Author: "Doğa Veske" - Searchworks@Jio Institute Digital Library Search Results

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23 results on '"Doğa Veske"'

1. Probing the dark Solar system: detecting binary asteroids with a space-based interferometric asteroid explorer

Author: Andrew G Sullivan, Doğa Veske, Zsuzsa Márka, Imre Bartos, and Szabolcs Márka
Subjects: Earth and Planetary Astrophysics (astro-ph.EP), Space and Planetary Science, Physics::Space Physics, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics - Earth and Planetary Astrophysics
Abstract: With the inception of gravitational wave astronomy, astrophysical studies using interferometric techniques have begun to probe previously unknown parts of the universe. In this work, we investigate the potential of a new interferometric experiment to study a unique group of gravitationally interacting sources within our solar system: binary asteroids. We present the first study into binary asteroid detection via gravitational signals. We identify the interferometer sensitivity necessary for detecting a population of binary asteroids in the asteroid belt. We find that the space-based gravitational wave detector LISA will have negligible ability to detect these sources as these signals will be well below the LISA noise curve. Consequently, we propose a 4.6 AU and a 1 AU arm-length interferometers specialized for binary asteroid detection, targeting frequencies between $10^{-6}$ and $10^{-4}$ Hz. Our results demonstrate that the detection of binary asteroids with space-based gravitational wave interferometers is possible though very difficult, requiring substantially improved interferometric technology over what is presently proposed for space-based missions. If that threshold can be met, an interferometer may be used to map the asteroid belt, allowing for new studies into the evolution of our solar system., Comment: 17 pages, 18 figures, Accepted for Publication to Monthly Notices of the Royal Astronomical Society
Published: 2022
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2. Swift Follow-up Observations of Gravitational-wave and High-energy Neutrino Coincident Signals

Author: Azadeh Keivani, Jamie A. Kennea, Phil A. Evans, Aaron Tohuvavohu, Riki Rapisura, Samantha R. Oates, Stefan Countryman, Imre Bartos, Zsuzsa Márka, Doğa Veske, Szabolcs Márka, and Derek B. Fox
Published: 2021
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3. Multi-messenger Emission from Tidal Waves in Neutron Star Oceans

Author: Andrew G Sullivan, Lucas M B Alves, Georgina O Spence, Isabella P Leite, Doğa Veske, Imre Bartos, Zsuzsa Márka, and Szabolcs Márka
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Solar and Stellar Astrophysics, Astronomy and Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics
Abstract: Neutron stars in astrophysical binary systems represent exciting sources for multi-messenger astrophysics. A potential source of electromagnetic transients from compact binary systems is the neutron star ocean, the external fluid layer encasing a neutron star. We present a groundwork study into tidal waves in neutron star oceans and their consequences. Specifically, we investigate how oscillation modes in neutron star oceans can be tidally excited during compact binary inspirals and parabolic encounters. We find that neutron star oceans can sustain tidal waves with frequencies between $0.01-20$ Hz. Our results suggest that tidally resonant neutron star ocean waves may serve as a never-before studied source of precursor electromagnetic emission prior to neutron star-black hole and binary neutron star mergers. If accompanied by electromagnetic flares, tidally resonant neutron star ocean waves, whose energy budget can reach $10^{46}$ erg, may serve as early warning signs ($\gtrsim 1$ minute before merger) for compact binary mergers. Similarly, excited ocean tidal waves will coincide with neutron star parabolic encounters. Depending on the neutron star ocean model and a flare emission scenario, tidally resonant ocean flares may be detectable by Fermi and NuSTAR out to $\gtrsim 100$ Mpc with detection rates as high as $\sim 7$ yr$^{-1}$ for binary neutron stars and $\sim0.6$ yr$^{-1}$ for neutron star-black hole binaries. Observations of emission from neutron star ocean tidal waves along with gravitational waves will provide insight into the equation of state at the neutron star surface, the composition of neutron star oceans and crusts, and neutron star geophysics., 16 pages, 3 figures, 3 tables; accepted for publication in MNRAS
Published: 2022

4. Generalized approach to matched filtering using neural networks

Author: Jingkai Yan, Mariam Avagyan, Robert E. Colgan, Doğa Veske, Imre Bartos, John Wright, Zsuzsa Márka, and Szabolcs Márka
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), FOS: Computer and information sciences, Computer Science - Machine Learning, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics (astro-ph.IM), General Relativity and Quantum Cosmology, Machine Learning (cs.LG)
Abstract: Gravitational wave science is a pioneering field with rapidly evolving data analysis methodology currently assimilating and inventing deep learning techniques. The bulk of the sophisticated flagship searches of the field rely on the time-tested matched filtering principle within their core. In this paper, we make a key observation on the relationship between the emerging deep learning and the traditional techniques: matched filtering is formally equivalent to a particular neural network. This means that a neural network can be constructed analytically to exactly implement matched filtering, and can be further trained on data or boosted with additional complexity for improved performance. Moreover, we show that the proposed neural network architecture can outperform matched filtering, both with or without knowledge of a prior on the parameter distribution. When a prior is given, the proposed neural network can approach the statistically optimal performance. We also propose and investigate two different neural network architectures MNet-Shallow and MNet-Deep, both of which implement matched filtering at initialization and can be trained on data. MNet-Shallow has simpler structure, while MNet-Deep is more flexible and can deal with a wider range of distributions. Our theoretical findings are corroborated by experiments using real LIGO data and synthetic injections, where our proposed methods significantly outperform matched filtering at false positive rates above $5\times 10^{-3}\%$. The fundamental equivalence between matched filtering and neural networks allows us to define a "complexity standard candle" to characterize the relative complexity of the different approaches to gravitational wave signal searches in a common framework. Finally, our results suggest new perspectives on the role of deep learning in gravitational wave detection., 18 pages, 13 figures
Published: 2022
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5. An Archival Search for Very-High-Energy Counterparts to Sub-Threshold Neutron-Star Merger Candidates

Author: Szabolcs Marka, Z. Márka, K. Rainer Corley, Doğa Veske, Imre Bartos, and C. Adams
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma ray, FOS: Physical sciences, Astronomy, Cherenkov Telescope Array, Coincidence, LIGO, IceCube Neutrino Observatory, Neutron star, Astrophysics - High Energy Astrophysical Phenomena, Event (particle physics)
Abstract: The recent discovery of electromagnetic signals in coincidence with gravitational waves from neutron-star mergers has solidified the importance of multimessenger campaigns for studying the most energetic astrophysical events. Pioneering multimessenger observatories, such as the LIGO/Virgo gravitational wave detectors and the IceCube neutrino observatory, record many candidate signals that fall short of the detection significance threshold. These sub-threshold event candidates are promising targets for multimessenger studies, as the information provided by these candidates may, when combined with time-coincident gamma-ray observations, lead to significant detections. In this contribution, I describe our use of sub-threshold binary neutron star merger candidates identified in Advanced LIGO's first observing run (O1) to search for transient events in very-high-energy gamma rays using archival observations from the VERITAS imaging atmospheric Cherenkov telescope array. I describe the promise of this technique for future joint sub-threshold searches.
