille, Nicola Vittorio, Aritoki Suzuki, Realini, S, Patanchon, G, Kataoka, Y, Zonca, A, Zannoni, M, Yumoto, J, Yoshida, T, Yanagisawa, M, Yamasaki, N, Yamamoto, R, Westbrook, B, Wehus, I, Watanabe, N, Vittorio, N, Utsunomiya, S, Uozumi, S, Tsujimoto, M, Tsuji, M, Tristram, M, Trappe, N, Tomida, H, Tomasi, M, Thorne, B, Thompson, K, Terao, Y, Taylor, E, Takakura, S, Takakura, H, Takaku, R, Suzuki, J, Suzuki, A, Sugiyama, S, Sugai, H, Stompor, R, Smecher, G, Signorelli, G, Shiraishi, M, Shinozaki, K, Sherwin, B, Savini, G, Sakurai, Y, Sakurai, H, Remazeilles, M, Raum, C, Puglisi, G, Poletti, D, Polenta, G, Pisano, G, Piacentini, F, Okada, N, Ohsaki, H, Ogawa, H, Ochi, H, O'Sullivan, C, Nishino, H, Nishibori, T, Natoli, P, Namikawa, T, Nakamura, S, Nagata, R, Nagai, M, Murphy, A, Murata, Y, Mot, B, Morgante, G, Montier, L, Molinari, D, Mitsuda, K, Minami, Y, Mennella, A, Matsumura, T, Masi, S, Martinez-Gonzalez, E, Maki, M, Maffei, B, Linder, E, Lee, A, Lamagna, L, Kushino, A, Kurinsky, N, Kuo, C, Krachmalnicoff, N, Konishi, K, Komatsu, K, Komatsu, E, Kohri, K, Kogiso, N, Kobayashi, Y, Kisner, T, Kimura, K, Kikuchi, T, Kibayashi, A, Keskitalo, R, Kawasaki, T, Katayama, N, Kashima, S, Kanai, H, Arnold, K, Jaehnig, G, Ishino, H, Imada, H, Ichiki, K, Hubmayr, J, Hoang, D, Hivon, E, Hirota, Y, Hill, C, Henrot-Versille, S, Hazumi, M, Hattori, M, Hasegawa, M, Hasebe, T, Hargrave, P, Halverson, N, Gruppuso, A, Grain, J, Ghigna, T, Gao, J, Ganga, K, Fuskeland, U, Franceschet, C, Flauger, R, Errand, J, Eriksen, H, Elleflot, T, Ebisawa, K, Ducout, A, Duband, L, Dotani, T, Dobbs, M, de Petris, M, de Bernardis, P, Curtis, D, Cukierman, A, Columbro, F, Chinone, Y, Challinor, A, Calabrese, E, Bucher, M, Brown, M, Boulanger, F, Borill, J, Bersanelli, M, Beckman, S, Basak, S, Banerji, R, Banday, A, Baccigalupi, C, Austermann, J, Aumont, J, Mangilli, A, Ade, P, Winter, B, Ota, I, Noviello, F, Sekimoto, Y, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Service des Basses Températures (SBT ), Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), and LiteBIRD
Subjects: Cosmic microwave background, Cryogenic telescope, Millimeter-wave polarization, Space program, Electronic, Optical and Magnetic Materials, Condensed Matter Physics, Computer Science Applications1707 Computer Vision and Pattern Recognition, Applied Mathematics, Electrical and Electronic Engineering, media_common.quotation_subject, satellite, Lagrangian point, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, frequency: high, law.invention, NO, Telescope, cosmic background radiation: B-mode, FIS/05 - ASTRONOMIA E ASTROFISICA, Settore FIS/05 - Astronomia e Astrofisica, law, 0103 physical sciences, Electronic, Cosmology, Cosmic Microwave Background, CMB, Polarimetry, Inflation, Instrumentation, structure, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Optical and Magnetic Materials, 010306 general physics, Astrophysics::Galaxy Astrophysics, media_common, Physics, polarization, 010308 nuclear & particles physics, Gravitational wave, Settore FIS/05, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Polarization (waves), sensitivity, Superconducting detectors, frequency: low, angular resolution, Sky, cryogenics, Launch vehicle, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: LiteBIRD is a candidate for JAXA’s strategic large mission to observe the cosmic microwave background (CMB) polarization over the full sky at large angular scales. It is planned to be launched in the 2020s with an H3 launch vehicle for three years of observations at a Sun-Earth Lagrangian point (L2). The concept design has been studied by researchers from Japan, U.S., Canada and Europe during the ISAS Phase-A1. Large scale measurements of the CMB B-mode polarization are known as the best probe to detect primordial gravitational waves. The goal of LiteBIRD is to measure the tensor-to-scalar ratio (r) with precision of δr < 0.001. A 3-year full sky survey will be carried out with a low frequency (34 - 161 GHz) telescope (LFT) and a high frequency (89 - 448 GHz) telescope (HFT), which achieve a sensitivity of 2.5 µK-arcmin with an angular resolution of ∼ 30 arcminutes around 100 GHz. The concept design of LiteBIRD system, payload module (PLM), cryo-structure, LFT and verification plan is described in this paper. © 2018 Society of Photo-Optical Instrumentation Engineers (SPIE)
Published: 2018
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19. The LiteBIRD Satellite Mission: Sub-Kelvin Instrument

Author: A. Suzuki, P. A. R. Ade, Y. Akiba, D. Alonso, K. Arnold, J. Aumont, C. Baccigalupi, D. Barron, S. Basak, S. Beckman, J. Borrill, F. Boulanger, M. Bucher, E. Calabrese, Y. Chinone, S. Cho, B. Crill, A. Cukierman, D. W. Curtis, T. de Haan, M. Dobbs, A. Dominjon, T. Dotani, L. Duband, A. Ducout, J. Dunkley, J. M. Duval, T. Elleflot, H. K. Eriksen, J. Errard, J. Fischer, T. Fujino, T. Funaki, U. Fuskeland, K. Ganga, N. Goeckner-Wald, J. Grain, N. W. Halverson, T. Hamada, T. Hasebe, M. Hasegawa, K. Hattori, M. Hattori, L. Hayes, M. Hazumi, N. Hidehira, C. A. Hill, G. Hilton, J. Hubmayr, K. Ichiki, T. Iida, H. Imada, M. Inoue, Y. Inoue, K. D. Irwin, H. Ishino, O. Jeong, H. Kanai, D. Kaneko, S. Kashima, N. Katayama, T. Kawasaki, S. A. Kernasovskiy, R. Keskitalo, A. Kibayashi, Y. Kida, K. Kimura, T. Kisner, K. Kohri, E. Komatsu, K. Komatsu, C. L. Kuo, N. A. Kurinsky, A. Kusaka, A. Lazarian, A. T. Lee, D. Li, E. Linder, B. Maffei, A. Mangilli, M. Maki, T. Matsumura, S. Matsuura, D. Meilhan, S. Mima, Y. Minami, K. Mitsuda, L. Montier, M. Nagai, T. Nagasaki, R. Nagata, M. Nakajima, S. Nakamura, T. Namikawa, M. Naruse, H. Nishino, T. Nitta, T. Noguchi, H. Ogawa, S. Oguri, N. Okada, A. Okamoto, T. Okamura, C. Otani, G. Patanchon, G. Pisano, G. Rebeiz, M. Remazeilles, P. L. Richards, S. Sakai, Y. Sakurai, Y. Sato, N. Sato, M. Sawada, Y. Segawa, Y. Sekimoto, U. Seljak, B. D. Sherwin, T. Shimizu, K. Shinozaki, R. Stompor, H. Sugai, H. Sugita, J. Suzuki, O. Tajima, S. Takada, R. Takaku, S. Takakura, S. Takatori, D. Tanabe, E. Taylor, K. L. Thompson, B. Thorne, T. Tomaru, T. Tomida, N. Tomita, M. Tristram, C. Tucker, P. Turin, M. Tsujimoto, S. Uozumi, S. Utsunomiya, Y. Uzawa, F. Vansyngel, I. K. Wehus, B. Westbrook, M. Willer, N. Whitehorn, Y. Yamada, R. Yamamoto, N. Yamasaki, T. Yamashita, M. Yoshida, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Service des Basses Températures (SBT ), Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire des Cryoréfrigérateurs et Cryogénie Spatiale (LCCS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Sorbonne Université (SU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: Cosmic microwave background, FOS: Physical sciences, cosmic background radiation: polarization, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Radio spectrum, law.invention, Antenna array, Telescope, Optics, bolometer, Settore FIS/05 - Astronomia e Astrofisica, law, Polarization, 0103 physical sciences, B-mode, Inflation, Satellite, General Materials Science, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, activity report, detector: design, Physics, 010308 nuclear & particles physics, business.industry, Gravitational wave, Detector, Bolometer, Astrophysics::Instrumentation and Methods for Astrophysics, Condensed Matter Physics, Astrophysics - Astrophysics of Galaxies, Atomic and Molecular Physics, and Optics, cryogenics, Astrophysics of Galaxies (astro-ph.GA), electronics: readout, interference: quantum, Transition edge sensor, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], business, cosmic background radiation: anisotropy
Abstract: 著者人数: 153名（所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 堂谷, 忠靖; 羽澄, 昌史; 今田, 大皓; 満田, 和久; 坂井, 真一郎; Tomida, T.; 辻本, 匡弘; Yamamoto, R.; 山崎, 典子）, Accepted: 2018-04-30, 資料番号: SA1180210000
Published: 2018
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20. The POLARBEAR-2 and Simons Array Focal Plane Fabrication Status

Author: Adrian T. Lee, Neil Goeckner-Wald, D. Beck, D. Leon, A. Cukierman, M. Navaroli, Brian Keating, Y. Segawa, Tucker Elleflot, Masaya Hasegawa, Maximiliano Silva-Feaver, Peter A. R. Ade, Y. Akiba, Matt Dobbs, Julian Borrill, Paul L. Richards, Stephen M. Feeney, Rolando Dünner, K. M. Rotermund, C. Tsai, Oliver Jeong, Osamu Tajima, A. T. P. Pham, Eric V. Linder, Gabriel M. Rebeiz, Josquin Errard, S. Takakura, D. Plambeck, Lucio Piccirillo, Nathan Whitehorn, Yuji Chinone, S. Beckman, Giulio Fabbian, L. Howe, M. Le Jeune, Federico Bianchini, Christopher Raum, Daisy Mak, Grant Teply, W. L. Holzapfel, Andrew May, Joshua Montgomery, Carlo Baccigalupi, H. Roberts, S. Takatori, Christian L. Reichardt, Reijo Keskitalo, A. J. Gilbert, Gary A. Fuller, R. Tat, Akito Kusaka, Nobuhiko Katayama, D. Boettger, A. Tikhomirov, John Groh, Benjamin Westbrook, Giuseppe Puglisi, Charles A. Hill, Scott Chapman, Nicoletta Krachmalnicoff, Colin Ross, Amy N. Bender, A. Madurowicz, Darcy Barron, J. Peloton, N. W. Halverson, L. N. Lowry, Aritoki Suzuki, Chang Feng, Andrew H. Jaffe, Takayuki Tomaru, Davide Poletti, A. Zahn, Radek Stompor, Mario Ferrada Aguilar, Theodore Kisner, T. de Haan, T. Hamada, Gabriele Coppi, Yuto Minami, Yuki Inoue, Nathan J. Miller, D. Tanabe, H. Nishino, G. Jaehnig, Masashi Hazumi, Nicholas Galitzki, Blake D. Sherwin, Kevin D. Crowley, Kam Arnold, Frederick Matsuda, D. Kaneko, Praween Siritanasak, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Westbrook, B, Ade, P, Aguilar, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Beckman, S, Bender, A, Bianchini, F, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Coppi, G, Crowley, K, Cukierman, A, de Haan, T, Dunner, R, Dobbs, M, Elleflot, T, Errard, J, Fabbian, G, Feeney, S, Feng, C, Fuller, G, Galitzki, N, Gilbert, A, Goeckner-Wald, N, Groh, J, Halverson, N, Hamada, T, Hasegawa, M, Hazumi, M, Hill, C, Holzapfel, W, Howe, L, Inoue, Y, Jaehnig, G, Jaffe, A, Jeong, O, Kaneko, D, Katayama, N, Keating, B, Keskitalo, R, Kisner, T, Krachmalnicoff, N, Kusaka, A, Le Jeune, M, Lee, A, Leon, D, Linder, E, Lowry, L, Madurowicz, A, Mak, D, Matsuda, F, May, A, Miller, N, Minami, Y, Montgomery, J, Navaroli, M, Nishino, H, Peloton, J, Pham, A, Piccirillo, L, Plambeck, D, Poletti, D, Puglisi, G, Raum, C, Rebeiz, G, Reichardt, C, Richards, P, Roberts, H, Ross, C, Rotermund, K, Segawa, Y, Sherwin, B, Silva-Feaver, M, Siritanasak, P, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Takatori, S, Tanabe, D, Tat, R, Teply, G, Tikhomirov, A, Tomaru, T, Tsai, C, Whitehorn, N, Zahn, A, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)
Subjects: Cosmic microwave background, cosmic background radiation: polarization, CMB, Dichroic glass, 01 natural sciences, law.invention, law, Atomic and Molecular Physics, Polarization, General Materials Science, silicon: nitrogen, Instrumentation, Mathematical Physics, 010302 applied physics, Physics, Settore FIS/05, superconductivity, Detector, Detectors, Polarization (waves), Condensed Matter Physics, Atomic and Molecular Physics, and Optics, Cardinal point, Materials Science (all), silicon: oxygen, Astrophysics - Instrumentation and Methods for Astrophysics, Transition edge sensor, performance, Astrophysics - Cosmology and Nongalactic Astrophysics, Fabrication, Sinuous antenna, Inflation, General Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Classical Physics, FOS: Physical sciences, Telescope, Optics, Settore FIS/05 - Astronomia e Astrofisica, bolometer, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), detector: design, activity report, business.industry, Bolometer, and Optics, business
Abstract: 著者人数: 93名（所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 羽澄, 昌史), Accepted: 2018-08-27, 資料番号: SA1180208000
Published: 2017
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21. Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD

Author: D. W. Curtis, M. Nakajima, T. Funaki, R. Takaku, Yoshinori Uzawa, Carlo Baccigalupi, Johannes Hubmayr, U. Fuskeland, Theodore Kisner, S. Beckman, Anna Mangilli, Erminia Calabrese, Neil Goeckner-Wald, Uroš Seljak, M. Nagai, N. Katayama, Jonathan Aumont, Carole Tucker, Suguru Takada, Shin Utsunomiya, Kazunori Kohri, R. Nagata, Kam Arnold, M. Bucher, A. Dominjon, N. Sato, M. A. Dobbs, Shin-ichiro Sakai, Darcy Barron, Gene C. Hilton, H. K. Eriksen, Yasuhiro Yamada, Oliver Jeong, Aritoki Suzuki, Atsushi Okamoto, Tadayasu Dotani, T. Tomida, D. Meilhan, L. Duband, S. A. Kernasovskiy, S. Takakura, S. Takatori, R. Stompor, A. Ducout, B. Thorne, Eiichiro Komatsu, Hajime Sugai, Keisuke Shinozaki, N. Tomita, J. Fischer, Yuji Chinone, C. L. Kuo, L. Montier, Akito Kusaka, Toshiaki Iida, Aaron Lee, Yuki Inoue, Makoto Sawada, Ingunn Kathrine Wehus, L. Hayes, Mitsuhiro Yoshida, K. L. Thompson, H. Nishino, Mathieu Remazeilles, Tomotake Matsumura, Shugo Oguri, K. Komatsu, Reijo Keskitalo, T. Yamashita, T. Kawasaki, Takahiro Okamura, Masashi Hazumi, Osamu Tajima, Takayuki Tomaru, G. Patanchon, M. Tristram, Giampaolo Pisano, Hirokazu Ishino, Masato Naruse, Jun-ichi Suzuki, H. M. Cho, Paul Turin, Toshiya Namikawa, Yuki Sakurai, Y. Kida, Blake D. Sherwin, J. Grain, Chiko Otani, Noriko Y. Yamasaki, N. W. Halverson, Shuji Matsuura, S. Uozumi, Takashi Noguchi, T. Nagasaki, H. Imada, M. Willer, Y. Sato, M. Inoue, J. M. Duval, Bruno Maffei, Toshifumi Shimizu, Yuto Minami, F. Boulanger, Tucker Elleflot, Charles A. Hill, Benjamin Westbrook, Shogo Nakamura, Peter A. R. Ade, Kaori Hattori, Paul L. Richards, Alex Lazarian, Y. Segawa, Julian Borrill, Ryo Yamamoto, Kiyotomo Ichiki, M. Maki, Satoru Mima, D. Tanabe, Jo Dunkley, Kazuhisa Mitsuda, Soumen Basak, Gabriel M. Rebeiz, Tom Nitta, T. de Haan, T. Hamada, H. Kanai, K. Ganga, Hideo Ogawa, D. Kaneko, A. Cukierman, Nathan Whitehorn, Eric V. Linder, Masaya Hasegawa, Josquin Errard, Kimihiro Kimura, Hiroyuki Sugita, David Alonso, T. Hasebe, Kent D. Irwin, E. Taylor, Norio Okada, N. Hidehira, Shingo Kashima, A. Kibayashi, Noah Kurinsky, T. Fujino, Y. Akiba, Makoto Hattori, Dale Li, Masahiro Tsujimoto, Yutaro Sekimoto, F. Vansyngel, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Electronique et des Technologies de l'Information (CEA-LETI), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Service des Basses Températures (SBT ), Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Laboratoire des Cryoréfrigérateurs et Cryogénie Spatiale (LCCS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Université Grenoble Alpes (UGA)-Direction de Recherche Technologique (CEA) (DRT (CEA))
Subjects: Cosmic microwave background radiation, Inflation, Satellite, Telescope, Silicon, Cosmic microwave background, chemistry.chemical_element, engineering.material, 01 natural sciences, law.invention, 010309 optics, Optics, Settore FIS/05 - Astronomia e Astrofisica, Coating, law, 0103 physical sciences, General Materials Science, Sensitivity (control systems), [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Physics, business.industry, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, Lens (optics), chemistry, engineering, Reflection (physics), business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: 著者人数: 152名（所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 長谷部, 孝; 堂谷, 忠靖; 羽澄, 昌史; 今田, 大皓; 満田, 和久; 坂井, 真一郎; 関本, 裕太郎; Tomida, T.; 辻本, 匡弘; Yamamoto, R.; 山崎, 典子), Accepted: 2018-04-07, 資料番号: SA1180209000
Published: 2017
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22. Cross-correlation of CMB Polarization Lensing with High-z Submillimeter Herschel-ATLAS Galaxies

Author: Grant Teply, Masashi Hazumi, Tucker Elleflot, Nicholas Galitzki, D. Beck, Akito Kusaka, Carlo Baccigalupi, Blake D. Sherwin, Nicoletta Krachmalnicoff, Christian L. Reichardt, Clara Vergès, Eric V. Linder, Giulio Fabbian, Giuseppe Puglisi, L. Howe, Hamza El Bouhargani, Osamu Tajima, Neil Goeckner-Wald, D. Boettger, M. Navaroli, Kam Arnold, K. Cheung, MA Faúndez, Josquin Errard, D. Leon, Julien Carron, S. Takakura, Masaya Hasegawa, Radek Stompor, N. Katayama, Brian Keating, Atp Pham, Federico Bianchini, Darcy Barron, L. N. Lowry, C. Tsai, H. Nishino, Chang Feng, Max Silva-Feaver, A. Suzuki, Julian Borrill, Frederick Matsuda, Aaron Lee, Yuji Chinone, D. Kaneko, S. Takatori, Davide Poletti, Yuto Minami, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Faundez, M, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Bianchini, F, Boettger, D, Borrill, J, Carron, J, Cheung, K, Chinone, Y, Bouhargani, H, Elleflot, T, Errard, J, Fabbian, G, Feng, C, Galitzki, N, Goeckner-Wald, N, Hasegawa, M, Hazumi, M, Howe, L, Kaneko, D, Katayama, N, Keating, B, Krachmalnicoff, N, Kusaka, A, Lee, A, Leon, D, Linder, E, Lowry, L, Matsuda, F, Minami, Y, Navaroli, M, Nishino, H, Pham, A, Poletti, D, Puglisi, G, Reichardt, C, Sherwin, B, Silva-Feaver, M, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Takatori, S, Teply, G, Tsai, C, Verges, C, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Polarbear
Subjects: QB991.L37, Cosmic microwave background radiation (322), 010504 meteorology & atmospheric sciences, astro-ph.GA, Cosmic microwave background, Large-scale structure of the universe (902), Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Astronomy & Astrophysics, Atomic, Physical Chemistry, 01 natural sciences, Cosmology, QB0460, Particle and Plasma Physics, Settore FIS/05 - Astronomia e Astrofisica, QB0980, 0103 physical sciences, cosmic background radiation: polarization, cosmic background radiation: temperature, error: statistical, halo: mass, galaxy, redshift: dependence, lens, cosmic background radiation: power spectrum, Nuclear, 10. No inequality, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, polarization lensing, ComputingMilieux_MISCELLANEOUS, Weak gravitational lensing, QB, 0105 earth and related environmental sciences, [PHYS]Physics [physics], Physics, Settore FIS/05, Astrophysics::Instrumentation and Methods for Astrophysics, Molecular, Spectral density, Astronomy and Astrophysics, Polarization (waves), Redshift, Galaxy, Weak gravitational lensing (1797), Space and Planetary Science, High-redshift galaxies (734), astro-ph.CO, Halo, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Cosmology (343), Astronomical and Space Sciences, Physical Chemistry (incl. Structural)
Abstract: 著者人数: 48名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 羽澄, 昌史), Number of authors: 48 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Hazumi, Masashi), Accepted: 2019-09-26, 資料番号: SA1190160000
Published: 2019
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23. The POLARBEAR-2 Experiment

Author: Kam Arnold, W. Holzapfel, Tomotake Matsumura, M. Sholl, R. Stompor, N. W. Halverson, M. Atlas, Guangyuan Feng, N. Katayama, Masashi Hazumi, Colin Ross, H. Yamaguchi, Y. Akiba, Kaja Rotermund, Praween Siritanasak, Tucker Elleflot, S. Takakura, J. Borrill, Paul L. Richards, Jun-ichi Suzuki, Giulio Fabbian, O. Zahn, H. Morii, H. Nishino, G. Jaehnig, Josquin Errard, Reijo Keskitalo, Y. Hori, A. Cukierman, Scott Chapman, Takahiro Okamura, Kaori Hattori, Frederick Matsuda, Yuki Inoue, Brian Keating, C. Reichart, Yuji Chinone, Aritoki Suzuki, Suguru Takada, M. A. Dobbs, Graeme Smecher, William F. Grainger, A. J. Gilbert, Takayuki Tomaru, B. Wilson, C. Aleman, Darcy Barron, S. Moyerman, Nathan Stebor, Masaya Hasegawa, Adrian T. Lee, Theodore Kisner, M. Myers, M. Navaroli, Zigmund Kermish, and Peter A. R. Ade
Subjects: Physics, Gravitational wave, business.industry, Cosmic microwave background, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Condensed Matter Physics, Polarization (waves), Noise-equivalent temperature, Atomic and Molecular Physics, and Optics, Computational physics, symbols.namesake, Gravitational lens, Optics, symbols, General Materials Science, Planck, Neutrino, Transition edge sensor, business
Abstract: We present an overview of the design and development of the POLARBEAR-2 experiment. The POLARBEAR-2 experiment is a cosmic microwave background polarimetry experiment, which aims to characterize the small angular scale B-mode signal due to gravitational lensing and search for the large angular scale B-mode signal from inflationary gravitational waves. The experiment will have a 365 mm diameter multi-chroic focal plane filled with 7,588 polarization sensitive antenna-coupled Transition Edge Sensor bolometers and will observe at 95 and 150 GHz. The focal plane is cooled to 250 mK. The bolometers will be read-out by SQUIDs with $$32\times $$ frequency domain multiplexing. The experiment will utilize high purity alumina lenses and thermal filters to achieve the required high optical throughput. A continuously rotating, cooled half-wave plate will be used to give stringent control over systematic errors. The experiment is designed to achieve a noise equivalent temperature of 5.7 $$\mu $$ K $$\sqrt{s}$$ , and this allows us to constrain the signal from the inflationary primordial gravitational corresponding to a tensor-to-scalar ratio of $$r = 0.01$$ ( $$2\sigma $$ ). POLARBEAR-2 will also be able to put a constraint on the sum of neutrino masses to 90 meV ( $$1\sigma $$ ) with POLARBEAR-2 data alone and 65 meV ( $$1\sigma $$ ) when combined with the Planck satellite. We plan to start observations in 2014 in the Atacama Desert in Chile.
Published: 2014
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24. The POLARBEAR Cosmic Microwave Background Polarization Experiment

Author: Tomotake Matsumura, M. A. Dobbs, S. Moyerman, Nathan Stebor, Chase Owen Shimmin, H. Morii, P. Hyland, Masashi Hazumi, Oliver Zahn, Scott Chapman, Hans P. Paar, A. Ghribi, Masaya Hasegawa, Josquin Errard, Praween Siritanasak, Eric V. Linder, M. Le Jeune, Peter A. R. Ade, W. L. Holzapfel, Andrew H. Jaffe, Yuji Chinone, Aritoki Suzuki, Adrian T. Lee, Julian Borrill, Nathan J. Miller, Gabriel M. Rebeiz, William F. Grainger, Brian Keating, A. E. Anthony, Kam Arnold, Theodore Kisner, Takayuki Tomaru, Paul L. Richards, N. W. Halverson, J. Peloton, Daniel Flanigan, Amit P. S. Yadav, M. J. Myers, Jonathon Howard, H. Nishino, G. Fabbian, D. Boettger, Reijo Keskitalo, G. Jaehnig, Bryan Steinbach, Zigmund Kermish, A. Shimizu, Colin Ross, Meir Shimon, Jennifer Edwards, X. Meng, Carole Tucker, Radek Stompor, M. Sholl, E. Quealy, Christian L. Reichardt, Gary A. Fuller, Kaori Hattori, Helmuth Spieler, Darcy Barron, Marius Lungu, and Frederick Matsuda
Subjects: Physics, Gravitational wave, Bolometer, Cosmic microwave background, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Lenslet, Condensed Matter Physics, Polarization (waves), Atomic and Molecular Physics, and Optics, law.invention, Cardinal point, Gravitational lens, law, Extremely high frequency, General Materials Science
Abstract: The polarbear cosmic microwave background (CMB) polarization experiment has been observing since early 2012 from its 5,200 m site in the Atacama Desert in Northern Chile. polarbear’s measurements will characterize the expected CMB polarization due to gravitational lensing by large scale structure, and search for the possible B-mode polarization signature of inflationary gravitational waves. polarbear’s 250 mK focal plane detector array consists of 1,274 polarization-sensitive antenna-coupled bolometers, each with an associated lithographed band-defining filter and contacting dielectric lenslet, an architecture unique in current CMB experiments. The status of the polarbear instrument, its focal plane, and the analysis of its measurements are presented.
Published: 2014
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25. High performance file system for supercomputing environment.

Author: H. Nishino, S. Naka, K. Ikumi, and W. Leslie
Published: 1989
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26. Erratum: 'A Measurement of the Cosmic Microwave Background B-Mode Polarization Power Spectrum at Sub-degree Scales with POLARBEAR' (2014, ApJ, 794, 171)

Author: Masashi Hazumi, P. Hyland, Kam Arnold, Y. Akiba, Frederick Matsuda, Paul L. Richards, M. Atlas, Yuji Chinone, A. E. Anthony, Amit P. S. Yadav, P. A. R. Ade, Y. Hori, A Orlando, S. Moyerman, Aaron Lee, Reijo Keskitalo, M. Navaroli, Nathan Stebor, I. Schanning, Bryan Steinbach, N. W. Halverson, Yuki Inoue, Chase Owen Shimmin, Zigmund Kermish, H. Nishino, Tucker Elleflot, M. J. Myers, G. Fabbian, Christian L. Reichardt, Eric V. Linder, Masaya Hasegawa, Kaori Hattori, E. M. Leitch, Helmuth Spieler, Theodore Kisner, Chang Feng, Meir Shimon, J. Howard, Praween Siritanasak, Brian Keating, O. Zahn, J. Peloton, Julian Borrill, D. Boettger, Darcy Barron, Radek Stompor, Marius Lungu, H. Morii, S. Takakura, A. Shimizu, Tomotake Matsumura, Hans P. Paar, William F. Grainger, Gabriel M. Rebeiz, E. Quealy, Graeme Smecher, X. Meng, D. E. Schenck, Scott Chapman, Takayuki Tomaru, A. J. Gilbert, Josquin Errard, D. Poletti, B. Wilson, W. L. Holzapfel, Aritoki Suzuki, Daniel Flanigan, Colin Ross, Nathan J. Miller, M. Le Jeune, M. A. Dobbs, Blake D. Sherwin, G. Jaehnig, Andrew H. Jaffe, Cardiff University, The Graduate University for Advanced Studies (SOKENDAI), Shonan International Village, Hayama-cho, University of Colorado, Department of Astrophysical and Planetary Sciences, Center for Astrophysics and Space Astronomy (CASA), Department of Physics, Le Conte Hall, University of California, Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, Department of Physics and Atmospheric Science, Dalhousie University, Department of Physics, University of California, Berkeley, CA 94720, USA, Physics Department, McGill University, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Scuola Internazionale Superiore di Studi Avanzati (SISSA), STFC Rutherford Appleton Laboratory, High Energy Accelerator Research Organization (KEK), Physics Department, Austin College, Sherman, TX 75090, USA, Imperial College London, Department of Physics, Princeton University, Department of Astronomy and Astrophysics, University of Chicago, Lawrence Berkeley National Laboratory (LBNL), Observational Cosmology Laboratory (Code 665), NASA Goddard Space Flight Center, Greenbelt, Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), Todai Institutes for Advanced Study, University of California [San Diego] (UC San Diego), University of California (UC), and Department of Physics and Astronomy, University of British Columbia
Subjects: Physics, large-scale structure of universe, Science & Technology, 0306 Physical Chemistry (Incl. Structural), Cosmic microwave background, Spectral density, Molecular, Astronomy and Astrophysics, Astrophysics, cosmic background radiation, Astronomy & Astrophysics, Polarization (waves), 0305 Organic Chemistry, Atomic, observations [cosmology], 0201 Astronomical And Space Sciences, Particle and Plasma Physics, Space and Planetary Science, Physical Sciences, astro-ph.CO, Nuclear, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astronomical and Space Sciences, Physical Chemistry (incl. Structural)
Abstract: We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band powers are reported over angular multipoles 500 ≤ ℓ ≤ 2100, where the dominant B-mode signal is expected to be due to the gravitational lensing of E-modes. We reject the null hypothesis of no B-mode polarization at a confidence of 3.1σ including both statistical and systematic uncertainties. We test the consistency of the measured B-modes with the Λ Cold Dark Matter (ΛCDM) framework by fitting for a single lensing amplitude parameter A L = 0.60 +0.26-0.24(stat)+0.00-0.04 (inst) ± 0.14(foreground) ± 0.04(multi), where A L = 1 relative to the Planck 2015 best-fit model prediction. We obtain ±0.14(foreground) ±0.04(multi), where is the fiducial ΛCDM value.
Published: 2017
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27. POLARBEAR-2: an instrument for CMB polarization measurements

Author: Y. Inoue, P. Ade, Y. Akiba, C. Aleman, K. Arnold, C. Baccigalupi, B. Barch, D. Barron, A. Bender, D. Boettger, J. Borrill, S. Chapman, Y. Chinone, A. Cukierman, T. de Haan, M. A. Dobbs, A. Ducout, R. Dünner, T. Elleflot, J. Errard, G. Fabbian, S. Feeney, C. Feng, G. Fuller, A. J. Gilbert, N. Goeckner-Wald, J. Groh, G. Hall, N. Halverson, T. Hamada, M. Hasegawa, K. Hattori, M. Hazumi, C. Hill, W. L. Holzapfel, Y. Hori, L. Howe, F. Irie, G. Jaehnig, A. Jaffe, O. Jeong, N. Katayama, J. P. Kaufman, K. Kazemzadeh, B. G. Keating, Z. Kermish, R. Keskitalo, T. S. Kisner, A. Kusaka, M. Le Jeune, A. T. Lee, D. Leon, E. V. Linder, L. Lowry, F. Matsuda, T. Matsumura, N. Miller, K. Mizukami, J. Montgomery, M. Navaroli, H. Nishino, H. Paar, J. Peloton, D. Poletti, G. Puglisi, C. R. Raum, G. M. Rebeiz, C. L. Reichardt, P. L. Richards, C. Ross, K. M. Rotermund, Y. Segawa, B. D. Sherwin, I. Shirley, P. Siritanasak, N. Stebor, R. Stompor, J. Suzuki, A. Suzuki, O. Tajima, S. Takada, S. Takatori, G. P. Teply, A. Tikhomirov, T. Tomaru, N. Whitehorn, A. Zahn, O. Zahn, Holland, Wayne S, Zmuidzinas, Jonas, Institut Lagrange de Paris, Sorbonne Université (SU), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), POLARBEAR, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Sorbonne Universités, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Inoue, Y, Ade, P, Akiba, Y, Aleman, C, Arnold, K, Baccigalupi, C, Barch, B, Barron, D, Bender, A, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, De Haan, T, Dobbs, M, Ducout, A, Dunner, R, Elleflot, T, Errard, J, Fabbian, G, Feeney, S, Feng, C, Fuller, G, Gilbert, A, Goeckner-Wald, N, Groh, J, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hattori, K, Hazumi, M, Hill, C, Holzapfel, W, Hori, Y, Howe, L, Irie, F, Jaehnig, G, Jaffe, A, Jeong, O, Katayama, N, Kaufman, J, Kazemzadeh, K, Keating, B, Kermish, Z, Keskitalo, R, Kisner, T, Kusaka, A, Le Jeune, M, Lee, A, Leon, D, Linder, E, Lowry, L, Matsuda, F, Matsumura, T, Miller, N, Mizukami, K, Montgomery, J, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Poletti, D, Puglisi, G, Raum, C, Rebeiz, G, Reichardt, C, Richards, P, Ross, C, Rotermund, K, Segawa, Y, Sherwin, B, Shirley, I, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, A, Tajima, O, Takada, S, Takatori, S, Teply, G, Tikhomirov, A, Tomaru, T, Whitehorn, N, Zahn, A, Zahn, O, Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie ( APC - UMR 7164 ), and Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA )
Subjects: [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Cosmic microwave background, cosmic background radiation: polarization, Gravitational Wave, Astrophysics, 01 natural sciences, law.invention, law, Polarization, Cosmic Microwave Background, neutrino: mass, mirror, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Weak gravitational lensing, Physics, Equipment and services, Settore FIS/05, superconductivity, Astrophysics::Instrumentation and Methods for Astrophysics, Bolometers, Polarization (waves), vacuum system, astro-ph.CO, readout, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, IR filter, Cosmology and Nongalactic Astrophysics (astro-ph.CO), lens, Bolometer, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 010309 optics, POLARBEAR-2, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Sensors, Gravitational wave, gravitational radiation: primordial, temperature, millimeter wave, optics, Gravitational lens, Extremely high frequency, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], astro-ph.IM
Abstract: POLARBEAR-2 (PB-2) is a cosmic microwave background (CMB) polarization experiment that will be located in the Atacama highland in Chile at an altitude of 5200 m. Its science goals are to measure the CMB polarization signals originating from both primordial gravitational waves and weak lensing. PB-2 is designed to measure the tensor to scalar ratio, r, with precision {\sigma}(r) < 0.01, and the sum of neutrino masses, {\Sigma}m{\nu}, with {\sigma}({\Sigma}m{\nu}) < 90 meV. To achieve these goals, PB-2 will employ 7588 transition-edge sensor bolometers at 95 GHz and 150 GHz, which will be operated at the base temperature of 250 mK. Science observations will begin in 2017., Comment: 9pages,8figures
Published: 2016
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28. The Simons Array CMB polarization experiment