Published: 2021
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6. Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs

Author: A. Grimaldi, M. A. Barton, Samuele Cortese, Charlie Hoy, Charalampos Markakis, L. Trozzo, Albert Lazzarini, Benno Willke, A. Grado, P. Booker, C. Cahillane, Norichika Sago, J. Hennig, V. Gayathri, J. Baird, M. Jeunon, Sascha Husa, Samaya Nissanke, S. Walsh, A. Hreibi, M. J. Szczepańczyk, M. Chaturvedi, G. Venugopalan, S. R. Mohite, Alessandra Buonanno, Gabrielle Allen, H. Y. Cheung, Rana X. Adhikari, Om Sharan Salafia, F. Donovan, Edoardo Milotti, B. Lantz, M. A. Bizouard, B. K. Berger, Denis Martynov, Claudia Moreno, N. V. Krishnendu, Marco Bazzan, Satoshi Tsuchida, C. Ingram, D. A. Melchor, F. Marion, E. Goetz, Matthew Giesler, D.B. DeBra, Giuseppe Castaldi, S. G. Crowder, K. Ito, E. Lalande, M. Cannavacciuolo, E. N. Clark, Geoffrey Lovelace, L. Nguyen Quynh, J. D. E. Creighton, Lijing Shao, M. Carpinelli, J. Liu, A. Pasqualetti, R. Bajpai, F. Garufi, Archana Pai, Surendra Nadh Somala, Yoshiyuki Obuchi, C. Talbot, Carl-Johan Haster, S. Nozaki, H. Sun, V. JaberianHamedan, Tyson Littenberg, T. Washimi, T. D. Creighton, L. A. Rees, Silvia Corezzi, S. Bae, Kai-Feng Chen, F. Paoletti, Felice Sorrentino, C. L. Chan, P. Szewczyk, A. K. Prajapati, M. Patel, C. M. Mow-Lowry, Sergey P. Vyatchanin, L. Aiello, Luigi Troiano, M. Gosselin, R. Green, H. Yuzurihara, D. Hoyland, B. F. Whiting, J. Casanueva Diaz, V. M. Bedakihale, Masako Kakizaki, R. Maggiore, C. Van Den Broeck, E. Sowell, E. Coccia, M. E. Zucker, B. A. Weaver, G. Vajente, S. M. Gaebel, T. Shimoda, Y. Okutani, J. G. Rollins, A. Mhaske, H. Hansen, T. Wlodarczyk, Laura Cadonati, L. Rolland, S. T. Countryman, S. Penn, R. M. S. Schofield, K. Mogushi, H. Estelles, Y. Huang, P. A. Duverne, S. Karki, D. Moraru, A. Dmitriev, E. Floden, V. B. Adya, A. Renzini, G. L. Mansell, Y. K. Lecoeuche, G. M. Harry, L. Naticchioni, T. Shishido, Salvatore Vitale, A. Cumming, F. Di Renzo, Gianpietro Cagnoli, L.-W. Wei, S. Katsanevas, Madeline Wade, M. Tse, D. S. Tsai, D. M. Macleod, T. D. Ramirez, M. T. Hübner, Yasufumi Kojima, J. F. J. van den Brand, C. Pluchar, P. Chanial, Abhirup Ghosh, S. Sunil, M. Tacca, G. Kang, E. Capote, A. K. Mehta, N. Man, H. Pang, K. A. Strain, K. Haughian, P. Ruggi, A. Puecher, A. Mullavey, T. J. N. Nelson, Filip Morawski, P. J. Easter, G. Guixé, Xiaohui Fan, P. Leaci, Y. R. Chen, Alessandro Bertolini, J. C. Driggers, John A. Clark, Ben Farr, Fabrizio Barone, Giuseppe Intini, D. Rozza, V. Dattilo, Tejinder Kaur, Edwin J. Son, Isobel M. Romero-Shaw, T. C. Pechsiri, Umakant D. Rapol, G. S. Wallace, Stefan Hild, J. D. Jones, A. C. Baylor, L. M. DaneshgaranBajastani, R. Huxford, Surabhi Sachdev, Christopher J. Moore, V. V. Frolov, Kazuhiro Hayama, K. Venkateswara, R. Cotesta, R. Mittleman, Kentaro Komori, Soubhik Kumar Bhaumik, Yuri Levin, Akito Araya, J. Von Wrangel, T. Kajita, L. Kleybolte, S. Oshino, G. S. Davies, T. Huynh-Dinh, Hajime Sotani, A. Z. Jan, C. Makarem, Martin Hendry, Cecilio García-Quirós, Hong Wu, J.-G. Ducoin, Richard O'Shaughnessy, B. Barr, M. C. Díaz, A. Menendez-Vazquez, P. Figura, C. M. Compton, Antonios Kontos, B. L. Swinkels, Wei-Tou Ni, V. Tiwari, K. A. Thorne, Hisa-aki Shinkai, Isabel Cordero-Carrión, S. Wu, Ll. M. Mir, Junwei Cao, R. Kirchhoff, S. P. Jadhav, M. C. Heintze, Yann Bouffanais, V. Fafone, A. Pereira, J. A. Rocha, Nelson Christensen, S. A. Usman, E. G. Seo, E. K. Porter, Kendall Ackley, R. K. Nayak, A. Allocca, Marco Romanelli, Christophe Collette, C. J. Perez, B. D. O'Brien, R. P. Udall, R. C. Walet, C. Di Fronzo, T. R. Saravanan, J. Zhang, L. F. Ortega, V. P. Mitrofanov, R. Cummings, G. Koekoek, J. Betzwieser, M. Zhan, D. W. Yeeles, Antoine Heidmann, A. Brillet, G. Eddolls, A. D. Viets, D. Meacher, E. N. Tapia San Martin, K. Haris, F. Vetrano, Z. Hong, K. Kaihotsu, S. E. Dwyer, David Keitel, A. Hagiwara, L. C. Strang, R. L. Savage, Chunglee Kim, F. W. Yang, J. S. Kissel, H. Cao, Marc Favata, A. J. Weinstein, Fumihiro Uraguchi, Roger Jones, V. Villa-Ortega, David A. Williams, S. J. Cooper, N. Raza, I. W. Harry, C-Y. Lin, N. Y. Washington, N. Letendre, Nikhil Sarin, J. Heinzel, Thanh D. Nguyen, V. J. Roma, Leo Tsukada, E. Z. Hamilton, M. Matiushechkina, Nikita S. Shcheblanov, B. H. Hsieh, Y. Miyazaki, A. D. Huddart, N. Kawai, R. J. Trudeau, Anindita Ganguly, M. Diaz-Ortiz, J. Venneberg, W. Del Pozzo, P. F. Cohadon, K. E. Ramirez, H. Heitmann, D. Sawant, M. Laxen, Anchal Gupta, Kei Kotake, H. Y. Chia, E. Cuoco, N. A. Didio, E. N.Tapia San Mertin, Fabrizio Giulio Luca Pilo, F. E. Peña Arellano, A. Ueda, D. Lumaca, L. Xiao, A. P. Spencer, A. M. Farah, M. F. Carney, D. D. Brown, Chad Hanna, A. Bramley, Yue Zhao, C. Kimball, Sakae Araki, J. J. McCann, T. J. Slaven-Blair, S. ShyamSundar, C. Stachie, A. Parisi, J. Oberling, M. Pirello, Alena Ananyeva, A. Lartaux-Vollard, Suvadeep Bose, A. Depasse, A. F. Helmling-Cornell, Ajay Kumar, N. D. Ormsby, C. Whittle, Yuki Inoue, A. M. Gretarsson, C. Bradaschia, W-R. Xu, F. Carbognani, Yang Yang, Yoshiaki Himemoto, I. M. Pinto, I. La Rosa, Jean-René Cudell, C. De Rossi, Stanislav Babak, S. Sayah, H. Overmier, B. Garaventa, Nobutada Kimura, Ka Yee C. Lee, M. A. Okada, Matteo Pegoraro, Piero Rettegno, R. Gouaty, A. V. Bhandari, Z. Márka, M. Boer, Shubhanshu Tiwari, T. B. Edo, R. Gray, Masashi Ohkawa, V. Srivastava, Y. Aso, M. Fays, N. van Bakel, M. Leonardi, Osamu Miyakawa, Lior Cohen, R. Zhang, Ik Siong Heng, Geert Raaijmakers, P. Fulda, M. Mondin, K. Mason, S. Shibagaki, D. Rosińska, E. R. G. von Reis, Ray-Kuang Lee, F. Y. Khalili, Ofelia Durante, Jay D. Tasson, J. L. Willis, M. Eisenmann, Ofek Birnholtz, Sanjeev Dhurandhar, M. Merzougui, Sebastien Biscans, S. A. Nichols, A. Malik, S. Gaudio, G. Valdes, Pulak Ranjan Giri, A. Adams, I. Tosta e Melo, Deirdre Shoemaker, F. Robinet, J. K. Blackburn, Q. Chu, F. L. Linde, R. Tenorio, N. A. Holland, Yichen Huang, D. Sellers, G. R. Johns, S. Ponrathnam, Michael Williams, Moritz Mehmet, L. Terkowski, E. Cesarini, P. Kumar, A. Singha, Ken K. Y. Ng, M. Constancio, E. Chassande-Mottin, S. Galaudage, C. Darsow-Fromm, C. Di Giorgio, J. D. Callaghan, Torrey Cullen, G. Ge, A. Di Lieto, J. Sadiq, Angela Trapananti, Kopin Liu, M. Vasúth, W. Griffiths, Eric Howell, Sadakazu Haino, J. D. Merritt, A. Masserot, Sylvain Marsat, Yuichiro Sekiguchi, M. Nakano, Sheila Rowan, M. Ebersold, S. Márka, N. Sennett, C. Wu, K. Kawabe, Jimin George, M. Sieniawska, F. Kuei, Brynmor Haskell, Alberto Vecchio, Geoffrey Mo, Will M. Farr, M. Montani, F. K. Lin, Nancy Aggarwal, J. B. Carlin, Simone Mozzon, Patrice Hello, G. Pagliaroli, M. Was, Xin Chen, R. M. Martin, J. C. Barayoga, B. F. Neil, R. Robie, L. W. Luo, I. Molina, M. Landry, A. Tripathee, L. Di Fiore, B. Mours, F. Meylahn, C. Austin, N. W. Farrow, M. Barsuglia, A. L. Miller, Leo Singer, Bartosz Fornal, Shinji Miyoki, Matteo Breschi, W. Kastaun, H. Qi, K. Chandra, H. Vocca, S. Leavey, S. Eguchi, Hai-Ping Cheng, A. Iess, D. Ugolini, P. Jung, M. Bawaj, Lili Yang, J. Smetana, A. C. Utina, Riccardo Sturani, V. Bossilkov, A. Ramos-Buades, M. Bischi, Kiran Prasai, G. Ueshima, Kyujin Kwak, S. Nagano, V. Kringel, J. Bidler, R. Dean, A. B. Yelikar, D. Gao, E. Katsavounidis, K. Shimode, D. C. Y. Hui, F. Nocera, A. Grant, C. Zhao, D. Bankar, I. Dorrington, Xiuling Li, M. Branchesi, Xing-Jiang Zhu, Takuma Yamada, G. Vedovato, L. E. H. Datrier, Y. Sakai, I. Di Palma, J. Gais, L. K. Nuttall, R. Macas, G. Billingsley, D. Jariwala, K. Jung, R. Jaume, R. A. Eisenstein, Hee-Suk Cho, M. H. P. M. van Putten, Jishnu Suresh, L. Prudenzi, T. Zelenova, Riccardo Bassiri, D. B. Kozak, C. Vorvick, Ryan Magee, Nandita Khetan, R. Tso, M. Kovalam, Alec Mishkin, R. Cavalieri, Magnus Manske, A. K. Srivastava, A. E. Pace, K. Miyo, A. S. Hines, Roberto Chierici, P. Clearwater, S. Sudhagar, M. Pürrer, S. Kwang, I. Dave, S. Sato, D. Agarwal, Thierry Pradier, David Jones, A. Shoda, Marco Cavaglia, B. Hughey, N. Hirata, M. Curyło, Subroto Mukherjee, P. Astone, V. Kondrashov, Bruno Giacomazzo, L. Errico, D. B. Tanner, Kevin M. Ryan, Patrick M. Koch, Carmen S. Menoni, M. Korobko, T. Zhang, S. M. Aston, Michael W. Coughlin, Zhoujian Cao, I. Khan, S. Banagiri, T. Kawasaki, H. Radkins, J. Brooks, R. Musenich, M. Kamiizumi, J. Lange, Tania Regimbau, A. J. Tanasijczuk, A. M. Knee, K. Merfeld, Y. Tomigami, A. Viceré, Frances Hellman, K. Chakravarti, Arunava Mukherjee, Haruki Kitazawa, Fabio Marchesoni, J. Park, A. Chiummo, Kyungmin Kim, Debarati Chatterjee, B. O'Reilly, P. Gruning, Mario Spera, Peter Aufmuth, T. L. Lam, K. W. Tsang, E. J. Fauchon-Jones, Atsushi Nishizawa, Gianluca Grignani, D. Y. T. Pong, A. Gennai, A. Ain, E. Massera, Y. Asali, Y. Bae, D. Schaetzl, Thibaut Jacqmin, C. Olivetto, A. Yoon, M. Lormand, L. Zhang, D. Töyrä, O. Sauter, S. B. Anderson, K. M. Aleman, Graham Woan, Robert L. Byer, Stuart Reid, Riccardo Ciolfi, Yi Chen, Harald P. Pfeiffer, Peter T. H. Pang, Tomasz Bulik, T. Tomura, Francesco Chiadini, F. J. Hayes, A. Basti, C. I. Torrie, Alessandro Longo, Jürgen Heinze, K. Oohara, E. Maros, J. Glanzer, Manel Molina-Ruiz, Edward Seidel, Richard J. Oram, A. Bozzi, S. B. Coughlin, W. G. Anderson, G. Cella, Ryan N. Lang, D. D'Urso, Krzysztof Piotrzkowski, B. W. Schulte, Vuk Mandic, D. J. Stops, S. Ide, Y. Minenkov, M. Turconi, J. Junker, H. M. Lee, Jessica Steinlechner, M. Pracchia, A. Neunzert, Norikatsu Mio, D. Sentenac, M. Heurs, J. S. H. Lee, P. Couvares, Patrick Brady, T. Dal Canton, Felix Wellmann, J. Warner, Podila Satya Venkata Narasimha Sharma, E. K. Gustafson, M. Rizzo, G. Cho, Pablo Cerdá-Durán, Vivien Raymond, A. A. Ciobanu, David E. McClelland, J. C. Bayley, J.-P. Coulon, François Bondu, H. Chu, M. Kolstein, P. J. Veitch, M. Ball, M. L. Lollie, P. J. Sutton, M. Deenadayalan, Sung-Po Chao, R. De Simone, S. Ghosh, D. Passuello, F. Badaracco, E. A. Chase, Z. Frei, Jacob Scheuer, Astrid Lamberts, J. Woehler, S. V. Angelova, Kyohei Kawaguchi, I. Michaloliakos, R. Passaquieti, G. Pagano, Reed Essick, C. Nguyen, N. Kita, J. N. Hohmann, C. Jeon, A. Cirone, R. Coyne, Fabrice Matichard, R. De Rosa, Kazuyuki Tanaka, Bernard F. Schutz, Kwan-Lok Li, M. Ying, M. Saleem, Veronica Granata, Yi-Ting Hsu, M. Haney, A. Balsamo, S. Khadka, Marta Colleoni, Yuta Michimura, P. Thomas, M. Arène, J. A. Giaime, I. Nardecchia, A. Amato, L. E. Wade, B. U. Gadre, A. C. Green, J. Z. Wang, Y-K. Chu, K. Yokogawa, D. Corre, Y. M. Kim, R. G. Ormiston, Hyun Lee, J. Calderón Bustillo, Safura Sharifi, J. H. Romie, B. Edelman, G. Mendell, C. Rajan, S. Kandhasamy, M. Fishbach, R. Abbott, Samuel Deléglise, S. J. Jadhav, A. R. Williamson, A. Miyamoto, Felipe Guzman, I. Belahcene, Albert K. H. Kong, B. Sorazu, E. O'Shea, Y. Nakayama, Piotr Jaranowski, Kazuhiro Yamamoto, Geraint Pratten, H. Fair, H. W. Lee, Robert J. McCarthy, S. Takano, Linqing Wen, T. A. Callister, G. Kuehn, T. Sekiguchi, László Á. Gergely, A. Macquet, M. Boldrini, Philip F. Hopkins, Y. Kao, Fausto Acernese, K. Kuns, C-Y. Chiang, Laurent Pinard, Shaon Ghosh, F. J. Raab, N. Mukund, V. Savant, Valérie Martinez, M. Cieślar, Terry G. McRae, Takahiro Tanaka, J. B. Kanner, Li Ju, Yoshio Arai, Brittany Kamai, Andreu Sanuy, Y. Hiranuma, A. Fernandez-Galiana, Hideki Asada, C. V. Kalaghatgi, J. Hanson, H. Fong, G. Greco, Zong-Hong Zhu, Francesco Pannarale, A. L. Stuver, David Coward, A. Miani, Jan Harms, A. S. Sengupta, D. Bhattacharjee, Daniele A. Steer, H. Satari, D. Bersanetti, G. Ashton, B. Ikenoue, T. Yamamoto, E. Fenyvesi, C. Messenger, Fabrizio Bobba, Stephan Grimm, F. Hernandez Vivanco, C. H. Chan, E. Payne, Takashi Uchiyama, C. Gray, I. Fiori, A. K. Zadrożny, S. Ha, Kohei Yamamoto, T. J. Shaffer, Tomotada Akutsu, Shawn Rosofsky, H-S. Kuo, C. Osthelder, Daichi Tsuna, Anupreeta More, Y. Kuromiya, P. Relton, Michela Mapelli, Z. Chen, T. Mishra, R. Gustafson, G. A. Prodi, Andrea Chincarini, Minkyun Noh, Cesare Barbieri, Walter Winkler, A. S. Markosyan, R. DeSalvo, T. Z. Summerscales, A. Lemaître, J. N. Linley, F. Cipriano, Soichiro Morisaki, M. Bals, N. Radulesco, Kunihito Ioka, L. G. Prokhorov, Harald Lück, E. Knyazev, D. Verkindt, A. Rocchi, B. Goncharov, R. Birney, Zachariah B. Etienne, D. Lopez, Y. Drori, Jennifer Watchi, V. Boschi, M. van Beuzekom, H. L. Lin, A. L. James, Jade Powell, V. Mangano, C. Pankow, P. Dupej, M. Mantovani, Eric B. Flynn, J. Kume, Jianfang Wang, B. Gateley, A. Sur, T. Di Girolamo, Aaron Buikema, Hang Yu, N. Leroy, Kentaro Somiya, Iii H.W. Cain, D. Tsai, Christos Karathanasis, Eric Thrane, P. Barneo, W. Katzman, A. F. Vargas, T. Sadecki, Sheon Chua, R. Bonnand, Mariana Fazio, S. C. McGuire, J. F. Read, S. Di Pace, S. Otabe, Toshikazu Suzuki, Aldo Ejlli, M. Piendibene, M. K. M. Bader, D. L. Ferguson, Y. Sakuno, Miriam Lucio Martinez, Michael Thomas, S. Biscoveanu, W. Ogaki, E. Polini, B. Bécsy, Matthias H. Hennig, N. Van Remortel, Des