Author: N. Stebor, P. Ade, Y. Akiba, C. Aleman, K. Arnold, C. Baccigalupi, B. Barch, D. Barron, S. Beckman, A. Bender, D. Boettger, J. Borrill, S. Chapman, Y. Chinone, A. Cukierman, T. de Haan, M. Dobbs, A. Ducout, R. Dunner, T. Elleflot, J. Errard, G. Fabbian, S. Feeney, C. Feng, T. Fujino, G. Fuller, A. J. Gilbert, N. Goeckner-Wald, J. Groh, G. Hall, N. Halverson, T. Hamada, M. Hasegawa, K. Hattori, M. Hazumi, C. Hill, W. L. Holzapfel, Y. Hori, L. Howe, Y. Inoue, F. Irie, G. Jaehnig, A. Jaffe, O. Jeong, N. Katayama, J. P. Kaufman, K. Kazemzadeh, B. G. Keating, Z. Kermish, R. Keskitalo, T. Kisner, A. Kusaka, M. Le Jeune, A. T. Lee, D. Leon, E. V. Linder, L. Lowry, F. Matsuda, T. Matsumura, N. Miller, J. Montgomery, M. Navaroli, H. Nishino, H. Paar, J. Peloton, D. Poletti, G. Puglisi, C. R. Raum, G. M. Rebeiz, C. L. Reichardt, P. L. Richards, C. Ross, K. M. Rotermund, Y. Segawa, B. D. Sherwin, I. Shirley, P. Siritanasak, L. Steinmetz, R. Stompor, A. Suzuki, O. Tajima, S. Takada, S. Takatori, G. P. Teply, A. Tikhomirov, T. Tomaru, B. Westbrook, N. Whitehorn, A. Zahn, O. Zahn, Institut Lagrange de Paris, Sorbonne Universités, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Sorbonne Université (SU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Stebor, N, Ade, P, Akiba, Y, Aleman, C, Arnold, K, Baccigalupi, C, Barch, B, Barron, D, Beckman, S, Bender, A, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, De Haan, T, Dobbs, M, Ducout, A, Dunner, R, Elleflot, T, Errard, J, Fabbian, G, Feeney, S, Feng, C, Fujino, T, Fuller, G, Gilbert, A, Goeckner-Wald, N, Groh, J, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hattori, K, Hazumi, M, Hill, C, Holzapfel, W, Hori, Y, Howe, L, Inoue, Y, Irie, F, Jaehnig, G, Jaffe, A, Jeong, O, Katayama, N, Kaufman, J, Kazemzadeh, K, Keating, B, Kermish, Z, Keskitalo, R, Kisner, T, Kusaka, A, Le Jeune, M, Lee, A, Leon, D, Linder, E, Lowry, L, Matsuda, F, Matsumura, T, Miller, N, Montgomery, J, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Poletti, D, Puglisi, G, Raum, C, Rebeiz, G, Reichardt, C, Richards, P, Ross, C, Rotermund, K, Segawa, Y, Sherwin, B, Shirley, I, Siritanasak, P, Steinmetz, L, Stompor, R, Suzuki, A, Tajima, O, Takada, S, Takatori, S, Teply, G, Tikhomirov, A, Tomaru, T, Westbrook, B, Whitehorn, N, Zahn, A, Zahn, O, Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Holland, Wayne S, Zmuidzinas, Jonas, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: Gark energy, Cosmic microwave background, Observatories, cosmic background radiation: polarization, 01 natural sciences, Receivers, Multiplexing, law.invention, Cosmic microwave background radiation, law, Observatory, Polarization, Superconductors, dark energy, Physics, Settore FIS/05, precision measurement, superconductivity, polarimeters, Astrophysics::Instrumentation and Methods for Astrophysics, neutrinos, Polarization (waves), Bolometers, cryogenics, amplifier, interference: quantum, Dark matter, gravitational lensing, Gravitational lensing, Astrophysics::Cosmology and Extragalactic Astrophysics, dark matter, cosmic background radiation: B-mode, Settore FIS/05 - Astronomia e Astrofisica, bolometer, 0103 physical sciences, Neutrino, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], inflation, 010306 general physics, detector: design, activity report, cosmic microwave background radiation, polarization, 010308 nuclear & particles physics, Gravitational wave, Sensors, Bolometer, Astronomy, Polarimeter, Inflation, Amplifiers, Gravitational lens, Antennas, Transition edge sensor, Telescopes
Abstract: International audience; The Simons Array is a next generation cosmic microwave background (CMB) polarization experiment whose science target is a precision measurement of the B-mode polarization pattern produced both by inflation and by gravitational lensing. As a continuation and extension of the successful POLARBEAR experimental program, the Simons Array will consist of three cryogenic receivers each featuring multichroic bolometer arrays mounted onto separate 3.5m telescopes. The first of these, also called POLARBEAR-2A, will be the first to deploy in late 2016 and has a large diameter focal plane consisting of dual-polarization dichroic pixels sensitive at 95 GHz and 150 GHz. The POLARBEAR-2A focal plane will utilize 7,588 antenna-coupled superconducting transition edge sensor (TES) bolometers read out with SQUID amplifiers using frequency domain multiplexing techniques. The next two receivers that will make up the Simons Array will be nearly identical in overall design but will feature extended frequency capability. The combination of high sensitivity, multichroic frequency coverage and large sky area available from our mid-latitude Chilean observatory will allow Simons Array to produce high quality polarization sky maps over a wide range of angular scales and to separate out the CMB B-modes from other astrophysical sources with high fidelity. After accounting for galactic foreground separation, the Simons Array will detect the primordial gravitational wave B-mode signal to r > 0.01 with a significance of > 5σ and will constrain the sum of neutrino masses to 40 meV (1σ) when cross-correlated with galaxy surveys. We present the current status of this funded experiment, its future, and discuss its projected science return.© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Published: 2016
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29. System Design of the ETL Mk-6 Computer.

Author: S. Takahashi, H. Nishino, K. Yoshihiro, and Kazuhiro Fuchi
Published: 1962

30. Poster session Thursday 6 December - AM: Other myocardial diseases

Author: Z. Ojaghi-Haghighi, A. Mostafavi, H. Moladoust, F. Noohi, M. Maleki, M. Esmaeilzadeh, N. Samiei, S. Hosseini, R. Jasaityte, A. Teske, P. Claus, B. Verheyden, F. Rademakers, J. D'hooge, A. Patrianakos, A. Zacharaki, A. Kalogerakis, E. Nyktari, P. Maniatakis, F. Parthenakis, P. Vardas, J. M. Hilde, I. Skjoerten, S. Humerfelt, V. Hansteen, M. Melsom, J. Hisdal, K. Steine, R. Ippolito, P. Gripari, D. Muraru, R. Esposito, G. Kocabay, G. Tamborini, M. Galderisi, F. Maffessanti, L. Badano, M. Pepi, S. Yurdakul, F. Oner, T. Sahin, B. Avci, Y. Tayyareci, H. Direskeneli, S. Aytekin, T. Filali, B. Jedaida, D. Lahidheb, M. Gommidh, H. Mahfoudhi, N. Hajlaoui, R. Dahmani, W. Fehri, H. Haouala, V. Andova, L. Georgievska-Ismail, E. Srbinovska-Kostovska, Y. Gardinger, J. Joanna Hlebowicz, O. Ola Bjorgell, M. Magnus Dencker, M.-T. Liao, C.-T. Tsai, J.-L. Lin, K. Piestrzeniewicz, K. Luczak, M. Maciejewski, J. Komorowski, J. Jankiewicz-Wika, J. Drozdz, M. F. Ismail, A. Alasfar, M. Elassal, S. El-Sayed, M. Ibraheim, P. Dobrowolski, A. Klisiewicz, E. Florczak, A. Prejbisz, E. Szwench, J. Rybicka, A. Januszewicz, P. Hoffman, M. Santos Furtado, K. Nogueira, A. Arruda, A. C. Rodrigues, F. Carvalho, M. Silva, A. Cardoso, E. Lira-Filho, J. Pinheiro, J. L. Andrade, M. Mohammed, C. Zito, M. Cusma-Piccione, G. Di Bella, N. Taha, D. Zagari, A. Oteri, A. Quattrone, I. Boretti, S. Carerj, O. Obremska, B. Boratynska, P. Poczatek, Z. Zon, M. Magott, K. Klinger, O. Szenczi, Z. Szelid, P. Soos, Z. Bagyura, E. Edes, P. Jozan, B. Merkely, J. Ahn, D. Kim, D. Jeon, I. Kim, F. Baeza Garzon, M. Delgado, D. Mesa, M. Ruiz, J. S. De Lezo, M. Pan, C. Leon, F. Castillo, M. Morenate, F. Toledano, L. Zhong, E. Lim, N. Shanmugam, S. Law, B. Ong, K. Katwadi, R. Tan, Y. Chua, R. Liew, Z. Ding, H. Von Bibra, C. Leclerque, T. Schuster, P.-M. Schumm-Draeger, M. Bonios, A. Kaladaridou, O. Papadopoulou, A. Tasoulis, C. Pamboucas, A. Ntalianis, J. Nanas, S. Toumanidis, D. Silva, N. Cortez-Dias, P. Carrilho-Ferreira, R. Placido, C. Jorge, C. Calisto, S. Robalo Martins, J. Carvalho De Sousa, F. Pinto, A. Nunes Diogo, M. Przewlocka-Kosmala, A. Orda, B. Karolko, A. Mysiak, W. Kosmala, S. Moral Torres, J. Rodriguez-Palomares, V. Pineda, D. Gruosso, A. Evangelista, D. Garcia-Dorado, J. Figueras, E. Cambronero, M. J. Corbi, A. Valle, J. Cordoba, C. Llanos, M. Fernandez, I. Lopez, V. Hidalgo, M. Barambio, J. Jimenez, A. D'andrea, L. Riegler, R. Cocchia, M. Russo, E. Bossone, R. Calabro, A. Iniesta Manjavacas, S. Valbuena Lopez, T. Lopez Fernandez, S. Garcia-Blas, F. De Torres Alba, J. G. De Diego, U. Ramirez Valdiris, J. Mesa Garcia, M. Moreno Yanguela, J. Lopez-Sendon, B. Logstrup, H. Andersen, L. Thuesen, E. Christiansen, K. Terp, K. Klaaborg, S. Poulsen, A. Cacicedo, S. Velasco, U. Aguirre, J. Onaindia, I. Rodriguez, G. Oria, A. Subinas, G. Zugazabeitia, A. Romero, E. Laraudogoitia Zaldumbide, S. Weisz, J. Magne, R. Dulgheru, M. Rosca, L. Pierard, P. Lancellotti, V. Auffret, E. Donal, M. Bedossa, D. Boulmier, M. Laurent, J. Verhoye, H. Le Breton, S. Van Hall, T. Herbrand, U. Ketterer, S. Keymel, Y. Boering, T. Rassaf, C. Meyer, T. Zeus, M. Kelm, J. Balzer, M. Floria, S. Seldrum, M. Mariciuc, G. Laurence, M. Buche, P. Eucher, Y. Louagie, J. Jamart, B. Marchandise, E. Schroeder, A. Venkatesh, A. Sahlen, J. Johnson, L. Brodin, R. Winter, K. Shahgaldi, A. Manouras, L. Fusini, M. Muratori, F. Alamanni, A. Bartorelli, C. Ferrari, E. Caiani, E. Yaroslavskaya, V. Kuznetsov, G. Pushkarev, D. Krinochkin, I. Zyrianov, C. Ciobotaru, Y. Kobayashi, K. Yamamoto, E. Hirose, A. Hirohata, T. Ohe, P. Jhund, T. Cunningham, V. Murday, I. Findlay, P. Sonecki, I. Rangel, C. Sousa, A. Goncalves, A. Correia, A. Vigario, E. Martins, J. Silva-Cardoso, F. Macedo, M. Maciel, D. Lovric, J. Samardzic, D. Milicic, V. Reskovic, Z. Baricevic, I. Ivanac, J. Separovic Hanzevacki, K. Kim, J. Song, H. Jeong, H. Yoon, Y. Ahn, M. Jeong, J. Cho, J. Park, J. Kang, A. Iorio, B. Pinamonti, M. Bobbo, M. Merlo, G. Barbati, L. Massa, G. Faganello, A. Di Lenarda, G. Sinagra, F. Heggemann, K. Hamm, F. Streitner, T. Sueselbeck, T. Papavassiliu, M. Borggrefe, D. Haghi, F. Ferreira, A. Galrinho, R. Soares, L. Branco, J. Abreu, J. Feliciano, A. Papoila, M. Alves, A. Leal, R. Ferreira, A. Reynaud, L. H. Lund, E. Oger, E. Drouet, C. Hage, F. Bauer, C. Linde, J. Daubert, F. Schnell, P. Lentz, G. Kervio, G. Leurent, P. Mabo, F. Carre, A. Rodrigues, M. Roque, D. Becker, S. Barros, F. Kay, T. Emerick, P. Sampaio-Barros, J. Andrade, S. Yamada, K. Okada, H. Iwano, H. Nishino, M. Nakabachi, S. Yokoyama, S. Kaga, T. Mikami, H. Tsutsui, R. Mincu, S. Magda, S. Dumitrache Rujinski, T. Constantinescu, S. Mihaila, A. Ciobanu, M. Florescu, D. Vinereanu, T. Ashcheulova, O. Kovalyova, E. Ardeleanu, D. Gurgus, A. Gruici, R. Suciu, I. Ana, L. Bergenzaun, H. Ohlin, P. Gudmundsson, R. Willenheimer, M. Chew, A. Charalampopoulos, L. Howard, R. Davies, W. Gin-Sing, I. Tzoulaki, I. Grapsa, S. Gibbs, P. Massabuau, L. Weinert, O. Lairez, M. Berry, M. Sotaquira, P. Vaida, R. Lang, I. Khan, D. Waterhouse, S. Asegdom, M. Alqaseer, D. Foley, B. Mcadam, P. Colonna, E. Michelotto, W. Genco, M. Rubino, S. Pugliese, A. Belfiore, M. Sorino, M. Trisorio Liuzzi, G. Antonelli, G. Palasciano, A. Duszanska, I. Skoczylas, W. Streb, T. Kukulski, L. Polonski, Z. Kalarus, A. Fleig, K. Seitz, S. Secades, M. Martin, C. Corros, M. Rodriguez, J. De La Hera, A. Garcia, E. Velasco, E. Fernandez, V. Barriales, J. Lambert, D. R. Zwas, S. Hoss, D. Leibowitz, R. Beeri, C. Lotan, D. Gilon, K. Wierzbowska-Drabik, N. Roszczyk, M. Sobczak, M. Plewka, L. Chrzanowski, P. Lipiec, J. Kasprzak, K. Wita, K. Mizia-Stec, W. Wrobel, E. Plonska-Gosciniak, T. Pinho, Y. Wang, H. Houle, A. J. Madureira, J. Zamorano, M. J. Maciel, R. Ancona, S. Comenale Pinto, P. Caso, M. Coppola, O. Rapisarda, R. Calabro', R. Cadenas Chamorro, T. Lopez, J. Gomez, M. Moreno, P. Salinas, C. Jimenez Rubio, S. Valbuena, A. Manjavacas, F. De Torres, T. Vaugrenard, O. Huttin, A. Rouge, J. Schwartz, P. Zinzius, B. Popovic, J. Sellal, E. Aliot, Y. Juilliere, C. Selton-Suty, J. Looi, A. Lee, M. Hsiung, W. Song, R. Wong, M. J. Underwood, F. Fang, Q. Lin, Y. Lam, C. Yu, A. Vitarelli, B. Nguyen, L. Capotosto, G. D-Alessandro, M. D-Ascanio, A. Rafique, E. Gang, F. Barilla, R. Siegel, A. Kydd, F. Khan, W. Watson, L. Mccormick, M. Virdee, D. Dutka, S. Ranjbar, M. Karvandi, S. Hassantash, J. Grapsa, I. Efthimiadis, T. Pakrashi, D. Dawson, P. Punjabi, P. Nihoyannopoulos, M. Henein, S. Soderberg, E. Tossavainen, P. Lindqvist, H. Bellsham-Revell, A. Bell, O. Miller, J. Simpson, E. Altekin, M. Kucuk, A. Yanikoglu, S. Karakas, A. Er, D. Ozel, C. Ermis, I. Demir, G. Bajraktari, G. Di Salvo, L. Baldini, F. Del Gaizo, A. Rea, V. Pergola, G. Pacileo, B. Fadel, J.-S. Seo, G.-N. Choi, H.-Y. Jin, S.-H. Seol, J.-S. Jang, T.-H. Yang, D.-K. Kim, D.-S. Kim, E. Papadopoulou, S. Hatzidou, J. Agrios, C. Pamboukas, A. Antoniou, P. Gargiulo, S. Dellegrottaglie, D. Bruzzese, O. Scala, C. D'amore, D. Ruggiero, C. Marciano, E. Vassallo, E. Pirozzi, P. Perrone Filardi, V. Mor-Avi, N. Kachenoura, J. Lodato, S. Port, S. Chandra, B. Freed, N. Bhave, B. Newby, A. Patel, G. Dwivedi, M. Alam, K. Boczar, B. Chow, G. Staskiewicz, E. Czekajska-Chehab, S. Uhlig, A. Tomaszewski, J. Przegalinski, R. Maciejewski, A. Drop, G. Di Giammarco, C. Canosa, M. Foschi, G. Liberti, M. Bedir, D. Marinelli, S. Masuyama, R. Rabozzi, S. Vijayan, H. Miller, R. Muthusamy, S. Smith, L. Gargani, P. Pang, E. Davis, A. Schumacher, R. Sicari, E. Picano, A. Chmiel, M. Mizia, M. Haberka, K. Gieszczyk, A. Sikora - Puz, B. Lasota, O. Trojnarska, S. Grajek, Z. Gasior, A. Koumoulidis, I. Vlasseros, D. Tousoulis, V. Katsi, A. Avgeropoulou, M. Divani, C. Stefanadis, and I. Kallikazaros
Subjects: medicine.medical_specialty, business.industry, Internal medicine, Cardiology, medicine, Radiology, Nuclear Medicine and imaging, General Medicine, Function (mathematics), Cardiology and Cardiovascular Medicine, Independent predictor, business, Ventricular geometry
Published: 2012
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31. Poster session: Aortic stenosis