Gibson, H. K. Gulati, Hiroyuki Nakano, Eric Grimes, P. M. Meyers, A. Branch, K. Sakai, J. V. van Heijningen, C. C. Wipf, M. Fyffe, S. Koley, M. Brinkmann, P. Prosposito, S. Grunewald, R. Prasanna, P. Popolizio, Koji Arai, Gabriela Gonzalez, K. R. Corley, S. Choudhary, J. N. Leviton, D. Pascucci, T. Uehara, R. Gamba, M. J. Cowart, M. Nery, S. Raja, S. Maliakal, Yuka Fujii, O. V. Palashov, Sean T. McWilliams, F. Piergiovanni, D. E. Cohen, C. Michel, Maria Luisa Chiofalo, A. E. Gleckl, Rajesh Kumar, Kuo-Chuan Pan, I. Maksimovic, A. Effler, A. Franke, Vivishek Sudhir, C. C. Kuo, R. L. Ward, G. Hemming, Valeria Sipala, David H. Reitze, H. Masalehdan, D. Buskulic, Rahul Kashyap, C. McIsaac, N. De Lillo, N. Sorrentino, W. Jia, H. Zhang, I. J. Hollows, D. H. Shoemaker, James Healy, Y. Moriwaki, Masaki Ando, H. Vahlbruch, Gunnar Riemenschneider, J. C. Mills, K. Riles, K. Kusayanagi, J. Y. Vinet, H. Middleton, C. Affeldt, Ettore Majorana, R. P. Fisher, S. Mitra, M. Zevin, M. Fukunaga, S. Frasca, Jonathan Richardson, Sarah Caudill, M. P. Thirugnanasambandam, E. J. Sanchez, D. Tuyenbayev, Maria Ilaria Del Principe, Yogesh Verma, Kai Staats, S. Mastrogiovanni, L. 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D., Abraham, S., Acernese, F., Ackley, K., Adams, A., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., Agarwal, D., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Akutsu, T., Aleman, K. M., Allen, G., Allocca, A., Altin, P. A., Amato, A., Anand, S., Ananyeva, A., Anderson, S. B., Anderson, W. G., Ando, M., Angelova, S. V., Ansoldi, S., Antelis, J. M., Antier, S., Appert, S., Arai, Koya, Arai, Koji, Arai, Y., Araki, S., Araya, A., Araya, M. C., Areeda, J. S., Arène, M., Aritomi, N., Arnaud, N., Aronson, S. M., Asada, H., Asali, Y., Ashton, G., Aso, Y., Aston, S. M., Astone, P., Aubin, F., Aufmuth, P., Aultoneal, K., Austin, C., Babak, S., Badaracco, F., Bader, M. K. M., Bae, S., Bae, Y., Baer, A. M., Bagnasco, S., Bai, Y., Baiotti, L., Baird, J., Bajpai, R., Ball, M., Ballardin, G., Ballmer, S. W., Bals, M., Balsamo, A., Baltus, G., Banagiri, S., Bankar, D., Bankar, R. S., Barayoga, J. C., Barbieri, C., Barish, B. C., Barker, D., Barneo, P., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Barton, M. A., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Baylor, A. C., Bazzan, M., Bécsy, B., Bedakihale, V. M., Bejger, M., Belahcene, I., Benedetto, V., Beniwal, D., Benjamin, M. G., Bennett, T. F., Bentley, J. D., Benyaala, M., Bergamin, F., Berger, B. K., Bernuzzi, S., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bhandari, A. V., Bhattacharjee, D., Bhaumik, S., Bidler, J., Bilenko, I. A., Billingsley, G., Birney, R., Birnholtz, O., Biscans, S., Bischi, M., Biscoveanu, S., Bisht, A., Biswas, B., Bitossi, M., Bizouard, M. -A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bobba, F., Bode, N., Boer, M., Bogaert, G., Boldrini, M., Bondu, F., Bonilla, E., Bonnand, R., Booker, P., Boom, B. A., Bork, R., Boschi, V., Bose, N., Bose, S., Bossilkov, V., Boudart, V., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branch, A., Branchesi, M., Brau, J. E., Breschi, M., Briant, T., Briggs, J. H., Brillet, A., Brinkmann, M., Brockill, P., Brooks, A. F., Brooks, J., Brown, D. D., Brunett, S., Bruno, G., Bruntz, R., Bryant, J., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buscicchio, R., Buskulic, D., Byer, R. L., Cadonati, L., Caesar, M., Cagnoli, G., Cahillane, C., Cain, H. W., Bustillo, J. Calderón, Callaghan, J. D., Callister, T. A., Calloni, E., Camp, J. B., Canepa, M., Cannavacciuolo, M., Cannon, K. C., Cao, H., Cao, J., Cao, Z., Capocasa, E., Capote, E., Carapella, G., Carbognani, F., Carlin, J. B., Carney, M. F., Carpinelli, M., Carullo, G., Carver, T. L., Diaz, J. Casanueva, Casentini, C., Castaldi, G., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cerdá-Durán, P., Cesarini, E., Chaibi, W., Chakravarti, K., Champion, B., Chan, C. -H., Chan, C., Chan, C. L., Chan, M., Chandra, K., Chanial, P., Chao, S., Charlton, P., Chase, E. 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W., Wette, K., Whelan, J. T., White, D. D., Whiting, B. F., Whittle, C., Wilken, D., Williams, D., Williams, M. J., Williamson, A. R., Willis, J. L., Willke, B., Wilson, D. J., Winkler, W., Wipf, C. C., Wlodarczyk, T., Woan, G., Woehler, J., Wofford, J. K., Wong, I. C. F., Wu, C., Wu, D. S., Wu, H., Wu, S., Wysocki, D. M., Xiao, L., Xu, W-R., Yamada, T., Yamamoto, H., Yamamoto, Kazuhiro, Yamamoto, Kohei, Yamamoto, T., Yamashita, K., Yamazaki, R., Yang, F. W., Yang, L., Yang, Yang, Yang, Yi, Yang, Z., Yap, M. J., Yeeles, D. W., Yelikar, A. B., Ying, M., Yokogawa, K., Yokoyama, J., Yokozawa, T., Yoon, A., Yoshioka, T., Yu, Hang, Yu, Haocun, Yuzurihara, H., Zadrożny, A., Zanolin, M., Zeidler, S., Zelenova, T., Zendri, J. -P., Zevin, M., Zhan, M., Zhang, H., Zhang, J., Zhang, L., Zhang, R., Zhang, T., Zhao, C., Zhao, G., Zhao, Yue, Zhao, Yuhang, Zhou, Z., Zhu, X. J., Zhu, Z. -H., Zimmerman, A. B., Zucker, M. 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Subjects: gravitational radiation: anisotropy, Physics and Astronomy (miscellaneous), gravitational radiation: stochastic, Astronomy, Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, Physics, Particles & Fields, Cosmology & Astrophysics, energy: flux, energy: density, gravitational radiation: energy, LIGO, QC, QB, Physics, Settore FIS/01, Spectral index, Galactic Center, Amplitude, General relativity, Sidereal time, Physical Sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], gravitational radiation: power spectrum, Gravitation, data analysis method, Anisotropic stochastic gravitational-wave background, Experimental studies of gravity, FOS: Physical sciences, O3, O2, General Relativity and Quantum Cosmology (gr-qc), Astronomy & Astrophysics, Stochastic Background, Gravitational Waves, LIGO, Virgo, O1, O2, O3, O1, Gravitational waves, UPPER LIMITS, statistical analysis, 0103 physical sciences, advanced LIGO and Virgo, ddc:530, KAGRA, 010306 general physics, STFC, gravitational waves, Virgo, Gravitational Waves, Science & Technology, 010308 nuclear & particles physics, Gravitational wave, gravitational radiation: background, RCUK, Galaxy, VIRGO, gravitational radiation: emission, spectrum: density, RADIATION, CROSS-CORRELATION SEARCH, Stochastic Background, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, galaxy