Author: R. Piccolo, J. Clarke, C. A. Brambila, B. Igual Munoz, K. Hristova, M. S. Carvalho, M. Tesic, O. Azevedo, J. A. Del Prado, A. Mcculloch, O. Kaitozis, B. Popovic, S. Stankovic, H. Chamsi-Pasha, R. Abdelfatah, V. Parisi, K. Pushparajah, E. Zemtsovsky, B. Kilickiran Avci, A. Manouras, K. Takenaka, F. Parthenakis, P. Vardas, A. Goudev, M. Orii, A. Kutarski, R. De Rosa, M. Castillo Orive, A. Sahlen, H. Ahn, S. Nedjati-Gilani, G. J. King, H. Bellsham-Revell, D. Lahidheb, M. Anastasiou-Nana, F. Pereira Machado, S. Yurdakul, N. Olsen, S. Pica, A. Ebihara, T. Nakajima, P. Molina Aguilar, R. Hornsten, M. Elnoamany, M. Cramer, G. Tamborini, G. Pagano, H. Kim, S. Soderberg, A. M. Gonzalez, N. Zlatareva, E. Marangio, F. Yang, G. Cho, I. Paunovic, C. Jons, T. Tanimoto, H. Triantafyllidi, D. Gopalan, O. Ozcan, M. Norman, G. Grazioli, F. Castillo, E. Kort, R. Bruno, J. Kostic, M. Daimon, D. Kang, C. Badiu, C. Magnino, C. Bucca, I. Joao, F. Buendia Sanchez, A. Tomaszewski, M. Alasnig, J. Kisslo, T. Kawata, S. Fernandez Casares, A. Livingston, J. Silva Cardoso, S. Korkmaz, J. Rodriguez Garcia, M. Tomaszewski, Y. Motoyoshi, A. Kaneva, E. Kinova, J. Lekakis, N. Bruun, M. Elneklawy, K. Uno, K. Nour, J. M. Ferrer, T. Wada, T. Katova, E. Ermis, F. Gaita, S. Rafla, F. Macedo, S. Woo, S. Perry, M. Lonnebakken, K. Thapa, M. Banovic, C. Selton-Suty, V. Pereira, A. Lourenco, G. Dreyfus, W. Serra, M. Hedstrom, A. Hagendorff, H. Nishino, T. Filali, M. Muratori, F. De Stefano, J. Marin, B. Jedaida, I. Rangel, J. Haertel, S. Tzortzis, A. Kalogerakis, G. Galasso, P. Hoffman, L. Chen, Y. Juilliere, V. Kostova, J. Navarro Manchon, C. J. Lopez-Guarch, J L Moya Mur, J. D. J. Baguda, C. Moretti, C. Manisty, N. Hajlaoui, H. Mahfoudhi, E. Martins, F. Bourlon, Y. Choi, C. Papadopoulos, A. Santos, I. V. Vassiliadis, A. Pereira, D. Domingo Valero, P. Iacotucci, C. Fernandez-Golfin, P. Li, I. Xanthopoulou, G. Pontone, R. Tan, D. D. Valero, D. Cramariuc, D. Lovric, F. Maffessanti, V. Pehar Pejcinovic, Y. Xu, M. Gurzun, L. Mitrofanova, P. Sousa, M. Miglioranza, A. Goncalves, I. Nedeljkovic, S. Stanic, C Di Mario, Y. Shiono, Y. Bian, E. Tossavainen, N. Risum, L. Sargento, K. Hirata, K. Said, H. Park, A. M. Argudo, T. Kubo, S. Barker, A. Chetta, R. Palma Reis, E. Malev, C. Yao, I. Papadakis, R. Medeiros, J. Tong, M. Previtali, T. Yamaguchi, S.-H. Shin, M. Sitges, C. Calinescu, J. Rueda Soriano, K. Steine, R. Ichikawa, K. Farouk, S. Pedri, J. Ripsweden, S. Carillo, G. Gelbrich, P. Rees, F. Costantino, S. Hutchings, A. Bel Minguez, A. Gaspar, M. Petrovic, M. Li Kam Wa, E. Mavronasiou, R. Winter, I. Quelhas, J. Johnson, A. Gopal, H. Jurin, R. Rordorf, M. Al-Mallah, A. Kydd, M. Ezat, A. M. Duncan, A. Kyriacou, Y. Kim, D. Mihalcea, J. Lessa, L. Mont, T. Fritz Hansen, J. Separovic Hanzevacki, D. Mesa, R. Mincu, G. Pavlidis, A.D.J. Ten Harkel, L. Gabrielli, F. Civaia, B. Vujisic-Tesic, M. Lourenco, C. Cefalu, C. Alexandrescu, L. Stefani, D. Gerede, M. Bartesaghi, C. Calin, F. Alamanni, A. Giesecke, P. Fazendas, C. Sousa, C. Ginghina, J. Magne, S. Lemoine, M. Gonzalez, C. Gohlke-Baerwolf, K. H. Hirata, S. Fawzi, H. Kisacik, B. Popescu, L. Visconti, W. Brzozowski, M. Driessen, V. Schiano Lomoriello, S. Yamada, I. Machado, F. Silveira, A. Nordin, E. Velazquez, J. Simpson, D. Vasilev, R. Rimbas, R. Murphy, C. Szymanski, T. Imanishi, M. Martirosyan, E. Najjar, J. Chambers, I. Jovanovic, A. Nagorni, E. Gunyeli, M. Omelchenko, P. De Araujo Goncalves, E. Avenatti, R. Marinov, A. Rieck, C. Tribouilloy, I. Sitges, P. Navas Tejedor, N. Lousada, W. Fehri, B. Pezo Nikolic, T. Leiner, C. Lazaro Rivera, H. Pereira, M. Loeffler, R. Hural, D. Caldeira, D. Francis, M. Di Natale, P. Salgado Filho, F. Gao, C. Alm, G. Tarsia, A. Aleixo, D. Vinereanu, C. Cotrim, M. Lotfi, B. Mc Loughlin, H. Morita, S. K. Saha, A. Djordjevic-Dikic, D. Voilliot, R. Camporotondo, J. Shin, P. Pavlov, M. A. Cattabiani, G. Sekita, A. Djordjevic Dikic, K. Ishibashi, C. Pare, J. Kwan, S. Miyazaki, V. Di Tante, E. Svenungsson, V. Giga, Y. Ino, M. Rover, J. Niewiadomska, M. Florescu, I. Skjoerten, C. Wilson, P. Davlouros, M. Hazekamp, N. Moat, A. Correia, C. Tekedis, I. Ikonomidis, B. Dilekci, L. Magda, T. Le, D. Sohn, S. Hamdy, M. Cinteza, R. Enache, A. Milan, R. Dahmani, A. Lopez Granados, J. Zamorano Gomez, E. Zorio Grima, S. Ghulam Ali, B. Demirkan, A. Shehata, M. Vono, M. Chiarlo, Miguel Mota Carmo, D. Trifunovic, B. Bijnens, Y. Yatomi, J J Jimenez Nacher, B. Rogge, R. Nagai, D. Dutka, X. Shen, I. Mordi, M. Henein, F. Celeste, G. Nadais, H. El Atroush, T. Yamano, D. Andreini, B. Beleslin, H. Suzuki, L. Yan, S. Ghio, C. C. De Sousa, S. Stoebe, S. Petrovic-Nagorni, D. Leosco, T. Komori, S. El-Tobgi, S. Mihaila, A. Madureira, T. Leiria, G. Kim, H. Haouala, B. Stuart, G. Touati, K. Oleszczak, M. Ostojic, J. Song, D. Presutti, A. Fournier, H. Daida, M. Perez Guillen, I. Kuipers, H. Hwang, B. Belesiln, K. Park, Y. Guray, D. Pfeiffer, C. Reverberi, A. Lech, A. Valentini, A. Cogo, F. Piscione, S. Negrea, S. Mezghani, V. Pilosoff, P. Sogaard, N. Blom, N. Tzemos, A. Mantovani, K. Okada, A. Turco, M. Peltier, B. Lopez Melgar, U. Guray, Q. Chen, S. Chamuleau, T. Stanton, F. Baeza, S. M. Rafla, J. Roquette, I. Almuntaser, E. Picano, D. Rusinaru, R. Kalil, R. Martin Asenjo, A. Kiotsekoglou, A. Chilingaryan, B. Candemir, P. Sonecki, A. Moulias, M. Rosca, H. Marques, A. Patrianakos, S. Sahin, J. Estornell Erill, O. Enescu, J. Spratt, P. Barbier, M. Maciel, I. Ivanac Vranesic, P. Lindqvist, T. Snow, J. Silva-Cardoso, N. Koutsogiannis, D. Ardissino, L. Zhong, K. Adamyan, L. Mccormick, A. Calin, P. Innelli, S. Yokoyama, C. Erol, P. Pabari, A. Tarr, M. Galderisi, S. Govind, B. Suran, I. Simova, E. Guyeli, T. Pinho, L. Bjornadal, B. Diaz Anton, J. Hilde, R. Sicari, C. Beladan, M. Ege, A. Zacharaki, L. Ghiadoni, A. A. La Huerta, S. Zdravkovic-Ciric, O. Huttin, K. Jensen-Urstad, F. Veglio, M. Elsedi, M. Nakabachi, P. Zinzius, D. Kim, H. Dores, A. Kakkavas, H. Badran, V. Sanchez Sanchez, E. Duo, J. Carrasco, A. Almeida, M. Virdee, M. Llemit, A. Anwar, L. Pratali, J. Monmeneu Menadas, S. Nevin, L. Fusini, F. Lombera Romero, E. Despotopoulos, E. Nyktari, G. Galanti, K. Kim, A. Van Der Hulst, H. Khachab, M. Dikic, I. Cruz, M. Melsom, J. Brugada, V. Mitic, M. Landolina, S. Turhan, V. Hansteen, D Rodriguez Munoz, J. S. De Lezo, N. Gori, Z. Baricevic, S.-P. Lee, M. Arnau Vives, S. Lee, P. Gripari, S. Humerfelt, F. Huang, T. Mikami, G. Soltan, T. Akasaka, S. Kaga, G. Penney, L. Toncelli, K. Boman, B. Basnyat, E. Kowalik, A. Bartolini, S. Georgiev, K. Shahgaldi, M. Pepi, M. Ruiz Ortiz, R. Sant'anna, H. Tsutsui, P. A. Fernandez, G. Tempesti, S. Aytekin, H. Iwano, Y. Nosir, C. Raineri, J. Rasmunsson, S. Lasarov, P. Lopez Lereu, V. Persic, F. Khan, J. Hisdal, M. Gommidh, A. Alhagoly, E. Gerdts, M. Milicia, G. Rengo, K. Kimura, F. Hakansson, M. Morenate, P. Mitev, M. Yacoub, M. Satendra, B. Kusmierczyk-Droszcz, E. Romo, R. Jankovic-Tomasevic, A. Roest, J. Stepanovic, J. Schwartz, Z. Ashour, L. Klitsie, J. Giner Blasco, M. Delgado, P. Omede, S. Mayordomo Gomez, I. Paraskevaidis, J. L. Zamorano, N. Goodfield, E. Dores, S. Davies, N. Patrascu, D. Alexopoulos, L. Donate Bertolin, D. Stanojevic, E. Psathakis, M. Dobric, P. Trivilou, H. Sasmaz, A. Marinkovic, O. Mirea, G. Sieswerda, M. Maruyama, A. M. Maceira Gonzalez, T. I. Imanishi, A. Santoro, G. Festa, R. Coma Samartin, and V. Atanaskovic
Subjects: medicine.medical_specialty, Stenosis, business.industry, Internal medicine, Cardiology, medicine, Radiology, Nuclear Medicine and imaging, General Medicine, Session (computer science), Cardiology and Cardiovascular Medicine, business, medicine.disease
Published: 2012
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32. Polymorphisms in the 5′-UTR of PTEN and other gene polymorphisms in normal Japanese individuals

Author: Y. Ohsaka and H. Nishino
Subjects: Genetics, Untranslated region, biology, Five prime untranslated region, Intron, Cell Biology, Agricultural and Biological Sciences (miscellaneous), Molecular biology, Exon, biology.protein, PTEN, Tensin, Genotyping, Gene
Abstract: Polymorphisms are distributed differently in populations, including those of regions, ethnic groups, and diseased patients. In order to investigate variation in nucleotide sequences in normal individuals, we isolated genomic DNA from the blood of healthy Japanese individuals and sequenced the 5'-untranslated region (5'-UTR) of the phosphatase and tensin homolog deleted on chromosome 10 (PTEN) gene and the gene promoter, intron, and exon nucleotides of p53, p14(ARF), murine double minute 2 (MDM2), and the beta2- and beta3-adrenoceptor (-AR). We found polymorphisms in these regions, including a deletion at positions -465 to -463 and a substitution at position -404 in PTEN and a substitution at position -4924 in p14(ARF), in normal individuals. Individuals with or without the PTEN polymorphism harbored a different distribution of polymorphisms, including simultaneous alterations in nucleotides of p53, MDM2, and beta3-AR, and also harbored some polymorphic nucleotides located in the same set of associatively altered nucleotides. Our results show that multiple nucleotides, including the PTEN nucleotides, are altered in normal Japanese individuals and provide useful information for genotyping studies in individuals and populations.
Published: 2012
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33. Influence of contents rate and dispersion of carbon nanotubes on interfacial adhesion between continuous fiber reinforced thermoplastics and injection resin

Author: H. Nishino, K. Matsumoto, T. Tanaka, and J. Shiode
Subjects: Materials science, Interfacial adhesion, 02 engineering and technology, General Medicine, Carbon nanotube, 010402 general chemistry, 021001 nanoscience & nanotechnology, 01 natural sciences, 0104 chemical sciences, law.invention, law, Dispersion (optics), Fiber, Composite material, 0210 nano-technology
Published: 2018
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34. High-speed charge-to-time converter ASIC for the Super-Kamiokande detector

Author: Masato Shiozawa, H. Nishino, K. Ishikawa, Atsushi Takeda, Yoshio Arai, A. Minegishi, Kimihiro Okumura, K. Awai, Y. Hayato, and Shoei Nakayama
Subjects: Physics, Nuclear and High Energy Physics, Signal processing, Physics - Instrumentation and Detectors, Preamplifier, business.industry, Detector, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Analog signal processing, Signal, Time-to-digital converter, Optoelectronics, Waveform, business, Instrumentation, Electronic circuit
Abstract: A new application-specific integrated circuit (ASIC), the high-speed charge-to-time converter (QTC) IWATSU CLC101, provides three channels, each consisting of preamplifier, discriminator, low-pass filter, and charge integration circuitry, optimized for the waveform of a photomultiplier tube (PMT). This ASIC detects PMT signals using individual built-in discriminators and drives output timing signals whose width represents the integrated charge of the PMT signal. Combined with external input circuits composed of passive elements, the QTC provides full analog signal processing for the detector's PMTs, ready for further processing by time-to-digital converters (TDCs). High-rate (>1MHz) signal processing is achieved by short-charge-conversion-time and baseline-restoration circuits. Wide-range charge measurements are enabled by offering three gain ranges while maintaining a short cycle time. QTC chip test results show good analog performance, with efficient detection for a single photoelectron signal, four orders of magnitude dynamic range (0:3mV ~ 3V; 0:2 ~ 2500 pC), 1% charge linearity, 0.2 pC charge resolution, and 0.1 ns timing resolution. Test results on ambient temperature dependence, channel isolation, and rate dependence also meet specifications., 24 pages, 19 figures
Published: 2009
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35. Study of TeV neutrinos with upward showering muons in Super-Kamiokande

Author: C. W. Walter, R. Wendell, R. Svoboda, T. Ishizuka, S. Yamada, T. Sasaki, M. Yoshida, H. G. Berns, M. B. Smy, Y. Furuse, K. Kaneyuki, C. Saji, Masashi Yokoyama, R. Terri, A. Minamino, J. Dunmore, Takaaki Kajita, Y. Totsuka, K. Iida, M. Koshiba, Y. Oyama, B. S. Yang, Y. Choi, K. Ishihara, T. J. Haines, T. Sato, D. W. Liu, Haruki Watanabe, Masato Shiozawa, N. Tamura, H. Nishino, I. Kato, Lawrence Sulak, J. L. Raaf, J. L. Stone, S. Mine, Y. Takeuchi, Atsushi Takeda, E. Kearns, S. T. Clark, C. Ishihara, Shantanu Desai, Kunio Inoue, M. Sugihara, H. Ishii, C. K. Jung, T. Ishida, M. Swanson, K. Abe, T. Kobayashi, K. Nishikawa, T. Nakaya, T. Nakadaira, Yusuke Koshio, K. Nitta, J. Yoo, S. Yamamoto, Kate Scholberg, J. Y. Kim, C. McGrew, M. R. Vagins, C. Yanagisawa, K. Kobayashi, Y. Obayashi, K. Washburn, W. E. Keig, M. Hasegawa, Shigetaka Moriyama, S. Likhoded, G. Mitsuka, K. Ueshima, I. S. Jeong, M. Sakuda, Y. Hayato, R. Gran, T. Hasegawa, F. Dufour, I. T. Lim, H. K. Seo, A. K. Ichikawa, J. S. Jang, T. Tanaka, D. Kielczewska, Y. Kuno, K. Nishijima, S. Nakayama, M. Ishitsuka, N. Tanimoto, S. Tasaka, H. Okazawa, R. J. Wilkes, W. Wang, Masayuki Nakahata, Alec Habig, T. Koike, B. Hartfiel, Y. Takenaga, K. Okumura, Y. Fukuda, Y. Idehara, K. S. Ganezer, M. Miura, Hirokazu Ishino, M. D. Messier, C. Regis, J. Kameda, Katsuki Hiraide, S. Dazeley, J. P. Cravens, T. Ishii, H. Sato, Y. Gando, J. Hill, Yasunari Suzuki, S. Matsuno, G. Guillian, A. T. Suzuki, H. W. Sobel, Eric Thrane, M. Fechner, Y. Watanabe, W. R. Kropp, S. B. Kim, A. Clough, David William Casper, C. Mitsuda, H. Ogawa, K. K. Shiraishi, I. Higuchi, J. G. Learned, H. Maesaka, M. Goldhaber, T. Kato, Yoshitaka Itow, S. Hatakeyama, K. Nakamura, and A. Sarrat
Subjects: Physics, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Bremsstrahlung, Astronomy and Astrophysics, High Energy Physics - Experiment, Nuclear physics, Pair production, WIMP, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Super-Kamiokande, Neutrino oscillation, Zenith
Abstract: A subset of neutrino-induced upward through-going muons in the Super-Kamiokande detector consists of high energy muons which lose energy through radiative processes such as bremsstrahlung, e^{+} e^{-} pair production and photonuclear interactions. These ``upward showering muons'' comprise an event sample whose mean parent neutrino energy is approximately 1 TeV. We show that the zenith angle distribution of upward showering muons is consistent with negligible distortion due to neutrino oscillations, as expected of such a high-energy neutrino sample. We present astronomical searches using these high energy events, such as those from WIMP annihilations in the Sun, Earth and Galactic Center, some suspected point sources, as well as searches for diffuse flux from the interstellar medium., Comment: Submitted for publication to Astroparticle Physics. Fig 12 has slightly higher resolution in the version submitted to the journal
Published: 2008
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36. Modeling Atmospheric Emission for CMB Ground-based Observations

Author: Nathan Stebor, Tomotake Matsumura, Christian L. Reichardt, Michael J. Myers, S. Takakura, Masaya Hasegawa, Giuseppe Puglisi, Adrian T. Lee, Kaori Hattori, Charles A. Hill, Julian Borrill, Nobuhiko Katayama, K. M. Rotermund, Stephen M. Feeney, Kam Arnold, Davide Poletti, E. M. Leitch, Darcy Barron, Neil Goeckner-Wald, Yuji Chinone, Peter A. R. Ade, Nathan Whitehorn, M. Atlas, Y. Akiba, Greg Jaehnig, Andrew H. Jaffe, Chang Feng, Scott Chapman, Gabriel M. Rebeiz, Brian Keating, A. Gilbert, Colin Ross, M. Navaroli, Aritoki Suzuki, Tucker Elleflot, Graeme Smecher, Hans P. Paar, Ted Kisner, J. Peloton, Oliver Jeong, Amit P. S. Yadav, Giulio Fabbian, J. P. Kaufman, D. E. Schenck, N. W. Halverson, A. Ducout, A. Tikhomirov, Masashi Hazumi, Takayuki Tomaru, Radek Stompor, Praween Siritanasak, Zigmund Kermish, Oliver Zahn, Blake D. Sherwin, D. Boettger, M. Le Jeune, Takahiro Okamura, A. Cukierman, B. Wilson, D. Leon, Nathan J. Miller, Reijo Keskitalo, Bryan Steinbach, M. A. Dobbs, Yuki Inoue, Josquin Errard, W. L. Holzapfel, Y. Hori, Jacques Delabrouille, Paul L. Richards, Frederick Matsuda, H. Nishino, Osamu Tajima, Eric V. Linder, Carlo Baccigalupi, Biological Imaging Core, Department of Biological Sciences, University of Notre Dame [Indiana] (UND), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Regional Virus Laboratory, Royal Victoria Hospital, Laboratoire de glaciologie et géophysique de l'environnement (LGGE), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Berkeley], University of California [Berkeley], University of California-University of California, Korea Research Institute for Human Settlements (KRIHS), Korea Research Institute for Human Settlements, Department of Endocrinology, Universiteit Gent = Ghent University [Belgium] (UGENT), Centre interdisciplinaire de recherches sur les valeurs, les idées, les identités et les compétences en Éducation et en formation (CIVIIC), Université de Rouen Normandie (UNIROUEN), Normandie Université (NU)-Normandie Université (NU), Department of Computer Science [Amherst], University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS)-University of Massachusetts System (UMASS), Department of Atmospheric Science [Laramie], University of Wyoming (UW), The University of Tokyo (UTokyo), Carnegie Mellon University [Pittsburgh] (CMU), Columbia University [New York], University of California [San Diego] (UC San Diego), University of California, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), University of California [Berkeley] (UC Berkeley), University of California (UC)-University of California (UC), Universiteit Gent = Ghent University (UGENT), University of California (UC), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS), Ghent University [Belgium] (UGENT), The University of Tokyo, Science and Technology Facilities Council (STFC), Imperial College Trust, Science and Technology Facilities Council [2006-2012], Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Errard, J, Ade, P, Akiba, Y, Arnold, K, Atlas, M, Baccigalupi, C, Barron, D, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, Delabrouille, J, Dobbs, M, Ducout, A, Elleflot, T, Fabbian, G, Feng, C, Feeney, S, Gilbert, A, Goeckner-Wald, N, Halverson, N, Hasegawa, M, Hattori, K, Hazumi, M, Hill, C, Holzapfel, W, Hori, Y, Inoue, Y, Jaehnig, G, Jaffe, A, Jeong, O, Katayama, N, Kaufman, J, Keating, B, Kermish, Z, Keskitalo, R, Kisner, T, Le Jeune, M, Lee, A, Leitch, E, Leon, D, Linder, E, Matsuda, F, Matsumura, T, Miller, N, Myers, M, Navaroli, M, Nishino, H, Okamura, T, Paar, H, Peloton, J, Poletti, D, Puglisi, G, Rebeiz, G, Reichardt, C, Richards, P, Ross, C, Rotermund, K, Schenck, D, Sherwin, B, Siritanasak, P, Smecher, G, Stebor, N, Steinbach, B, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Tikhomirov, A, Tomaru, T, Whitehorn, N, Wilson, B, Yadav, A, and Zahn, O
Subjects: COMPONENT SEPARATION, POLARIZATION, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 0306 Physical Chemistry (Incl. Structural), atmospheric effect, Cosmic microwave background, FOS: Physical sciences, Astronomy & Astrophysics, 0305 Organic Chemistry, 01 natural sciences, NOISE, Weather station, Atmosphere, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Physics::Atmospheric and Oceanic Physics, ComputingMilieux_MISCELLANEOUS, SITES, Science & Technology, Settore FIS/05, 010308 nuclear & particles physics, Linear polarization, Detector, Astronomy and Astrophysics, FLUCTUATIONS, methods: data analysis, Computational physics, 0201 Astronomical And Space Sciences, Wavelength, methods: observational, 13. Climate action, Space and Planetary Science, Physical Sciences, astro-ph.CO, TURBULENCE, Environmental science, Millimeter, MICROWAVE BACKGROUND EXPERIMENTS, Astrophysics - Instrumentation and Methods for Astrophysics, methods: data analysi, Noise (radio), Astrophysics - Cosmology and Nongalactic Astrophysics, astro-ph.IM, atmospheric effects
Abstract: Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies their effective noise, while its fluctuations introduce spatial and temporal correlations between detected signals. We present a physically motivated 3d-model of the atmosphere total intensity emission in the millimeter and sub-millimeter wavelengths. We derive a new analytical estimate for the correlation between detectors time-ordered data as a function of the instrument and survey design, as well as several atmospheric parameters such as wind, relative humidity, temperature and turbulence characteristics. Using an original numerical computation, we examine the effect of each physical parameter on the correlations in the time series of a given experiment. We then use a parametric-likelihood approach to validate the modeling and estimate atmosphere parameters from the POLARBEAR-I project first season data set. We derive a new 1.0% upper limit on the linear polarization fraction of atmospheric emission. We also compare our results to previous studies and weather station measurements. The proposed model can be used for realistic simulations of future ground-based CMB observations., Comment: 20 pages, 16 figures
Published: 2015
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37. The POLARBEAR-2 and the Simons Array Experiment

Author: Peter A. R. Ade, O. Zahn, Gabriel M. Rebeiz, Suguru Takada, Josquin Errard, D. Poletti, Zigmund Kermish, K. Mizukami, Carlo Baccigalupi, Darcy Barron, Neil Goeckner-Wald, Theodore Kisner, Christopher Raum, G. Hall, R. Dunner, Joshua Montgomery, Tucker Elleflot, Paul L. Richards, A. J. Gilbert, Stephen M. Feeney, M. Navaroli, T. Fujino, Nathan Stebor, Aritoki Suzuki, S. Takatori, D. Boettger, M. A. Dobbs, J. Kaufman, T. Yamashita, Eric V. Linder, Giulio Fabbian, Y. Akiba, Adrian T. Lee, A. Tikhomirov, B. Westbrook, Tomotake Matsumura, Jose H. Groh, Amy N. Bender, Masaya Hasegawa, Scott Chapman, Brian Keating, Colin Ross, Nathan J. Miller, Y. Hori, Radek Stompor, L. Howe, Reijo Keskitalo, A. Ducout, H. Nishino, A. Cukierman, G. Jaehnig, Takayuki Tomaru, I. Shirley, K. M. Rotermund, Osamu Tajima, Masashi Hazumi, D. Leon, Christian L. Reichardt, Kam Arnold, Blake D. Sherwin, Praween Siritanasak, J. Peloton, Kaori Hattori, T. Hamada, L. Lowry, M. Le Jeune, C. Aleman, Giuseppe Puglisi, Jun-ichi Suzuki, F. Irie, Akito Kusaka, W. Holzapfel, O. B. Jeong, Julian Borrill, Chang Feng, A. Zahn, Yuji Chinone, Nobuhiko Katayama, N. Whitehorn, Y. Segawa, K. Kazemzadeh, S. Takakura, Andrew H. Jaffe, N. W. Halverson, T. de Haan, Yuki Inoue, Frederick Matsuda, C. Hill, G. Fuller, Université Paris-Sorbonne (UP4), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), POLARBEAR, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Suzuki, A, Ade, P, Akiba, Y, Aleman, C, Arnold, K, Baccigalupi, C, Barch, B, Barron, D, Bender, A, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, Dobbs, M, Ducout, A, Dunner, R, Elleflot, T, Errard, J, Fabbian, G, Feeney, S, Feng, C, Fujino, T, Fuller, G, Gilbert, A, Goeckner-Wald, N, Groh, J, Haan, T, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hattori, K, Hazumi, M, Hill, C, Holzapfel, W, Hori, Y, Howe, L, Inoue, Y, Irie, F, Jaehnig, G, Jaffe, A, Jeong, O, Katayama, N, Kaufman, J, Kazemzadeh, K, Keating, B, Kermish, Z, Keskitalo, R, Kisner, T, Kusaka, A, Jeune, M, Lee, A, Leon, D, Linder, E, Lowry, L, Matsuda, F, Matsumura, T, Miller, N, Mizukami, K, Montgomery, J, Navaroli, M, Nishino, H, Peloton, J, Poletti, D, Puglisi, G, Rebeiz, G, Raum, C, Reichardt, C, Richards, P, Ross, C, Rotermund, K, Segawa, Y, Sherwin, B, Shirley, I, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, J, Tajima, O, Takada, S, Takakura, S, Takatori, S, Tikhomirov, A, Tomaru, T, Westbrook, B, Whitehorn, N, Yamashita, T, Zahn, A, Zahn, O, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sorbonne ( UP4 ), AstroParticule et Cosmologie ( APC - UMR 7164 ), and Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA )
Subjects: Cosmic microwave background, Inflation, Gravitational weak lensing, Polarization, B-mode, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], cosmic background radiation, 7. Clean energy, 01 natural sciences, pixel, optical, General Materials Science, neutrino: mass, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Weak gravitational lensing, Mathematical Physics, Physics, Settore FIS/05, Astrophysics::Instrumentation and Methods for Astrophysics, Polarization (waves), Condensed Matter Physics, Atomic and Molecular Physics, and Optics, astro-ph.CO, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, General Physics, noise, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Frequency band, Classical Physics, Cosmic background radiation, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Noise-equivalent temperature, Optics, Settore FIS/05 - Astronomia e Astrofisica, gravitation: lens, bolometer, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010308 nuclear & particles physics, business.industry, Gravitational wave, gravitational radiation, temperature, sensitivity, Transition edge sensor, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], astro-ph.IM
Abstract: We present an overview of the design and status of the \Pb-2 and the Simons Array experiments. \Pb-2 is a Cosmic Microwave Background polarimetry experiment which aims to characterize the arc-minute angular scale B-mode signal from weak gravitational lensing and search for the degree angular scale B-mode signal from inflationary gravitational waves. The receiver has a 365~mm diameter focal plane cooled to 270~milli-Kelvin. The focal plane is filled with 7,588 dichroic lenslet-antenna coupled polarization sensitive Transition Edge Sensor (TES) bolometric pixels that are sensitive to 95~GHz and 150~GHz bands simultaneously. The TES bolometers are read-out by SQUIDs with 40 channel frequency domain multiplexing. Refractive optical elements are made with high purity alumina to achieve high optical throughput. The receiver is designed to achieve noise equivalent temperature of 5.8~$\mu$K$_{CMB}\sqrt{s}$ in each frequency band. \Pb-2 will deploy in 2016 in the Atacama desert in Chile. The Simons Array is a project to further increase sensitivity by deploying three \Pb-2 type receivers. The Simons Array will cover 95~GHz, 150~GHz and 220~GHz frequency bands for foreground control. The Simons Array will be able to constrain tensor-to-scalar ratio and sum of neutrino masses to $\sigma(r) = 6\times 10^{-3}$ at $r = 0.1$ and $\sum m_\nu (\sigma =1)$ to 40 meV., Comment: Accepted to Journal of Low Temperature Physics LTD16 Special Issue, Low Temperature Detector 16 Conference Proceedings, 5 pages, 1 figure
Published: 2015
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38. Measurement of neutrino oscillation by the K2K experiment

Author: S. Andringa, T. Nakadaira, R. Gran, Tadayuki Takahashi, Yoshitaka Itow, Makoto Sakuda, F. Nakata, K. Fujii, A. Rodriguez, D. Kerr, M. H. Ahn, U. Dore, S. Likhoded, S P Mikheyev, K. Martens, Y. Totsuka, Y. Takubo, Kate Scholberg, Y. Takeuchi, Yu. Kudenko, Shinya Yamada, H. I. Jang, S. C. Boyd, M. Okumura, A. Blondel, A. Ikeda, K. Tashiro, Itsuo Nakano, C. K. Jung, M. Sekiguchi, H. Yokoyama, F. Pierre, Minoru Yoshida, M. Kitamura, L. Whitehead, K. Taki, S. Nawang, N. Yershov, Shogo Nishiyama, O. V. Mineev, E. Sharkey, K. Kaneyuki, Hirokazu Ishino, D. Kielczewska, Shoei Nakayama, Taichi Morita, Y. Kurimoto, Hiroyuki Noumi, T. Otaki, R. Schroeter, L. Ludovici, E. J. Jeon, Takashi Kobayashi, J. Kameda, M. Onchi, Y. Yamanoi, C. Cavata, M. Sorel, Katsuki Hiraide, H. C. Bhang, P. F. Loverre, J. Bouchez, M. Y. Pac, G. Sitjes, S. Mine, C. O. Kim, I. Kato, E. Seo, A. Shima, T. Kutter, K. Hayashi, H. So, S. M. Oser, T. Ishida, J. Hill, J. Catala, A. K. Ichikawa, Tomoyuki Maruyama, T. Hara, K. K. Joo, Lawrence Sulak, P. Novella, Susumu Noda, S. Fukuda, K. Takenaka, Yoshitaka Kuno, T. Ishii, Masaaki Tanaka, F. Nova, John G. Learned, Y. Yamada, B. H. Kang, Y. Obayashi, M. Takasaki, A. Minamino, A. Tornero-Lopez, J.J. Gómez-Cadenas, Takanori Sasaki, M. Fechner, S. Echigo, C. Yanagisawa, J. Zalipska, C. McGrew, G. Jover, J.H. Kim, K. Nakamura, K. B. McConnel Mahn, S. B. Kim, V. A. Matveev, M. Minakawa, A. Cervera, C. W. Walter, Y. Takenaga, Y. Hayato, Yuichi Oyama, Masaya Hasegawa, M. Miura, G. Kume, M. Tada, David William Casper, Takehisa Hasegawa, C. Mitsuda, K. Sato, J. Hosaka, A. Suzuki, R. L. Helmer, Hyosun Kim, Katsuhiro Kobayashi, A. Sakai, Nobuyuki Sakurai, Yusuke Koshio, S. Ueda, Shoji Yamamoto, J. Mallet, S. Matsuno, H. Takeuchi, T. Ooyabu, Masayuki Nakahata, Y. Aoyama, R. Terri, R. Ashie, H. Ishii, Y. Suga, Masashi Yokoyama, J. S. Jang, G. Mitsuka, E. Aliu, H. Tanaka, A. Sarrat, Mark R. Vagins, K. K. Shiraishi, Takaaki Kajita, Masaki Ishitsuka, Kenichi Tanaka, Yoshihiro Suzuki, H. Park, Masaharu Ieiri, X. Espinal, Y. Moriguchi, Beom Jun Kim, Michael B. Smy, Y. Fukuda, T. Iwashita, R. J. Wilkes, I. Higuchi, I. T. Lim, Y. Kato, W. R. Kropp, Federico Sanchez, Toshio Namba, C. Mariani, H. Maesaka, Ko Okumura, E. Kearns, Shigeki Aoki, T. Toshito, Hiroshi Sato, K. Asakura, P. Kitching, C. Mauger, J. Argyriades, H. Nishino, S. H. Lim, A. Okada, M. Kohama, M. Takatsuki, F. Berghaus, Tsuyoshi Nakaya, C. Saji, J. Kubota, Jordi Burguet-Castell, H. G. Berns, W. Wang, Masataka Iinuma, E. Hirose, J. Yoo, K. Nishikawa, J. Y. Kim, Henry W. Sobel, K. Nitta, Y. Tanaka, Masato Shiozawa, Shaomin Chen, A. Konaka, Shigetaka Moriyama, K. O. Cho, R. Nambu, N. Tamura, Silvia Borghi, J. L. Stone, T. Inagaki, A. N. Khotjantsev, Y. Fujii, J. H. Choi, M. M. Khabibullin, Stephane T'Jampens, E. Fernandez, I. S. Jeong, and K. Ishihara
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Tamura, Norio, 010308 nuclear & particles physics, Oscillation, T2K experiment, FOS: Physical sciences, Física, Elementary particle, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, Massless particle, High Energy Physics - Experiment (hep-ex), K2K experiment, 0103 physical sciences, 田村, 詔生, Neutrino, 010306 general physics, Neutrino oscillation, Lepton
Abstract: We present measurements of nu_mu disappearance in K2K, the KEK to Kamioka long-baseline neutrino oscillation experiment. One hundred and twelve beam-originated neutrino events are observed in the fiducial volume of Super-Kamiokande with an expectation of 158.1^{+9.2}_{-8.6} events without oscillation. A distortion of the energy spectrum is also seen in 58 single-ring muon-like events with reconstructed energies. The probability that the observations are explained by the expectation for no neutrino oscillation is 0.0015% (4.3sigma). In a two flavor oscillation scenario, the allowed Delta m^2 region at sin^2(2theta) is between 1.9 and 3.5 x 10^{-3} eV^2 at the 90% C.L. with a best-fit value of 2.8 x 10^{-3} eV^2., Comment: 40 pages, 48 figures
Published: 2006

39. Knudsen Effect in a Nonequilibrium Gas

Author: Hisao Hayakawa and Taka H. Nishino
Subjects: Molecular dynamics, Boundary layer, Materials science, Distribution function, Statistical Mechanics (cond-mat.stat-mech), Heat flux, FOS: Physical sciences, General Physics and Astronomy, Non-equilibrium thermodynamics, Mechanics, Knudsen number, Condensed Matter - Statistical Mechanics, Pressure difference
Abstract: From the molecular dynamics simulation of a system of hard-core disks in which an equilibrium cell is connected with a nonequilibrium cell, it is confirmed that the pressure difference between two cells depends on the direction of the heat flux. From the boundary layer analysis, the velocity distribution function in the boundary layer is obtained. The agreement between the theoretical result and the numerical result is fairly good., 4pages, 4figures
Published: 2005
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40. Measurements of the T2K neutrino beam properties using the INGRID on-axis near detector