Abstract: We report results from searches for anisotropic stochastic gravitational-wave backgrounds using data from the first three observing runs of the Advanced LIGO and Advanced Virgo detectors. For the first time, we include Virgo data in our analysis and run our search with a new efficient pipeline called {\tt PyStoch} on data folded over one sidereal day. We use gravitational-wave radiometry (broadband and narrow band) to produce sky maps of stochastic gravitational-wave backgrounds and to search for gravitational waves from point sources. A spherical harmonic decomposition method is employed to look for gravitational-wave emission from spatially-extended sources. Neither technique found evidence of gravitational-wave signals. Hence we derive 95\% confidence-level upper limit sky maps on the gravitational-wave energy flux from broadband point sources, ranging from $F_{\alpha, \Theta} < {\rm (0.013 - 7.6)} \times 10^{-8} {\rm erg \, cm^{-2} \, s^{-1} \, Hz^{-1}},$ and on the (normalized) gravitational-wave energy density spectrum from extended sources, ranging from $\Omega_{\alpha, \Theta} < {\rm (0.57 - 9.3)} \times 10^{-9} \, {\rm sr^{-1}}$, depending on direction ($\Theta$) and spectral index ($\alpha$). These limits improve upon previous limits by factors of $2.9 - 3.5$. We also set 95\% confidence level upper limits on the frequency-dependent strain amplitudes of quasimonochromatic gravitational waves coming from three interesting targets, Scorpius X-1, SN 1987A and the Galactic Center, with best upper limits range from $h_0 < {\rm (1.7-2.1)} \times 10^{-25},$ a factor of $\geq 2.0$ improvement compared to previous stochastic radiometer searches., Comment: 23 Pages, 9 Figures
Published: 2021
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7. All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

Author: L. Kleybolte, Valérie Martinez, E. G. Seo, Susan M. Scott, E. K. Porter, Cesare Barbieri, Walter Winkler, Kopin Liu, Chad Hanna, A. Bramley, A. S. Markosyan, C. Kimball, Harald Lück, J. Oberling, M. Pirello, D. Passuello, A. Cirone, T. B. Edo, E. Knyazev, D. Verkindt, D. Ugolini, Roberto Chierici, P. Clearwater, Fiodor Sorrentino, C. Di Giorgio, J. Cao, S. C. McGuire, J. F. Read, S. Di Pace, H. Satari, J. Bidler, R. Dean, J. Calderón Bustillo, Miriam Lucio Martinez, F. Nocera, N. Letendre, Safura Sharifi, Alicia M. Sintes, M. Curyło, Nikhil Sarin, J. V. van Heijningen, E. J. Fauchon-Jones, A. Yoon, M. Lormand, J. Heinzel, Thanh D. Nguyen, E. Cuoco, D. Lumaca, M. A. Okada, K. Mason, D. J. Stops, Sanjeev Dhurandhar, J. S. H. Lee, T. Dal Canton, Felix Wellmann, J. Warner, I. Maksimovic, R. L. Ward, G. Hemming, R. Passaquieti, Laurent Pinard, F. Cleva, C. Messenger, M. P. Ross, M. Pichot, Maximiliano Isi, M. Croquette, E. M. Gretarsson, Ying Guo, D. Beniwal, Peter Fritschel, Wenxiao Wang, V. Valsan, M. Masso-Reid, Z. J. Holmes, J. Petermann, Xin Chen, R. M. Martin, Piotr Jaranowski, L. E. Sanchez, A. C. Utina, D. Hartwig, C. Rajan, Enrico Calloni, G. Traylor, S. Soni, Thomas Corbitt, L. Salconi, C. A. Costa, R. K. Choudhary, V. Boudart, W. Jia, T. Zhang, Thibaut Jacqmin, D. Lopez, Y. Drori, S. Choate, N. Leroy, S. T. Countryman, Albert Lazzarini, Geraint Pratten, H. Fair, Surabhi Sachdev, Christopher J. Moore, Q. Chu, D. Bersanetti, G. Ashton, Samuele Cortese, G. A. Prodi, Christos Karathanasis, Eric Thrane, P. Thomas, M. Arène, E. Polini, B. Bécsy, I. Molina, Des Gibson, C. Michel, R. DeSalvo, A. Viceré, V. V. Frolov, Sarah Caudill, A. Vajpeyi, T. D. Knowles, Marica Valentini, Riccardo Ciolfi, Yi Chen, Peter T. H. Pang, B. W. Schulte, Samaya Nissanke, H. Y. Cheung, M. A. Bizouard, C. H. Chan, A. W. Jones, Kentaro Komori, Soubhik Kumar Bhaumik, O. V. Palashov, Sean T. McWilliams, Charlie Hoy, P. Booker, W. Kastaun, H. Qi, B. K. 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Huerta, H. L. Sawant, S. Frasca, Jonathan Richardson, François Bondu, R. De Simone, F. Badaracco, Giuseppe Castaldi, S. G. Crowder, M. P. Thirugnanasambandam, A. Balsamo, S. Khadka, P. A. Altin, Bartosz Fornal, Yang Yang, D. Rosińska, M. Stover, P.H. Nguyen, D. Barker, D. Singh, A. Samajdar, B. Sassolas, Roman Schnabel, H. L. Griggs, J. E. Brau, Terry G. McRae, R. Kirchhoff, Ryan Magee, D. Rozza, J. B. Carlin, M. Was, R. Flaminio, V. Dattilo, S. P. Jadhav, R. Robie, Tejinder Kaur, P. Popolizio, Koji Arai, E. J. Sanchez, Patrice Hello, V. Fafone, Jonathan E. Thompson, Xing-Jiang Zhu, G. Pagliaroli, A. B. Yelikar, E. Katsavounidis, R. Goetz, Stefano Ansoldi, Y. Kao, Daniele A. Steer, Kendall Ackley, R. K. Nayak, Efim A. Khazanov, Imre Bartos, Isobel M. Romero-Shaw, Tarun Souradeep, Prafulla K. Panda, G. Ballardin, Wolfango Plastino, M. Kasprzack, C. Talbot, Gregory M. Harry, C. I. Torrie, Jan Harms, A. S. Sengupta, R. Jaume, T. Wlodarczyk, Nandita Khetan, L. G. Prokhorov, D. C. 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JaberianHamedan, Chandra Kant Mishra, R. Bhandare, T. Hardwick, F. Travasso, S. Appert, J. Südbeck, Hartmut Grote, Michał Bejger, C. Affeldt, Y. Setyawati, Jordan Camp, D. Tao, E. J. Marx, Jessica Steinlechner, A. Neunzert, M. Heurs, C. Vorvick, G. Losurdo, H. W. Cain, D. Agarwal, A. C. Baylor, G. G. Fronzé, C. Bradaschia, R. Zhang, Bruno Giacomazzo, Tyson Littenberg, T. D. Creighton, A. K. Y. Li, J. Jiang, P. Shawhan, I. Ferrante, S. Barnum, Patrick Godwin, Rico K. L. Lo, D. Ganapathy, D. D. White, P. Charlton, V. Hui, Giovanni Carapella, A. Perreca, G. Gemme, M. Drago, Richard O'Shaughnessy, B. Barr, Ik Siong Heng, I. Tosta e Melo, Gregorio Carullo, Anuradha Gupta, Reed Essick, S. Kandhasamy, M. Fishbach, B. Sorazu, E. O'Shea, G. Eddolls, A. D. Viets, D. Meacher, Olivier Minazzoli, M. Razzano, C. L. Chan, A. K. Prajapati, M. C. Araya, S. Rodriguez, Guenakh Mitselmakher, E. N. Tapia San Martin, K. Haris, B. A. Boom, A. M. Sergeev, Paul Hill, Binlei Ding, Neil J. 