Author: J. Marteau, Z. Williamson, P. F. Loverre, M. Iida, T. Ishii, M. M. Khabibullin, H. Kaji, J. Blocki, Andrew Marone, S. Dytman, H. Kubo, J. M. Roney, T. Ishida, J. Bouchez, Thorsten Lux, J. Zmuda, Frédéric Dufour, M. Gonin, G. P. Ward, Y. Kouzuma, L. Escudero, Kenichi Tanaka, Akitaka Ariga, R.P. Kurjata, S. W. Bentham, J. R. Wilson, C. Nielsen, M. Messina, I. T. Lim, Shigeki Aoki, S. Giffin, I. Z. Danko, Justin Albert, A. V. Waldron, P. A. Rodrigues, M. Besnier, J. Dobson, A. Minamino, N. Abgrall, Joshua Hignight, Yoshihiro Suzuki, K. Tashiro, Katsuyu Kasami, S. Tobayama, J. L. Stone, J. J. Walding, V. Galymov, K. Kowalik, J. Myslik, M. Malek, L. L. Kormos, S. Horikawa, Masashi Tanaka, Koji Nakamura, A. N. Khotjantsev, Y. Fujii, Suyong Choi, Alastair Grant, T. Golan, C. Hansen, Y. Totsuka, J. D. Perkin, M. Barbi, G. Mituka, V. Paolone, T. Maryon, K. Iyogi, Yutaka Yamanoi, M. M. Tanaka, W. Metcalf, W. Coleman, T. Wongjirad, F. Di Lodovico, André Rubbia, S. Takahashi, F. Bay, Hiroshi Yamaoka, A. Marchionni, T. Nobuhara, C. A. Chavez, J. Kisiel, T. Kikawa, A. C. Weber, M. J. Wilking, E. D. Zimmerman, Tomiyoshi Haruyama, Robert Henderson, K. Zaremba, Atsushi Takeda, M. Siyad, V. Pettinacci, M. Miura, Barry L. Nelson, Yu. G. Kudenko, T. Ozaki, E. Mazzucato, N. Kimura, L. Monfregola, J. Dumarchez, J. P.A.M. De André, Robert Wilson, K. Suzuki, D. Naples, Y. Takeuchi, Shinya Yamada, A. Robert, J. Steinmann, S. Di Luise, M. Ravonel, K. Nitta, Norio Higashi, K. Gilje, G. F. Pearce, R. A. Johnson, C. Giganti, H. S. Budd, Oleg Mineev, Alexander Finch, N. Grant, A. Izmaylov, A. Curioni, M. Taguchi, C. K. Jung, J. L. Raaf, Michal Dziewiecki, G. Jover-Manas, M. Ziembicki, G. Collazuol, Sy Suzuki, M. Murdoch, Minoru Otani, E. L. Mathie, K. Nishikawa, A. Carver, P. Paul, Kazuhiro Yamamoto, J. A. Nowak, D. Kielczewska, M. Batkiewicz, C. Ishihara, A. Dabrowska, Takahiro Okamura, J. Argyriades, D. Ruterbories, Mark Scott, Jan T. Sobczyk, P. de Perio, K. Laihem, A.K. Ghosh, J. Beucher, N. West, I. Kato, S. Yen, T. Yano, T. Dealtry, Michel Raymond, A. Missert, P. Guzowski, S. B. Boyd, M. Sorel, Takaaki Kajita, G. D. Lopez, Luigi Salvatore Esposito, N. Nagai, J. Zalipska, J. Lagoda, M. Iwasaki, T. Hara, F. Pierre, R. A. Wendell, G. Christodoulou, T. Lindner, O. Drapier, M. Bass, A. Suzuki, B. Hartfiel, Masashi Yokoyama, Y. Obayashi, C. Densham, K. Sasaki, F. Moreau, M. A. Ward, Vincenzo Berardi, E. Poplawska, K. Ueno, Hiroaki Aihara, P. N. Ratoff, P. T. Le, C. Bojechko, R. J. Smith, S. Manly, J. M. Levy, M. Zito, A. Konaka, S. Gomi, Yasuhiro Makida, M. Szeptycka, Leigh H. Whitehead, T. Kutter, A. K. Ichikawa, S. Roth, Federico Sanchez, K. Koseki, Tomoko Ariga, I. Kreslo, T. Sekiguchi, Kimihiro Okumura, A. Cazes, M. Ieva, N. Kulkarni, A. Hillairet, A. Cervera, K. Ieki, V. Palladino, Tsuyoshi Nakaya, J. Kubota, Masayuki Nakahata, Y. Uchida, J. Escallier, C. W. Walter, D. G. Brook-Roberge, H. Kakuno, C. Matsumura, D. Payne, R. Tacik, C. Hearty, A. Delbart, Tatsushi Nakamoto, M. A. George, K. Kaneyuki, Gavin Davies, J. Ilic, L. Ludovici, B. E. Berger, G. Vasseur, S. Murphy, D. Karlen, K. Hamano, T. Tsukamoto, Toru Ogitsu, K. Mavrokoridis, F. d. M. Blaszczyk, P. Kitching, G. Ganetis, Michael Anerella, R. Castillo, Yuichi Oyama, Scott Davis, D. Hansen, M. O. Wascko, R. P. Litchfield, E. Kearns, Masato Shiozawa, L. Zambelli, R. J. Wilkes, B. A. Popov, David Calvet, Hiroyuki Kawamuko, S. Koike, F. Retiere, C. Licciardi, S. J. Ives, S. Assylbekov, A. Haesler, C. A. Miller, Takayuki Tomaru, Biagio Rossi, Hiroyuki Sekiya, I. Taylor, T. Szeglowski, Soo-Bong Kim, B. Still, G. Wikström, S. Bhadra, B. Kirby, C. Strabel, Kendall Mahn, Kate Scholberg, E. Frank, Marco Laveder, M. Hartz, A. Ferrero, W. Toki, S. Nakayama, P. Mijakowski, A. Sarrat, S. Short, N. C. Hastings, U. Dore, A. Thorley, Henry W. Sobel, T. M. Raufer, M. D. Haigh, A. Gendotti, A. Korzenev, Joseph Muratore, P. Wanderer, J. J. Gomez-Cadenas, Yoshinari Hayato, C. Yanagisawa, Gareth J. Barker, Y. Shimizu, Dmitriy Beznosko, J. P. Coleman, Rhiju Das, B. Jamieson, Y. Kurimoto, Michael Litos, P. Gumplinger, C. Touramanis, Antonio Ereditato, N. Yershov, R. L. Helmer, Kevin Scott McFarland, Takashi Kobayashi, D. I. Scully, E. Radicioni, T. Maruyama, Marek Stodulski, T. Nakadaira, A. Yamamoto, F. Khanam, G.D. Barr, D. L. Wark, M. Y. Pac, K. P. Lee, A. Muir, Kodai Matsuoka, R. Terri, T. Hasegawa, S. Mine, A. D. Marino, A. Blondel, S. Sabouri, M. Fechner, Fred Gannaway, J. Marzec, N. J. Buchanan, A. Bravar, O. Araoka, Y. Yamada, K. Nakajima, M. Tada, Hirokatsu Ohhata, S. L. Cartwright, Y. Fukuda, D. Autiero, K. Connolly, T. Yamauchi, S. W. K. Emery, Yasuo Ajima, T. McLachlan, D. Terhorst, K. Abe, R. Sacco, A. Terashima, C. McGrew, C. Andreopoulos, M. L. Navin, H.A. Tanaka, Achim Stahl, N. Tanimoto, J. M. Poutissou, C. Bronner, T. C. Nicholls, Iain Alexander Bertram, J. Imber, S. Moriyama, P. Stamoulis, A. Gaudin, W. Qian, M. B. Smy, A. Zalewska, G. Kogan, J. Swierblewski, M. Shibata, G. De Rosa, H. Nishino, A. Hyndman, R. A. Owen, A. Badertscher, S. M. Oser, M. Macaire, Y. Seiya, J. Schwehr, Y. Takenaga, M. Goldhaber, T. Yuan, K. Mizouchi, Viktor Matveev, Paul Fraser Harrison, T. Okusawa, Jungsang Kim, S. Y. Suzuki, M. Ikeda, Ken Sakashita, Antonin Vacheret, W. R. Kropp, J. F. Martin, M. Tzanov, C. J. Metelko, R. Poutissou, P. Masliah, B. Morgan, A. Hatzikoutelis, J. Y. Kim, R. Sulej, K. K. Joo, T. Wachala, Yusuke Koshio, M. Mezzetto, A. Murakami, T. Nakai, Jing Wang, E. Rondio, P. Dinh Tran, N. McCauley, J. Kameda, P. Przewlocki, Lester D.R. Thompson, K. Hayashi, M. Vagins, B. Andrieu, J. Holeczek, M. Dziomba, Eiichi Hirose, M. Posiadala, M. G. Catanesi, V. Kravtsov, M. Day, A. Longhin, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, T2K, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Abgrall, Nicolas, Argyriades, Jeremy, Blondel, Alain, Bravar, Alessandro, Dufour, Fanny, Ferrero, Andréa, Haesler, Alexis, Korzenev, Alexander, Murphy, Sébastien, Ravonel Salzgeber, Melody, Wikstrom, Gustav, K., Abe, N., Abgrall, Y., Ajima, H., Aihara, J. B., Albert, C., Andreopoulo, B., Andrieu, M. D., Anerella, S., Aoki, O., Araoka, J., Argyriade, A., Ariga, T., Ariga, S., Assylbekov, D., Autiero, A., Badertscher, M., Barbi, G. J., Barker, G., Barr, M., Ba, M., Batkiewicz, F., Bay, S., Bentham, V., Berardi, B. E., Berger, I., Bertram, M., Besnier, J., Beucher, D., Beznosko, S., Bhadra, F. d. M., Blaszczyk, J., Blocki, A., Blondel, C., Bojechko, J., Bouchez, S. B., Boyd, A., Bravar, C., Bronner, D. G., Brook Roberge, N., Buchanan, H., Budd, D., Calvet, S. L., Cartwright, A., Carver, R., Castillo, M. G., Catanesi, A., Caze, A., Cervera, C., Chavez, S., Choi, G., Christodoulou, J., Coleman, G., Collazuol, W., Coleman, K., Connolly, A., Curioni, A., Dabrowska, I., Danko, R., Da, G. S., Davie, S., Davi, M., Day, DE ROSA, Gianfranca, J. P. A. M., de André, P., de Perio, T., Dealtry, A., Delbart, C., Densham, F., Di Lodovico, S., Di Luise, P., Dinh Tran, J., Dobson, U., Dore, O., Drapier, F., Dufour, J., Dumarchez, S., Dytman, M., Dziewiecki, M., Dziomba, S., Emery, A., Ereditato, J. E., Escallier, L., Escudero, L. S., Esposito, M., Fechner, A., Ferrero, A. J., Finch, E., Frank, Y., Fujii, Y., Fukuda, V., Galymov, G. L., Ganeti, F. C., Gannaway, A., Gaudin, A., Gendotti, M., George, S., Giffin, C., Giganti, K., Gilje, A. K., Ghosh, T., Golan, M., Goldhaber, J. J., Gomez Cadena, S., Gomi, M., Gonin, N., Grant, A., Grant, P., Gumplinger, P., Guzowski, A., Haesler, M. D., Haigh, K., Hamano, C., Hansen, D., Hansen, T., Hara, P. F., Harrison, B., Hartfiel, M., Hartz, T., Haruyama, T., Hasegawa, N. C., Hasting, A., Hatzikouteli, K., Hayashi, Y., Hayato, C., Hearty, R. L., Helmer, R., Henderson, N., Higashi, J., Hignight, A., Hillairet, E., Hirose, J., Holeczek, S., Horikawa, A., Hyndman, A. K., Ichikawa, K., Ieki, M., Ieva, M., Iida, M., Ikeda, J., Ilic, J., Imber, T., Ishida, C., Ishihara, T., Ishii, S. J., Ive, M., Iwasaki, K., Iyogi, A., Izmaylov, B., Jamieson, R. A., Johnson, K. K., Joo, G. V., Jover Mana, C. K., Jung, H., Kaji, T., Kajita, H., Kakuno, J., Kameda, K., Kaneyuki, D., Karlen, K., Kasami, I., Kato, H., Kawamuko, E., Kearn, M., Khabibullin, F., Khanam, A., Khotjantsev, D., Kielczewska, T., Kikawa, J., Kim, J. Y., Kim, S. B., Kim, N., Kimura, B., Kirby, J., Kisiel, P., Kitching, T., Kobayashi, G., Kogan, S., Koike, A., Konaka, L. L., Kormo, A., Korzenev, K., Koseki, Y., Koshio, Y., Kouzuma, K., Kowalik, V., Kravtsov, I., Kreslo, W., Kropp, H., Kubo, J., Kubota, Y., Kudenko, N., Kulkarni, Y., Kurimoto, R., Kurjata, T., Kutter, J., Lagoda, K., Laihem, M., Laveder, K. P., Lee, P. T., Le, J. M., Levy, C., Licciardi, I. T., Lim, T., Lindner, R. P., Litchfield, M., Lito, A., Longhin, G. D., Lopez, P. F., Loverre, L., Ludovici, T., Lux, M., Macaire, K., Mahn, Y., Makida, M., Malek, S., Manly, A., Marchionni, A. D., Marino, A. J., Marone, J., Marteau, J. F., Martin, T., Maruyama, T., Maryon, J., Marzec, P., Masliah, E. L., Mathie, C., Matsumura, K., Matsuoka, V., Matveev, K., Mavrokoridi, E., Mazzucato, N., Mccauley, K. S., Mcfarland, C., Mcgrew, T., Mclachlan, M., Messina, W., Metcalf, C., Metelko, M., Mezzetto, P., Mijakowski, C. A., Miller, A., Minamino, O., Mineev, S., Mine, A. D., Missert, G., Mituka, M., Miura, K., Mizouchi, L., Monfregola, F., Moreau, B., Morgan, S., Moriyama, A., Muir, A., Murakami, J. F., Muratore, M., Murdoch, S., Murphy, J., Myslik, N., Nagai, T., Nakadaira, M., Nakahata, T., Nakai, K., Nakajima, T., Nakamoto, K., Nakamura, S., Nakayama, T., Nakaya, D., Naple, M. L., Navin, B., Nelson, T. C., Nicholl, C., Nielsen, K., Nishikawa, H., Nishino, K., Nitta, T., Nobuhara, J. A., Nowak, Y., Obayashi, T., Ogitsu, H., Ohhata, T., Okamura, K., Okumura, T., Okusawa, S. M., Oser, M., Otani, R. A., Owen, Y., Oyama, T., Ozaki, M. Y., Pac, Palladino, Vittorio, V., Paolone, P., Paul, D., Payne, G. F., Pearce, J. D., Perkin, V., Pettinacci, F., Pierre, E., Poplawska, B., Popov, M., Posiadala, J. M., Poutissou, R., Poutissou, P., Przewlocki, W., Qian, J. L., Raaf, E., Radicioni, P. N., Ratoff, T. M., Raufer, M., Ravonel, M., Raymond, F., Retiere, A., Robert, P. A., Rodrigue, E., Rondio, J. M., Roney, B., Rossi, S., Roth, A., Rubbia, D., Ruterborie, S., Sabouri, R., Sacco, K., Sakashita, F., Sánchez, A., Sarrat, K., Sasaki, K., Scholberg, J., Schwehr, M., Scott, D. I., Scully, Y., Seiya, T., Sekiguchi, H., Sekiya, M., Shibata, Y., Shimizu, M., Shiozawa, S., Short, M., Siyad, R. J., Smith, M., Smy, J. T., Sobczyk, H., Sobel, M., Sorel, A., Stahl, P., Stamouli, J., Steinmann, B., Still, J., Stone, M., Stodulski, C., Strabel, R., Sulej, A., Suzuki, K., Suzuki, S., Suzuki, S. Y., Suzuki, Y., Suzuki, J., Swierblewski, T., Szeglowski, M., Szeptycka, R., Tacik, M., Tada, M., Taguchi, S., Takahashi, A., Takeda, Y., Takenaga, Y., Takeuchi, K., Tanaka, H. A., Tanaka, M., Tanaka, M. M., Tanaka, N., Tanimoto, K., Tashiro, I., Taylor, A., Terashima, D., Terhorst, R., Terri, L. F., Thompson, A., Thorley, W., Toki, S., Tobayama, T., Tomaru, Y., Totsuka, C., Touramani, T., Tsukamoto, M., Tzanov, Y., Uchida, K., Ueno, A., Vacheret, M., Vagin, G., Vasseur, T., Wachala, J. J., Walding, A. V., Waldron, C. W., Walter, P. J., Wanderer, J., Wang, M. A., Ward, G. P., Ward, D., Wark, M. O., Wascko, A., Weber, R., Wendell, N., West, L. H., Whitehead, G., Wikström, R. J., Wilke, M. J., Wilking, Z., Williamson, J. R., Wilson, R. J., Wilson, T., Wongjirad, S., Yamada, Y., Yamada, A., Yamamoto, K., Yamamoto, Y., Yamanoi, H., Yamaoka, T., Yamauchi, C., Yanagisawa, T., Yano, S., Yen, N., Yershov, M., Yokoyama, T., Yuan, A., Zalewska, J., Zalipska, L., Zambelli, K., Zaremba, M., Ziembicki, E. D., Zimmerman, M., Zito, and J., Zmuda
Subjects: Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Neutrino oscillation, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, on-axis near detector, FOS: Physical sciences, ddc:500.2, 01 natural sciences, 7. Clean energy, neutrino oscillation, neutrino detector, wavelength shifting fiber, t2k, extruded scintillator, neutrino beam, Neutrino detector, Nuclear physics, Neutrino beam, 0103 physical sciences, Extruded scintillator, Muon neutrino, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, T2K, Physics, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Wavelength shifting fiber, T2K experiment, Física, Instrumentation and Detectors (physics.ins-det), Wavelength shiftingfiber, Measurements of neutrino speed, Physics::Accelerator Physics, High Energy Physics::Experiment, Neutrino, Beam (structure), Lepton
Abstract: Precise measurement of neutrino beam direction and intensity was achieved based on a new concept with modularized neutrino detectors. INGRID (Interactive Neutrino GRID) is an on-axis near detector for the T2K long baseline neutrino oscillation experiment. INGRID consists of 16 identical modules arranged in horizontal and vertical arrays around the beam center. The module has a sandwich structure of iron target plates and scintillator trackers. INGRID directly monitors the muon neutrino beam profile center and intensity using the number of observed neutrino events in each module. The neutrino beam direction is measured with accuracy better than 0.4 mrad from the measured profile center. The normalized event rate is measured with 4% precision., Comment: 32 pages, 27 figures, submitted to Nucl. Instr. and Meth. A
Published: 2012
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41. Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam

Author: S. Roth, J. Lagoda, M. Iwasaki, Paul Fraser Harrison, T. Okusawa, Jungsang Kim, S. Y. Suzuki, M. Ikeda, M. Bass, F. Pierre, R. A. Wendell, C. Bojechko, C. W. Walter, B. A. Popov, Vincenzo Berardi, P. T. Le, P. Mijakowski, C. Licciardi, Tomoko Ariga, J. Ilic, M. Ravonel, T. Maruyama, E. L. Mathie, V. Galymov, T. Ishii, M. A. George, I. Taylor, G. Vasseur, T. Nakadaira, Kazuhiro Suzuki, M. Ieva, Hirokatsu Ohhata, Y. Fukuda, D. Autiero, P. Paul, Kate Scholberg, M. M. Khabibullin, A. Yamamoto, Toru Ogitsu, F. Khanam, G.D. Barr, T. Maryon, Michel Raymond, P. Kitching, R. Tacik, M. Hartz, G. Christodoulou, S. B. Boyd, J. R. Wilson, K. K. Joo, T. Wachala, E. Frank, M. O. Wascko, C. A. Chavez, Marco Laveder, A. Ferrero, B. Hartfiel, A. C. Weber, E. Kearns, K. P. Lee, Justin Albert, N. Abgrall, M. Szeptycka, M. M. Tanaka, Leigh H. Whitehead, J. P.A.M. De André, E. Mazzucato, Sy Suzuki, Y. Obayashi, K. Mavrokoridis, G. F. Pearce, J. J. Walding, A. Suzuki, J. Myslik, N. Grant, André Rubbia, M. Murdoch, S. W. K. Emery, Masayuki Nakahata, P. de Perio, G. Collazuol, Mark Scott, Yusuke Koshio, Masashi Tanaka, S. Yen, T. Ishida, Yoshikazu Yamada, F. d. M. Blaszczyk, T. Yano, T. Golan, Biagio Rossi, Hiroyuki Sekiya, Y. Uchida, C. Hansen, C. A. Miller, A. Minamino, M. Day, V. Paolone, P. Sutcliffe, Masashi Yokoyama, E. Poplawska, R. Poutissou, Hs Budd, P. Masliah, T. Szeglowski, Soo-Bong Kim, A. Longhin, Michael Litos, J. Marteau, O. Drapier, K. Iyogi, F. Moreau, E. D. Zimmerman, M. Iida, B. Morgan, M. A. Ward, Tomiyoshi Haruyama, J. M. Levy, L. L. Kormos, T. Kikawa, C. Touramanis, Kendall Mahn, Robert Henderson, A. Hatzikoutelis, H. Kaji, R. A. Johnson, Antonio Ereditato, H. Nishino, M. Zito, N. Yershov, A. Cazes, K. Zaremba, B. Kirby, I. Kreslo, J. Dumarchez, Kevin Scott McFarland, A. Cervera, Henry W. Sobel, V. Palladino, Tsuyoshi Nakaya, Takashi Kobayashi, M. Malek, J. Y. Kim, J. Kisiel, T. M. Raufer, T. Hasegawa, S. Mine, Y. Takeuchi, A. Delbart, J. D. Perkin, Scott Davis, D. Hansen, R. Sulej, Atsushi Takeda, Takaaki Kajita, G. D. Lopez, Oleg Mineev, K. Hamano, R. Castillo, Yuichi Oyama, T. Tsukamoto, S. J. Ives, R. P. Litchfield, Takayuki Tomaru, Masato Shiozawa, M. Ziembicki, S. Sabouri, Ken Sakashita, Norio Higashi, J. Zalipska, Minoru Otani, David Calvet, C. Strabel, S. Assylbekov, M. Siyad, V. Pettinacci, K. Gilje, A. Zalewska, Federico Sanchez, M. Fechner, A. Haesler, Fred Gannaway, Alexander Finch, D. Ruterbories, G. Wikström, S. Bhadra, Akitaka Ariga, Antonin Vacheret, W. R. Kropp, K. Kowalik, J. Marzec, C. Matsumura, D. Payne, T. Hara, J. F. Martin, M. Tzanov, C. J. Metelko, Koji Nakamura, M. Barbi, Hiroaki Aihara, G. Jover-Manas, A. Carver, Shigeki Aoki, P. N. Ratoff, T. Kutter, S. Giffin, A. N. Khotjantsev, Y. Fujii, W. Coleman, A. Gendotti, A. Missert, F. Bay, M. Miura, T. Ozaki, A. Muir, Kodai Matsuoka, P. Guzowski, A. Bravar, Frédéric Dufour, C. Yanagisawa, K. Nishikawa, G. P. Ward, I. T. Lim, R. Terri, J. Holeczek, P. Wanderer, J. J. Gomez-Cadenas, Michal Dziewiecki, Kazuhiro Yamamoto, Jan T. Sobczyk, K. Laihem, N. Kimura, H. Kubo, K. Nakajima, M. Tada, P. Gumplinger, R. L. Helmer, Gareth J. Barker, Kimihiro Okumura, K. Koseki, Y. Shimizu, Dmitriy Beznosko, D. G. Brook-Roberge, S. M. Oser, J. P. Coleman, Y. Seiya, J. Schwehr, Yasuo Ajima, T. McLachlan, S. Horikawa, A. Blondel, M. Goldhaber, S. Yamada, K. Ieki, D. Karlen, R. J. Wilkes, D. I. Scully, N. J. Buchanan, P. A. Rodrigues, E. Radicioni, M. L. Navin, H.A. Tanaka, Yoshinari Hayato, C. K. Jung, D. L. Wark, M. Y. Pac, Achim Stahl, J. L. Stone, D. Kielczewska, A. Dabrowska, A. D. Marino, J. M. Poutissou, C. Bronner, N. West, I. Kato, K. Kaneyuki, T. C. Nicholls, Gavin Davies, U. Dore, P. Stamoulis, A. Thorley, A. Korzenev, L. Ludovici, M. Sorel, A. Gaudin, W. Qian, T. Lindner, C. Densham, G. Kogan, G. De Rosa, S. Hastings, R. A. Owen, M. D. Haigh, A. Badertscher, M. Macaire, Y. Takenaga, M. J. Wilking, Rhiju Das, S. Dytman, B. Jamieson, J. L. Raaf, J. Bouchez, Thorsten Lux, O. Araoka, M. Gonin, L. Escudero, Kenichi Tanaka, J. Steinmann, K. Abe, R. Sacco, S. L. Cartwright, A. Terashima, C. McGrew, K. Connolly, C. Andreopoulos, D. Terhorst, T. Nakai, Jing Wang, E. Rondio, P. Dinh Tran, N. McCauley, K. Mizouchi, Viktor Matveev, M. Noy, N. Tanimoto, Iain Alexander Bertram, J. Imber, S. Moriyama, M. B. Smy, M. Shibata, A. Hyndman, J. Kameda, P. Przewlocki, P. F. Loverre, J. M. Roney, Lester D.R. Thompson, Y. Kouzuma, L. R. Sulak, M. Mezzetto, R.P. Kurjata, S. W. Bentham, I. Z. Danko, K. Sasaki, K. Tashiro, Koh Ueno, Katsuyu Kasami, Yasuhiro Makida, N. Kulkarni, C. Hearty, T. Sekiguchi, Tatsushi Nakamoto, Alastair Grant, Richard J.H. Smith, G. Mituka, A. Murakami, Yutaka Yamanoi, Hiroshi Yamaoka, A. Marchionni, S. Di Luise, F. Di Lodovico, A. Curioni, K. Hayashi, Barry L. Nelson, Yu. G. Kudenko, L. Monfregola, S. Koike, S. Manly, M. Vagins, B. Andrieu, C. Giganti, B. Still, J. A. Nowak, C. Ishihara, M. Dziomba, Eiichi Hirose, M. Posiadala, M. G. Catanesi, V. Kravtsov, S. Murphy, F. Retiere, Y. Totsuka, Susumu Takahashi, W. Metcalf, T. Wongjirad, S. Nakayama, A. Sarrat, S. Short, N. C. Hastings, D. Naples, A. Robert, A. Izmaylov, Steve K. Choi, J. Zmuda, M. Messina, A. V. Waldron, M. Besnier, J. Dobson, Joshua Hignight, Yoshihiro Suzuki, Robert Wilson, Takahiro Okamura, J. Argyriades, J. Beucher, A. Konaka, W. H. Toki, B. E. Berger, H. Kakuno, L. Zambelli, A. K. Ichikawa, Luigi Salvatore Esposito, Escudero Sanchez, Lorena [0000-0003-3464-9206], Whitehead, Leigh [0000-0002-3327-2534], Apollo - University of Cambridge Repository, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Département d'Electronique, des Détecteurs et d'Informatique (ex SEDI) (DEDI), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, T2K, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département d'Electronique, des Détecteurs et d'Informatique pour la Physique (ex SEDI) (DEDIP), Abgrall, Nicolas, Argyriades, Jeremy, Blondel, Alain, Bravar, Alessandro, Dufour, Fanny, Ferrero, Andréa, Haesler, Alexis, Korzenev, Alexander, Murphy, Sébastien, Ravonel Salzgeber, Melody, Wikstrom, Gustav, K., Abe, N., Abgrall, Y., Ajima, H., Aihara, J., Albert, C., Andreopoulo, B., Andrieu, S., Aoki, O., Araoka, J., Argyriade, A., Ariga, T., Ariga, S., Assylbekov, D., Autiero, A., Badertscher, M., Barbi, G., Barker, G., Barr, M., Ba, F., Bay, S., Bentham, V., Berardi, B., Berger, I., Bertram, M., Besnier, J., Beucher, D., Beznosko, S., Bhadra, F., Blaszczyk, A., Blondel, C., Bojechko, J., Bouchez, S., Boyd, A., Bravar, C., Bronner, D., Brook Roberge, N., Buchanan, H., Budd, D., Calvet, S., Cartwright, A., Carver, R., Castillo, M., Catanesi, A., Caze, A., Cervera, C., Chavez, S., Choi, G., Christodoulou, J., Coleman, W., Coleman, G., Collazuol, K., Connolly, A., Curioni, A., Dabrowska, I., Danko, R., Da, G., Davie, S., Davi, M., Day, DE ROSA, Gianfranca, J., de André, P., de Perio, A., Delbart, C., Densham, F., Di Lodovico, S., Di Luise, P., Dinh Tran, J., Dobson, U., Dore, O., Drapier, F., Dufour, J., Dumarchez, S., Dytman, M., Dziewiecki, M., Dziomba, S., Emery, A., Ereditato, L., Escudero, L., Esposito, M., Fechner, A., Ferrero, A., Finch, E., Frank, Y., Fujii, Y., Fukuda, V., Galymov, F., Gannaway, A., Gaudin, A., Gendotti, M., George, S., Giffin, C., Giganti, K., Gilje, T., Golan, M., Goldhaber, J., Gomez Cadena, M., Gonin, N., Grant, A., Grant, P., Gumplinger, P., Guzowski, A., Haesler, M., Haigh, K., Hamano, C., Hansen, D., Hansen, T., Hara, P., Harrison, B., Hartfiel, M., Hartz, T., Haruyama, T., Hasegawa, N., Hasting, S., Hasting, A., Hatzikouteli, K., Hayashi, Y., Hayato, C., Hearty, R., Helmer, R., Henderson, N., Higashi, J., Hignight, E., Hirose, J., Holeczek, S., Horikawa, A., Hyndman, A., Ichikawa, K., Ieki, M., Ieva, M., Iida, M., Ikeda, J., Ilic, J., Imber, T., Ishida, C., Ishihara, T., Ishii, S., Ive, M., Iwasaki, K., Iyogi, A., Izmaylov, B., Jamieson, R., Johnson, K., Joo, G., Jover Mana, C., Jung, H., Kaji, T., Kajita, H., Kakuno, J., Kameda, K., Kaneyuki, D., Karlen, K., Kasami, I., Kato, E., Kearn, M., Khabibullin, F., Khanam, A., Khotjantsev, D., Kielczewska, T., Kikawa, J., Kim, S., Kim, N., Kimura, B., Kirby, J., Kisiel, P., Kitching, T., Kobayashi, G., Kogan, S., Koike, A., Konaka, L., Kormo, A., Korzenev, K., Koseki, Y., Koshio, Y., Kouzuma, K., Kowalik, V., Kravtsov, I., Kreslo, W., Kropp, H., Kubo, Y., Kudenko, N., Kulkarni, R., Kurjata, T., Kutter, J., Lagoda, K., Laihem, M., Laveder, K., Lee, P., Le, J., Levy, C., Licciardi, I., Lim, T., Lindner, R., Litchfield, M., Lito, A., Longhin, G., Lopez, P., Loverre, L., Ludovici, T., Lux, M., Macaire, K., Mahn, Y., Makida, M., Malek, S., Manly, A., Marchionni, A., Marino, J., Marteau, J., Martin, T., Maruyama, T., Maryon, J., Marzec, P., Masliah, E., Mathie, C., Matsumura, K., Matsuoka, V., Matveev, K., Mavrokoridi, E., Mazzucato, N., Mccauley, K., Mcfarland, C., Mcgrew, T., Mclachlan, M., Messina, W., Metcalf, C., Metelko, M., Mezzetto, P., Mijakowski, C., Miller, A., Minamino, O., Mineev, S., Mine, A., Missert, G., Mituka, M., Miura, K., Mizouchi, L., Monfregola, F., Moreau, B., Morgan, S., Moriyama, A., Muir, A., Murakami, M., Murdoch, S., Murphy, J., Myslik, T., Nakadaira, M., Nakahata, T., Nakai, K., Nakajima, T., Nakamoto, K., Nakamura, S., Nakayama, T., Nakaya, D., Naple, M., Navin, B., Nelson, T., Nicholl, K., Nishikawa, H., Nishino, J., Nowak, M., Noy, Y., Obayashi, T., Ogitsu, H., Ohhata, T., Okamura, K., Okumura, T., Okusawa, S., Oser, M., Otani, R., Owen, Y., Oyama, T., Ozaki, M., Pac, Palladino, Vittorio, V., Paolone, P., Paul, D., Payne, G., Pearce, J., Perkin, V., Pettinacci, F., Pierre, E., Poplawska, B., Popov, M., Posiadala, J. M., Poutissou, R., Poutissou, P., Przewlocki, W., Qian, J., Raaf, E., Radicioni, P., Ratoff, T., Raufer, M., Ravonel, M., Raymond, F., Retiere, A., Robert, P., Rodrigue, E., Rondio, J., Roney, B., Rossi, S., Roth, A., Rubbia, D., Ruterborie, S., Sabouri, R., Sacco, K., Sakashita, F., Sánchez, A., Sarrat, K., Sasaki, K., Scholberg, J., Schwehr, M., Scott, D., Scully, Y., Seiya, T., Sekiguchi, H., Sekiya, M., Shibata, Y., Shimizu, M., Shiozawa, S., Short, M., Siyad, R., Smith, M., Smy, J., Sobczyk, H., Sobel, M., Sorel, A., Stahl, P., Stamouli, J., Steinmann, B., Still, J., Stone, C., Strabel, L., Sulak, R., Sulej, P., Sutcliffe, A., Suzuki, K., Suzuki, S., Suzuki, Y., Suzuki, T., Szeglowski, M., Szeptycka, R., Tacik, M., Tada, S., Takahashi, A., Takeda, Y., Takenaga, Y., Takeuchi, K., Tanaka, H., Tanaka, M., Tanaka, N., Tanimoto, K., Tashiro, I., Taylor, A., Terashima, D., Terhorst, R., Terri, L., Thompson, A., Thorley, W., Toki, T., Tomaru, Y., Totsuka, C., Touramani, T., Tsukamoto, M., Tzanov, Y., Uchida, K., Ueno, A., Vacheret, M., Vagin, G., Vasseur, T., Wachala, J., Walding, A., Waldron, C., Walter, P., Wanderer, J., Wang, M., Ward, G., Ward, D., Wark, M., Wascko, A., Weber, R., Wendell, N., West, L., Whitehead, G., Wikström, R., Wilke, M., Wilking, J., Wilson, R., Wilson, T., Wongjirad, S., Yamada, Y., Yamada, A., Yamamoto, K., Yamamoto, Y., Yamanoi, H., Yamaoka, C., Yanagisawa, T., Yano, S., Yen, N., Yershov, M., Yokoyama, A., Zalewska, J., Zalipska, L., Zambelli, K., Zaremba, M., Ziembicki, E., Zimmerman, M., Zito, J., ??muda, and Walter, Christopher W
Subjects: Particle physics, FOS: Physical sciences, General Physics and Astronomy, ddc:500.2, CHOOZ, 01 natural sciences, Particle identification, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), neutrino, 14.60.Pq, 13.15.+g, 25.30.Pt, 95.55.Vj, 0103 physical sciences, neutrino oscillation, Muon neutrino, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Neutrino oscillation, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), ComputingMilieux_MISCELLANEOUS, Physics, NOνA, Tribimaximal mixing, hep-ex, 010308 nuclear & particles physics, T2K experiment, Física, T2K Collaboration, particle identification, Electron neutrino, experimental results
Abstract: The T2K experiment observes indications of $\nu_\mu\rightarrow \nu_e$ appearance in data accumulated with $1.43\times10^{20}$ protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino oscillation scenario with $|\Delta m_{23}^2|=2.4\times10^{-3}$ eV$^2$, $\sin^2 2\theta_{23}=1$ and $\sin^2 2\theta_{13}=0$, the expected number of such events is 1.5$\pm$0.3(syst.). Under this hypothesis, the probability to observe six or more candidate events is 7$\times10^{-3}$, equivalent to 2.5$\sigma$ significance. At 90% C.L., the data are consistent with 0.03(0.04)$, Comment: 20 pages, 6 figures, version published in PRL
Published: 2011
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42. Adipose cells induce phospho-Thr-172 AMPK production by epinephrine or CL316243 in mouse 3T3-L1 adipocytes or MAPK activation and G protein-associated PI3K responses induced by CL316243 or aluminum fluoride in rat white adipocytes

Author: Y, Ohsaka, H, Nishino, and Y, Nomura
Subjects: Epinephrine, Adipocytes, White, Dioxoles, AMP-Activated Protein Kinases, Rats, Fluorides, Mice, Phosphatidylinositol 3-Kinases, Phosphothreonine, Pertussis Toxin, GTP-Binding Proteins, 3T3-L1 Cells, Animals, Immunoprecipitation, Mitogen-Activated Protein Kinases, Aluminum Compounds
Abstract: Responses of adipose cells to adrenoceptor regulation, including that of β-adrenoceptor (AR), and the signalling machinery involved in these responses are not sufficiently understood; information that is helpful for elucidating the adrenoceptor (adrenergic and β-AR)-responsive machinery is insufficient. We examined phospho-Thr-172 AMPK production in mouse-derived 3T3-L1 adipocytes treated with epinephrine or CL316243 (a β3-AR agonist) for 15 min. We also examined MAPK activation or G protein-associated PI3K activation or -associated PI3K p85 complex formation in rat epididymal (white) adipocytes treated with CL316243 for 15 min or aluminum fluoride (a G-protein signalling activator) for 20 min. Furthermore, we examined the effect of PTX (a trimeric G-protein inactivator) on p85 complex formation induced by aluminum fluoride treatment. Western blot analysis revealed that epinephrine or CL316243 treatment increased the phospho- Thr-172 AMPK (an active form of AMPK) level in 3T3-L1 adipocytes. Activated kinase analysis with a specific substrate showed that CL316243 or aluminum fluoride treatment activated MAPK in rat adipocytes. Immunoprecipitation experiments with a G-protein β subunit (Gβ) antibody showed that treatment of rat adipocytes with CL316243 activated PI3K and increased the PI3K p85 level in the Gβ antibody immunoprecipitates. Such an increase in the p85 level was similarly elicited by aluminum fluoride treatment in a PTX-sensitive manner. Our results provide possible clues for clarifying the signalling machinery involved in adrenoceptor responses, including those of β3-AR, in mouse-derived adipocytes and rat white adipocytes. Our findings advance the understanding of responses to adrenoceptor regulation in adipose cells and of the cellular signalling machinery present in the cells.
Published: 2014