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Saleem, A. D. Huddart, S. Márka, Sascha Husa, Stefano Bagnasco, Lucy E Clarke, N. Sennett, E. R. G. von Reis, Mairi Sakellariadou, J. Sadiq, M. Vasúth, T. F. Bennett, Gijs Nelemans, G. Venugopalan, S. R. Mohite, E. D. Hall, D.B. DeBra, G. Pillant, S. Meshkov, Seog Oh, V. Bossilkov, A. Ramos-Buades, Kenneth A. Strain, Jimin George, M. Sieniawska, A. Cumming, Brynmor Haskell, K. Chakravarti, Jolien D. E. Creighton, H. Estelles, Fabio Marchesoni, W. G. Anderson, G. Cella, Podila Satya Venkata Narasimha Sharma, D. B. Tanner, Paul M. Ricker, B. Biswas, Stefan Grimm, P. Chanial, A. C. Green, Kevin M. Ryan, Carmen S. Menoni, Tenglin Li, Kyungmin Kim, Debarati Chatterjee, B. O'Reilly, P. Gruning, E. Capote, T. Harder, K. S. Phukon, E. K. Gustafson, S. V. Angelova, M. Korobko, K. Holt, T. L. Carver, A. Zadroźny, J. Brooks, L. Haegel, Mario Spera, William Parker, Tatiana da Silva Pereira, Shreya Anand, F. Gissi, F. Salemi, M. Bitossi, Viola Sordini, J. C. Barayoga, B. F. Neil, G. S. Davies, K. A. Thorne, Isabel Cordero-Carrión, Richard J. Abbott, Rakesh Kumar, Ll. M. Mir, Francesco Chiadini, J. Junker, Fausto Acernese, K. Kuns, J. A. Rocha, D. Mukherjee, O. Durante, K. Wette, John J. Oh, Timothy Evans, F. Di Renzo, M. G. Benjamin, B. Cousins, M. Cieślar, B. Champion, P. Kolitsidou, T. R. Saravanan, J. Zhang, M. Mondin, C. Nguyen, G. Cho, B. Ratto, Nergis Mavalvala, Jerome Degallaix, M. Schneewind, C. Casentini, V. Del Favero, Rory Smith, C. Adams, R. M. Blair, D. Sigg, S. W. Ballmer, Gor Oganesyan, A. Singha, C. Frederick, A. F. Brooks, P. J. Quinonez, R. Coyne, T. J. Shaffer, Fabrice Matichard, M. Ying, M. Mantovani, L. F. Ortega, Sebastian Khan, B. C. Barish, F. De Matteis, Michelle E. Walker, Matteo Breschi, Alec Mishkin, R. Cavalieri, J. Eichholz, G. Moreno, H. Inchauspe, A. K. Srivastava, A. E. Pace, A. Sur, A. Basti, Ryan N. Lang, Krzysztof Piotrzkowski, J.-P. Coulon, S. Koley, M. Brinkmann, R. Cummings, J. N. Leviton, D. Pascucci, D. W. Yeeles, E. A. Chase, Z. Frei, N. Sorrentino, Lindsay DeMarchi, D. I. Jones, Philip F. Hopkins, Shaon Ghosh, F. Hernandez Vivanco, I. Fiori, Shawn Rosofsky, D. Petterson, T. Di Girolamo, Fabrizio Giulio Luca Pilo, A. Schindler-Tyka, M. BenYaala, A. L. Stuver, A. M. Gretarsson, F. Muciaccia, C. De Rossi, Anupam Sharma, Tim Dietrich, Lionel London, B. Idzkowski, V. Loriette, V. Skliris, E. Payne, Matthew Evans, J. K. Blackburn, F. L. Linde, E. Chassande-Mottin, S. Galaudage, Sylvain Marsat, X. Liu, D. Estevez, C. Magazzù, T. Sadecki, Sheila Rowan, M. Ebersold, S. D'Antonio, Edoardo Milotti, B. Lantz, M. Pürrer, S. Kwang, M. Piendibene, S. Grunewald, R. Prasanna, S. Klimenko, C. Gray, A. Franke, Zhihui Du, G. Ciani, E. Lalande, M. Cannavacciuolo, S. S. Eikenberry, James Healy, M. Carpinelli, Rosa Poggiani, B. Li, S. Farinon, A. Pele, P. Brockill, P. Raffai, G. I. McGhee, Vincenzo Fiumara, R. M. S. Schofield, P. A. Duverne, Andrew Matas, J. Hanks, A. Chen, Nicholas Demos, J. D. Lough, Soma Mukherjee, J. F. J. van den Brand, S. Sunil, M. Tacca, P. G. Murray, Matthew Giesler, D. Moraru, Martin Hendry, Cecilio García-Quirós, M. C. Díaz, A. Menendez-Vazquez, N. Gohlke, Fabien Kéfélian, E. Floden, J. H. Hough, P. W. F. Forsyth, S. R. Thondapu, Gianpietro Cagnoli, J. R. Palamos, G. Baltus, P. Figura, C. M. Compton, Michele Zanolin, I. Magaña Hernandez, Antonios Kontos, Giuseppe Intini, T. J. Massinger, T. Vo, G. D. Hammond, A. Allocca, Javed Rana, P. Weßels, H. Yamamoto, F. Vetrano, Graham Woan, Robert L. Byer, Stuart Reid, F. J. Hayes, K. Soni, J. C. Driggers, A. M. Baer, A. Schönbeck, V. D'Emilio, Daniel Wysocki, I. A. O. MacMillan, Steven D. Penn, Jacob Scheuer, S. E. Dwyer, David Keitel, I. Michaloliakos, J. Betzwieser, Antoine Heidmann, N. Raza, Jonathan R. Gair, G. Pagano, Bernard F. Schutz, Li Ju, Brittany Kamai, A. Lartaux-Vollard, H. Overmier, Suvadeep Bose, B. Garaventa, R. Tenorio, N. A. Holland, D. Sellers, Carlos O. Lousto, C. V. Kalaghatgi, J. Hanson, R. Gouaty, A. V. Bhandari, Z. Márka, Jianfang Wang, Hang Yu, Riccardo Sturani, M. Merzougui, F. Kuei, L. Giacoppo, C. North, Thomas Dent, P. Corban, S. J. Cooper, Alberto Vecchio, Geoffrey Mo, James Whelan, P. Ajith, D. Schaetzl, J. M. Fishner, Will M. Farr, M. Montani, D. Sentenac, Patrick Brady, O. J. Piccinni, HyunGyu Suh, D. Davis, Nancy Aggarwal, A. Effler, E. Bonilla, K. Isleif, Kazuhiro Agatsuma, Frank Ohme, Vicky Kalogera, E. Leon, O. Halim, M. Tonelli, L. Xiao, P. Fulda, J. Smetana, D. Jariwala, I. Dave, Guoying Zhao, S. L. Nadji, R. Quitzow-James, N. N. Janthalur, B. Hughey, J. L. Willis, M. Eisenmann, Ofek Birnholtz, Monica Colpi, W. Griffiths, Eric Howell, Andrew Lundgren, W. S. Kim, M. Pracchia, S. Leavey, Hai-Ping Cheng, A. Iess, L. K. Nuttall, Veronica Granata, Yi-Ting Hsu, M. Haney, T. A. Callister, R. Macas, G. Billingsley, J. N. Hohmann, A. L. James, Jade Powell, V. Mangano, I. Belahcene, H. K. Gulati, Valeria Sipala, David H. Reitze, Rahul Kashyap, C. McIsaac, N. De Lillo, Francesco Pannarale, Soichiro Morisaki, M. Bals, A. Rocchi, Alejandro Torres-Forné, B. Goncharov, R. Birney, Aldo Ejlli, Maria Ilaria Del Principe, M. Agathos, Soumen Roy, J. Neilson, Stephane Perries, S. H. Huttner, Andrew Melatos, M. Lorenzini, J. H. Briggs, Mark Hannam, A. Strunk, N. Kijbunchoo, Sheelu Abraham, J. D. Bentley, V. Sequino, C. J. Richardson, H. J. Bulten, D. Griffith, C. M. Weller, Bala R. Iyer, S. McCormick, Haocun Yu, R. S. Bankar, M. C. Milovich-Goff, A. Mhaske, A. K. Mehta, P. J. Easter, Alessandra Corsi, D. Laghi, T. Huynh-Dinh, A. Z. Jan, Chunglee Kim, J. S. Kissel, H. Cao, Marc Favata, Roger Jones, V. J. Roma, Nikita S. Shcheblanov, A. P. Spencer, D. D. Brown, A. Depasse, N. van Bakel, J. D. Merritt, A. Masserot, K. Kawabe, E. J. Daw, Maurizio Canepa, Antonio Marquina, Eric Hennes, A. S. Ubhi, T. A. Ferreira, K. D. Giardina, S. M. Aston, K. Ueno, Michael W. Coughlin, I. Khan, L. E. Wade, J. K. Wofford, M. A. Page, Samuel Deléglise, A. Fernandez-Galiana, C. Pankow, Eric Grimes, P. M. Meyers, A. Branch, H. Masalehdan, M. Zevin, John Veitch, J. Lehmann, N. Arnaud, Vijay Varma, M. MacInnis, Rémi Soulard, P. Rapagnani, T. Mistry, Andreas Freise, Vincenzo Pierro, Paul D. Lasky, R. K. Hasskew, J. W. Westhouse, B. E. Ewing, Z. Mark, Matthew Pitkin, N. Bose, M. Granata, M. C. Tringali, Peter Graham Jones, T. Prestegard, R. Musenich, V. Spagnuolo, J. Scott, J. Lange, Sebastiano Bernuzzi, Simone Mozzon, Tania Regimbau, A. J. Tanasijczuk, K. W. Tsang, S. B. Anderson, K. M. Aleman, M. Kolstein, Zachariah B. Etienne, Gianluca Grignani, P. J. Veitch, Jennifer Watchi, D. Tsai, M. Boer, J. B. Kanner, M. Pedraza, A. Lockwood, F. Cavalier, Santosh Roy, H. Fong, G. Greco, Y. Bai, A. K. Divakarla, S. Hochheim, N. A. Robertson, J. G. Bartlett, David Jonathan Hofman, B. Nayak, Jonathan Blackman, P. Prosposito, K. Toland, Giacomo Bruno, José A. Font, N. Singh, M. Mateu-Lucena, D. P. Kapasi, J. McIver, Karsten Danzmann, Andrea H. Tapia, Javier Sánchez, E. Schwartz, A. W. Criswell, M. Punturo, Leopoldo Milano, Slawomir Gras, S. W. S. Ng, M. J. Szczepańczyk, Denis Martynov, Marco Bazzan, C. Ingram, G. Vajente, S. M. Gaebel, Alessandro Bertolini, J.