43. LiteBIRD: mission overview and design tradeoffs

Author: N. Katayama, H. Nishino, K. Karatsu, Hirokazu Ishino, Shogo Nakamura, H. Morii, J. Borrill, Shin-ichiro Sakai, H. Ishitsuka, Paul L. Richards, S. Takakura, Hiroki Watanabe, Osamu Tajima, Y. Kibe, K. Koga, Suguru Takada, K. Natsume, Nobuhiro Kimura, T. Morishima, K. Yotsumoto, Kazuhisa Mitsuda, Yutaro Sekimoto, Yoh Takei, Chiko Otani, Takashi Noguchi, Koji Ishidoshiro, Shugo Oguri, Y. Hori, Eiichiro Komatsu, Y. Sato, Masato Naruse, Ryo Nagata, Yuki Inoue, Noriko Y. Yamasaki, J. Inatani, Y. Akiba, Y. Segawa, K. Nishijo, N. Sato, T. Yoshida, Shingo Kashima, A. Kibayashi, Masaya Hasegawa, Yoshinori Uzawa, Hiroyuki Sugita, W. L. Holzapfel, Takehiko Wada, Toshiyuki Nishibori, Isao Kawano, Abraham P. Lee, Mitsuhiro Yoshida, T. Suzuki, Makoto Nagai, Keisuke Shinozaki, M. Inoue, M. Hattori, Kaori Hattori, T. Namikawa, M. A. Dobbs, Masashi Hazumi, H. Fuke, I. S. Ohta, K. Mizukami, Yasuhiro Yamada, Aritoki Suzuki, Tomotake Matsumura, Takayuki Tomaru, N. Okada, Hideo Matsuhara, Atsushi Noda, Satoru Mima, M. Kozu, Yuji Chinone, H. Yamaguchi, Hideo Ogawa, and Kimihiro Kimura
Subjects: Physics, Satellite bus, Mission design, Cosmic microwave background, Systems engineering, Satellite, Orbital mechanics, Remote sensing
Abstract: We present the mission design of LiteBIRD, a next generation satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation (CMB) detection. The science goal of LiteBIRD is to measure the CMB polarization with the sensitivity of δr = 0:001, and this allows testing the major single-field slow-roll inflation models experimentally. The LiteBIRD instrumental design is purely driven to achieve this goal. At the earlier stage of the mission design, several key instrumental specifications, e.g. observing band, optical system, scan strategy, and orbit, need to be defined in order to process the rest of the detailed design. We have gone through the feasibility studies for these items in order to understand the tradeoffs between the requirements from the science goal and the compatibilities with a satellite bus system. We describe the overview of LiteBIRD and discuss the tradeoffs among the choices of scientific instrumental specifications and strategies. The first round of feasibility studies will be completed by the end of year 2014 to be ready for the mission definition review and the target launch date is in early 2020s.
Published: 2014
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44. System Organization of a Multiple-Cockpit Digital Operational Flight Trainer.

Author: Harry J. Gray Jr., Hiroshi H. Nishino, and Alvin L. Vivatson
Published: 1959
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45. Search for Dinucleon Decay into Kaons in Super-Kamiokande

Author: T. Tsukamoto, A. T. Suzuki, T. Nakadaira, Makoto Sakuda, Masato Shiozawa, Y. Choi, Minoru Yoshida, B. S. Yang, T. Ishida, M. Ikeda, Haoxiong Zhang, S. Hazama, R. Terri, T. Hasegawa, T. Ishizuka, K. Sakashita, Y. Takenaga, C. McGrew, Yoshihiro Suzuki, M. Miura, N. Tamura, Takaaki Mori, Y. Totsuka, T. Wongjirad, J. L. Stone, Ken-ichiro Kobayashi, Koji Nakamura, Henry W. Sobel, K. Iyogi, Y. Takeuchi, B. Henning, M. Goldhaber, J. P. Cravens, Shigeki Tasaka, E. Thrane, N. Tanimoto, K. Ueshima, T. Kajita, A. Kibayashi, Shigetaka Moriyama, Yoshitaka Itow, T. Ishii, H. Kaji, J. S. Jang, Tsutomu Yokozawa, T. McLachlan, Hiroshi Watanabe, M. B. Smy, K. Connolly, Zishuo Yang, Kate Scholberg, Michael Litos, Atsushi Takeda, C. W. Walter, John Hill, Justin Albert, H. Okazawa, Y. Kuno, T. Kobayashi, G. Mitsuka, S. B. Kim, J. Y. Kim, R. J. Wilkes, S. Mino, Hirokazu Ishino, I. T. Lim, W. E. Keig, Masashi Yokoyama, David William Casper, M. Vagins, K. Kaneyuki, H. Nishino, H. Ogawa, Y. Shimizu, J. G. Learned, Yuichi Oyama, M. Dziomba, K. Nishijima, K. Nishikawa, Y. Kozuma, K. Abe, C. Ishihara, Masayuki Nakahata, S. Mine, Tsuyoshi Nakaya, M. Koshiba, S. Matsuno, Tetsuya S. Tanaka, Ko Okumura, Y. Hayato, L. R. Sulak, K. S. Ganezer, G. Lopez, Yusuke Koshio, Koh Ueno, A. Minamino, C. Yanagisawa, S. Nakayama, R. A. Wendell, J. Kameda, P. Mijakowski, E. Kearns, T. Sekiguchi, K. Bays, Hiroyuki Sekiya, Y. Fukuda, Y. Heng, Frédéric Dufour, Song Chen, T. Iida, H. Toyota, C. Regis, C. K. Jung, J. L. Raaf, D. Kielczewska, Y. Watanabe, Y. Yokosawa, Y. Obayashi, W. R. Kropp, and S. Yamada
Subjects: Physics, Particle physics, Bound state, General Physics and Astronomy, Atmospheric neutrino, Super-Kamiokande, Lower limit
Abstract: A search for the dinucleon decay $pp\ensuremath{\rightarrow}{K}^{+}{K}^{+}$ has been performed using $91.6\text{ }\text{ }\mathrm{kton}\ifmmode\cdot\else\textperiodcentered\fi{}\text{yr}$ data from Super-Kamiokande-I. This decay provides a sensitive probe of the $R$-parity-violating parameter ${{\ensuremath{\lambda}}_{112}}^{\ensuremath{'}\ensuremath{'}}$. A boosted decision tree analysis found no signal candidates in the data. The expected background was $0.28\ifmmode\pm\else\textpm\fi{}0.19$ atmospheric neutrino induced events and the estimated signal detection efficiency was $12.6%\ifmmode\pm\else\textpm\fi{}3.2%$. A lower limit of $1.7\ifmmode\times\else\texttimes\fi{}{10}^{32}\text{ }\text{ }\text{years}$ has been placed on the partial lifetime of the decay $^{16}\mathrm{O}\ensuremath{\rightarrow}^{14}\mathrm{C}{K}^{+}{K}^{+}$ at 90% C.L. A corresponding upper limit of $7.8\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}9}$ has been placed on the parameter ${{\ensuremath{\lambda}}_{112}}^{\ensuremath{'}\ensuremath{'}}$.
Published: 2014
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46. Evidence for Gravitational Lensing of the Cosmic Microwave Background Polarization from Cross-Correlation with the Cosmic Infrared Background

Author: Aritoki Suzuki, Frederick Matsuda, Daniel Flanigan, Meir Shimon, Kam Arnold, Nathan J. Miller, Colin Ross, X. Meng, Y. Akiba, S. Takakura, A. E. Anthony, Y. Hori, Josquin Errard, D. Poletti, Julian Borrill, Hans P. Paar, Tomotake Matsumura, Yuki Inoue, Yuji Chinone, Takayuki Tomaru, W. L. Holzapfel, D. E. Schenck, Jonathon Howard, S. Moyerman, Tucker Elleflot, M. A. Dobbs, Nathan Stebor, P. Hyland, A. Tikhomirov, Paul L. Richards, I. Schanning, M. Le Jeune, Eric V. Linder, Masaya Hasegawa, Christian L. Reichardt, Giulio Fabbian, M. Atlas, Andrew H. Jaffe, J. Peloton, H. Morii, Oliver Zahn, A. Shimizu, Kaori Hattori, E. M. Leitch, Helmuth Spieler, Scott Chapman, N. W. Halverson, E. Quealy, Masashi Hazumi, William F. Grainger, M. J. Myers, Graeme Smecher, Chang Feng, Blake D. Sherwin, Darcy Barron, Theodore Kisner, Marius Lungu, Reijo Keskitalo, Bryan Steinbach, G. Jaehnig, Peter A. R. Ade, Praween Siritanasak, Kaja Rotermund, Gabriel M. Rebeiz, Amit P. S. Yadav, M. Navaroli, Colin Borys, Zigmund Kermish, Radek Stompor, Adrian T. Lee, A. J. Gilbert, B. Wilson, Brian Keating, D. Boettger, Chase Owen Shimmin, H. Nishino, Dalhousie University [Halifax], AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), The University of Tokyo (UTokyo), University of California [San Diego] (UC San Diego), University of California, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), The University of Tokyo, Ade, P, Akiba, Y, Anthony, A, Arnold, K, Atlas, M, Barron, D, Boettger, D, Borrill, J, Borys, C, Chapman, S, Chinone, Y, Dobbs, M, Elleflot, T, Errard, J, Fabbian, G, Feng, C, Flanigan, D, Gilbert, A, Grainger, W, Halverson, N, Hasegawa, M, Hattori, K, Hazumi, M, Holzapfel, W, Hori, Y, Howard, J, Hyland, P, Inoue, Y, Jaehnig, G, Jaffe, A, Keating, B, Kermish, Z, Keskitalo, R, Kisner, T, Le Jeune, M, Lee, A, Leitch, E, Linder, E, Lungu, M, Matsuda, F, Matsumura, T, Meng, X, Miller, N, Morii, H, Moyerman, S, Myers, M, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Poletti, D, Quealy, E, Rebeiz, G, Reichardt, C, Richards, P, Ross, C, Rotermund, K, Schanning, I, Schenck, D, Sherwin, B, Shimizu, A, Shimmin, C, Shimon, M, Siritanasak, P, Smecher, G, Spieler, H, Stebor, N, Steinbach, B, Stompor, R, Suzuki, A, Takakura, S, Tikhomirov, A, Tomaru, T, Wilson, B, Yadav, A, Zahn, O, APC - Gravitation (APC-Gravitation), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, POLARBEAR, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and University of California (UC)
Subjects: Physics, Gravitational Lensing, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Strong gravitational lensing, Cosmic microwave background, Astrophysics::Instrumentation and Methods for Astrophysics, General Physics and Astronomy, Astronomy, Spectral density, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Polarization (waves), Cosmology, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Gravitational lens, Settore FIS/05 - Astronomia e Astrofisica, Cosmic infrared background, Cosmic Microwave Background, Weak gravitational lensing, ComputingMilieux_MISCELLANEOUS, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We reconstruct the gravitational lensing convergence signal from Cosmic Microwave Background (CMB) polarization data taken by the POLARBEAR experiment and cross-correlate it with Cosmic Infrared Background (CIB) maps from the Herschel satellite. From the cross-spectra, we obtain evidence for gravitational lensing of the CMB polarization at a statistical significance of 4.0$\sigma$ and evidence for the presence of a lensing $B$-mode signal at a significance of 2.3$\sigma$. We demonstrate that our results are not biased by instrumental and astrophysical systematic errors by performing null-tests, checks with simulated and real data, and analytical calculations. This measurement of polarization lensing, made via the robust cross-correlation channel, not only reinforces POLARBEAR auto-correlation measurements, but also represents one of the early steps towards establishing CMB polarization lensing as a powerful new probe of cosmology and astrophysics., Comment: 6 pages, 2 figures. v2: replaced with version accepted for publication in Physical Review Letters. The companion paper (arXiv:1312.6646) describes a measurement of the polarization lensing power spectrum
Published: 2014
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47. POLARBEAR CMB Polarization Experiment

Author: A. Ghribi, Brian Keating, Josquin Errard, M. Le Jeune, Takahiro Okamura, Matt Dobbs, W. L. Holzapfel, N. Katayama, A. Shimizu, Yuji Chinone, R. Stompor, Helmuth Spieler, Christian L. Reichardt, Gary A. Fuller, Yuki Inoue, Frederick Matsuda, Hans P. Paar, N. W. Halverson, M. J. Myers, S. Moyerman, Kaori Hattori, Nathan Stebor, Zigmund Kermish, Jun-ichi Suzuki, J. Borrill, J. Peloton, Y. Kaneko, Paul L. Richards, Peter A. R. Ade, Masaya Hasegawa, Darcy Barron, Adrian T. Lee, M. Sholl, E. Quealy, O. Zahn, Chang Feng, William F. Grainger, D. Boettger, H. Nishino, T. Matsumura, Daniel Flanigan, Marius Lungu, Nathan Miller, G. Jaehnig, Masashi Hazumi, Jonathon Howard, Amit Yadav, Colin Ross, Takayuki Tomaru, Meir Shimon, H. Morii, Carole Tucker, Kam Arnold, K. Tanaka, P. Siritanasak, Andrew H. Jaffe, N. Kimura, Eric V. Linder, P. Hyland, A. Suzuki, G. Fabbian, Bryan Steinbach, Roger O'Brient, S. Chapmann, Theodore Kisner, Y. Akiba, Chase Owen Shimmin, and A. E. Anthony
Subjects: Physics, Beam size, law, Polarization (politics), Bolometer, Cosmic microwave background, Astronomy, Astrophysics, Cosmological model, law.invention
Published: 2014
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48. Topographic mapping of the axons of the femoral chordotonal organ neurons in the cricket Gryllus bimaculatus

Author: H, Nishino
Subjects: Gryllidae, Male, Histology, Neural Pathways, Animals, Sense Organs, Female, Neurons, Afferent, Cell Biology, Axons, Pathology and Forensic Medicine
Abstract: Central projections of the femoral chordotonal organ (FCO) neurons in the cricket Gryllus bimaculatus were investigated by selectively staining small numbers of axons. The FCOs in all legs consist of partly fused ventral and dorsal scoloparia in the proximal femur. The ventral scoloparium neurons can be reliably divided into two groups: the ventral group neurons (VG), which are arranged in a sequentially smaller manner distally, and dorsal group neurons (DG), which simply aggregate in the proximal region near the dorsal scoloparium. All axons of the FCO projected to the ipsilateral half of the respective thoracic ganglion. The VG axons possessed dorso-lateral branches in the motor association neuropile and antero-ventral branches dorso-lateral to the anterior ventral association centre. However, the more proximally the somata were situated, the more medially the main neurites terminated. The DG axons showed some variations: some axons of the distally located neurons possessed dorso-lateral branches and terminated on the boundary region of the mVAC, while the other axons terminated exclusively in the medical ventral association centre (mVAC), including the ventral part, which receives auditory sensory neuron projections. All axons of the dorsal scoloparium neurons projected exclusively into the dorsal part of the mVAC; however, the ventrally located neurons projected more ventrally than did the dorsally located neurons. The above characteristics were nearly identical in the pro- and metathoracic FCOs. These results suggest that the cricket FCO axons are roughly organized in a somatotopic map and are broadly differentiated in their function.
Published: 2000
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49. A Case of Early Sigmoid Colon Cancer with Metastasis to the Group 3 Lymph Node

Author: Hideyuki Ike, Shigeki Yamaguchi, H. Nishino, Shigeo Ohki, Hiroshi Shimada, Mitsuyasu Ota, and Yasushi Ichikawa
Subjects: Oncology, medicine.medical_specialty, business.industry, Gastroenterology, medicine.disease, Metastasis, medicine.anatomical_structure, Sigmoid colon cancer, Internal medicine, medicine, Surgery, Radiology, business, Lymph node
Abstract: 大腸sm癌のリンパ節転移頻度はおよそ10%とされているがほとんどが第1群ないし2群リンパ節転移に限られる. 今回, S状結腸の大きさ20mmのIsp型病変に対してD3手術を施行したところ第3群の253番リンパ節に転移を認めたsm癌を経験した. 本例は生検で中分化腺癌と診断され, 中央に不整な陥凹を有していた.
Published: 2000
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50. Two antagonistic functions of neural groups of the femoral chordotonal organ underlie thanatosis in the cricket Gryllus bimaculatus DeGeer

Author: H. Nishino, Laurence H. Field, and Masaki Sakai
Subjects: musculoskeletal diseases, Contraction (grammar), biology, Physiology, Gryllus bimaculatus, Sensory system, Anatomy, Catalepsy, musculoskeletal system, medicine.disease, biology.organism_classification, body regions, Chordotonal organ, Behavioral Neuroscience, medicine.anatomical_structure, medicine, Reflex, Animal Science and Zoology, Tibia, Neuron, Ecology, Evolution, Behavior and Systematics
Abstract: The cricket Gryllus bimaculatus displayed freezing (thanatosis) after struggling while the femoro-tibial joints of the walking legs were forcibly restrained. Myographic recording indicated that strong contraction of the flexor tibia muscle “leg flexion response” occurred under this restrained condition. During thanatosis, when the femoro-tibial joint was passively displaced and held for several seconds, it maintained its new position (catalepsy). Only discharge of the slow flexor units was mechanically indispensable for maintaining thanatosis and catalepsy. Differing roles of identified neuron subgroups of the femoral chordotonal organ were elucidated using this behavioral substrate. Ablation of the dorsal group neurons in the ventral scoloparium strengthened the leg flexion response and the normal resistance reflex, while ablation of the ventral group weakened both motor outputs. Ablation of the dorsal scoloparium neurons, or other main sensory nerves caused no detectable deficiency in femoro-tibial joint control. These results imply that both modes of flexor muscle activation promoted by the ventral group neurons are normally held under inhibitory control by the dorsal group. It is hypothesized that this antagonistic function causes immobilization of the femoro-tibial joint in a wide range of angles in thanatosis and catalepsy.
Published: 1999
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