-G. Ducoin, R. C. Walet, V. P. Mitrofanov, M. Diaz-Ortiz, J. Venneberg, W. Del Pozzo, P. F. Cohadon, H. Heitmann, D. Sawant, Matteo Pegoraro, Piero Rettegno, Laura Cadonati, Department of Science and Technology (India), Ministry of Human Resource Development (India), Agencia Estatal de Investigación (España), Govern de les Illes Balears, Generalitat de Catalunya, Foundation for Polish Science, European Commission, Scottish Funding Council, Hungarian Scientific Research Fund, Belgian Science Policy Office, National Research Foundation of Korea, Research Grants Council (Hong Kong), National Natural Science Foundation of China, Leverhulme Trust, Ministry of Science and Technology (Taiwan), Kavli Institute for Particle Astrophysics and Cosmology, LIGO Sci Collaboration, Virgo Collaboration, Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, A., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., Agarwal, D., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Aleman, K. M., Allen, G., Allocca, A., Altin, P. A., Amato, A., Anand, S., Ananyeva, A., Anderson, S. B., Anderson, W. G., Angelova, S. V., Ansoldi, S., Antelis, J. M., Antier, S., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arene, M., Arnaud, N., Aronson, S. M., Arun, K. G., Asali, Y., Ashton, G., Aston, S. M., Astone, P., Aubin, F., Aufmuth, P., Aultoneal, K., Austin, C., Babak, S., Badaracco, F., Bader, M. K. M., Bae, S., Baer, A. M., Bagnasco, S., Bai, Y., Baird, J., Ball, M., Ballardin, G., Ballmer, S. W., Bals, M., Balsamo, A., Baltus, G., Banagiri, S., Bankar, D., Bankar, R. S., Barayoga, J. C., Barbieri, C., Barish, B. C., Barker, D., Barneo, P., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Barton, M. A., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Baylor, A. C., Bazzan, M., Becsy, B., Bedakihale, V. M., Bejger, M., Belahcene, I., Benedetto, V., Beniwal, D., Benjamin, M. G., Bennett, T. F., Bentley, J. D., Benyaala, M., Bergamin, F., Berger, B. 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R, Maggiore, R, Majorana, E, Maksimovic, I, Maliakal, S, Malik, A, Man, N, Mandic, V, Mangano, V, Mango, J, Mansell, G, Manske, M, Mantovani, M, Mapelli, M, Marchesoni, F, Marion, F, Mark, Z, Marka, S, Marka, Z, Markakis, C, Markosyan, A, Markowitz, A, Maros, E, Marquina, A, Marsat, S, Martelli, F, Martin, I, Martin, R, Martinez, M, Martinez, V, Martinovic, K, Martynov, D, Marx, E, Masalehdan, H, Mason, K, Massera, E, Masserot, A, Massinger, T, Masso-Reid, M, Mastrogiovanni, S, Matas, A, Mateu-Lucena, M, Matichard, F, Matiushechkina, M, Mavalvala, N, Mccann, J, Mccarthy, R, Mcclelland, D, Mcclincy, P, Mccormick, S, Mcculler, L, Mcghee, G, Mcguire, S, Mcisaac, C, Mciver, J, Mcmanus, D, Mcrae, T, Mcwilliams, S, Meacher, D, Mehmet, M, Mehta, A, Melatos, A, Melchor, D, Mendell, G, Menendez-Vazquez, A, Menoni, C, Mercer, R, Mereni, L, Merfeld, K, Merilh, E, Merritt, J, Merzougui, M, Meshkov, S, Messenger, C, Messick, C, Meyers, P, Meylahn, F, Mhaske, A, Miani, A, Miao, H, Michaloliakos, I, 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Steinlechner, J, Steinlechner, S, Stops, D, Stover, M, Strain, K, Strang, L, Stratta, G, Strunk, A, Sturani, R, Stuver, A, Sudbeck, J, Sudhagar, S, Sudhir, V, Suh, H, Summerscales, T, Sun, H, Sun, L, Sunil, S, Sur, A, Suresh, J, Sutton, P, Swinkels, B, Szczepanczyk, M, Szewczyk, P, Tacca, M, Tait, S, Talbot, C, Tanasijczuk, A, Tanner, D, Tao, D, Tapia, A, Martin, E, Tasson, J, Tenorio, R, Terkowski, L, Test, M, Thirugnanasambandam, M, Thomas, M, Thomas, P, Thompson, J, Thondapu, S, Thorne, K, Thrane, E, Tiwari, S, Tiwari, V, Toland, K, Tolley, A, Tonelli, M, Torres-Forne, A, Torrie, C, E Melo, I, Toyra, D, Trapananti, A, Travasso, F, Traylor, G, Tringali, M, Tripathee, A, Troiano, L, Trovato, A, Trudeau, R, Tsai, D, Tsang, K, Tse, M, Tso, R, Tsukada, L, Tsuna, D, Tsutsui, T, Turconi, M, Ubhi, A, Udall, R, Ueno, K, Ugolini, D, Unnikrishnan, C, Urban, A, Usman, S, Utina, A, Vahlbruch, H, Vajente, G, Vajpeyi, A, Valdes, G, Valentini, M, Valsan, V, Van Bakel, N, Van Beuzekom, M, Van Den 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M, Yoon, A, Yu, H, Zadrozny, A, Zanolin, M, Zelenova, T, Zendri, J, Zevin, M, Zhang, J, Zhang, L, Zhang, R, Zhang, T, Zhao, C, Zhao, G, Zhao, Y, Zhou, Z, Zhu, X, Zucker, M, Zweizig, J, UCL - SST/IRMP - Institut de recherche en mathématique et physique, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), 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), and Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: binary: orbit, neutron star: binary, Physics and Astronomy (miscellaneous), Astronomy, binary [neutron star], Astrophysics, Gravitational Waves, LIGO (Observatory), Neutron Stars, 01 natural sciences, neutron stars, General Relativity and Quantum Cosmology, Monte Carlo: Markov chain, Physics, Particles & Fields, binary stars, binary systems, Binary Systems, LIGO, gravitational wave, QC, QB, pulsar, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, education.field_of_study, Settore FIS/03, orbit [binary], General relativity, Physical Sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics - High Energy Astrophysical Phenomena, binary star, data analysis method, sensitivity [detector], gr-qc, frequency [modulation], Population, neutron star: spin, FOS: Physical sciences, alternative theories of gravity, Markov chain [Monte Carlo], General Relativity and Quantum Cosmology (gr-qc), Astronomy & Astrophysics, Gravitational Waves, Neutron Stars, Binary Systems, LIGO, Virgo, emission [gravitational radiation], Pulsar, binary: coalescence, 0103 physical sciences, Binary star, ddc:530, spin [neutron star], background [gravitational radiation], 010306 general physics, education, STFC, Orbital elements, Science & Technology, 010308 nuclear & particles physics, Gravitational wave, Virgo, gravitational radiation: background, modulation: frequency, RCUK, gravitational radiation detector, detector: sensitivity, Neutron star, VIRGO, gravitational radiation: emission, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, coalescence [binary], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: Rapidly spinning neutron stars are promising sources of continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter under extreme conditions. A significant fraction of the known pulsar population belongs to binary systems. Searching for unknown neutron stars in binary systems requires specialized algorithms to address unknown orbital frequency modulations. We present a search for continuous gravitational waves emitted by neutron stars in binary systems in early data from the third observing run of the Advanced LIGO and Advanced Virgo detectors using the semicoherent, GPU-accelerated, binaryskyhough pipeline. The search analyzes the most sensitive frequency band of the LIGO detectors, 50-300 Hz. Binary orbital parameters are split into four regions, comprising orbital periods of three to 45 days and projected semimajor axes of two to 40 light seconds. No detections are reported. We estimate the sensitivity of the search using simulated continuous wave signals, achieving the most sensitive results to date across the analyzed parameter space., The authors also gratefully acknowledge research support from these agencies, as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigación, the Vicepresidència i Conselleria d’Innovació, Recerca i Turisme, the Conselleria d’Educació i Universitat and the Direcció General de Política Universitaria i Recerca del Govern de les Illes Balears, the Conselleria d’Innovació, Universitats, Ciència i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, the Barcelona Supercomputing Center—Centro Nacional de Supercomputación, Spain, the National Science Centre of Poland, and the Foundation for Polish Science (FNP), the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertées (ARC) and Fonds Wetenschappelijk Onderzoek—Vlaanderen (FWO), Belgium, the Paris Île-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, the Natural Science and Engineering Research Council Canada, Canadian Foundation for Innovation (CFI), the Brazilian Ministry of Science, Technology, and Innovations, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan, the U.S. DOE, and the Kavli Foundation.
Published: 2021
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8. Characterizing the observation bias in gravitational-wave detections and finding structured population properties

Author: Doğa Veske, Imre Bartos, Zsuzsa Márka, and Szabolcs Márka
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, FOS: Physical sciences, Astronomy and Astrophysics, General Relativity and Quantum Cosmology (gr-qc), Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), General Relativity and Quantum Cosmology
Abstract: The observed distributions of the source properties from gravitational-wave detections are biased due to the selection effects and detection criteria in the detections, analogous to the Malmquist bias. In this work, this observation bias is investigated through its fundamental statistical and physical origins. An efficient semi-analytical formulation for its estimation is derived which is as accurate as the standard method of numerical simulations, with only a millionth of the computational cost. Then, the estimated bias is used for unmodelled inferences on the binary black hole population. These inferences show additional structures, specifically two peaks in the joint mass distribution around binary masses $\sim10$ M$_\odot$ and $\sim30$ M$_\odot$. Example ready-to-use scripts and some produced datasets for this method are shared in an online repository., Comment: Accepted to ApJ. 8 pages, 3 figures + 2 page appendix
Published: 2021
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9. Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars

Author: D. Rosińska, Patrice Hello, I. M. Pinto, Stephane Perries, I. La Rosa, Jean-René Cudell, S. Ponrathnam, Chunnong Zhao, G. Pagliaroli, W. Z. Korth, Torrey Cullen, S. H. Huttner, F. Garufi, Rakesh Kumar, Gor Oganesyan, O. Schwarm, Bernard F. Whiting, R. L. Savage, M. Laxen, Anchal Gupta, S. Hochheim, N. A. Robertson, A. F. Brooks, P. J. Quinonez, Andrew Melatos, M. Lorenzini, Surendra Nadh Somala, David Jones, David H. Shoemaker, J. D. Callaghan, Angela Trapananti, H. Rafferty, I. Dorrington, I. Di Palma, J. G. Bartlett, Yu Huang, Geert Raaijmakers, F. Y. Khalili, Q. Chu, J. H. Briggs, Mark Hannam, Marco Cavaglia, Subroto Mukherjee, David Jonathan Hofman, Lindsay DeMarchi, H. Sun, V. JaberianHamedan, Liam Cunningham, V. Kringel, I. M. Romero-Shaw, R. Tso, Jonathan Blackman, Frances Hellman, I. Molina, Jürgen Heinze, P. J. Sutton, Tyson Littenberg, G. Valdes, A. Adams, Laura Cadonati, Ken K. Y. Ng, K. Toland, T. D. Creighton, S. Barnum, R. Kirchhoff, S. P. Jadhav, V. Fafone, Kendall Ackley, R. K. Nayak, H. Y. Chia, A. Strunk, D. Petterson, Pablo Cerdá-Durán, Vivien Raymond, B. Edelman, G. Stolle-McAllister, M. Was, Giacomo Bruno, Sheelu Abraham, J. D. Bentley, I. C. F. Wong, Peter Aufmuth, Tania Regimbau, A. J. Tanasijczuk, L. Mereni, Patrick M. Koch, S. Banagiri, T. L. Lam, José A. Font, Tomasz Bulik, N. Singh, S. B. Anderson, J. Gais, Maya Fishbach, Tim Dietrich, Manel Molina-Ruiz, S. B. Coughlin, M. Mateu-Lucena, Jessica Steinlechner, M. Kolstein, A. Neunzert, D. Fiorucci, C. L. Chan, M. Heurs, A. K. Prajapati, A. R. Wade, M. Patel, Benjamin Stappers, W. Kastaun, H. Qi, J. H. Romie, G. Kuehn, F. J. Raab, Zachariah B. Etienne, N. Mukund, Jennifer Watchi, L. Kleybolte, Daniel R. George, Susan M. Scott, E. K. Porter, V. B. Adya, T. P. Downes, C. Horst, M. Pedraza, F. Muciaccia, A. Lockwood, F. Cavalier, A. Bals, G. Baltus, Karl Gill, V. Srivastava, M. Fays, Santosh Roy, A. Allocca, A. M. Farah, M. F. Carney, A. F. Helmling-Cornell, Ajay Kumar, C. Whittle, A. K. Divakarla, M. Mondin, M. M. Hanke, H. Vocca, L. Xiao, C. M. Mow-Lowry, Sergey P. Vyatchanin, L. Aiello, R. Green, V. Sequino, C. J. Richardson, Alberto Vecchio, Geoffrey Mo, J. M. Fishner, Will M. Farr, M. Montani, Nancy Aggarwal, Anupam Sharma, Lionel London, P. Kumar, A. Singha, Matteo Breschi, László Á. Gergely, Terry G. McRae, L. G. Prokhorov, Alessandro Longo, Richard J. Oram, D. D'Urso, François Bondu, Reed Essick, S. Kandhasamy, B. Sorazu, Lili Yang, M. Branchesi, D. Y. T. Pong, R. Gustafson, P. Barneo, A. F. Vargas, Chad Hanna, A. Bramley, C. Kimball, J. Oberling, M. Pirello, Fiodor Sorrentino, A. Di Lieto, M. Saleem, Matthew Bailes, M. Vasúth, A. Malik, S. Gaudio, G. R. Johns, Michael Williams, Moritz Mehmet, C. Darsow-Fromm, A. L. Stuver, T. J. Slaven-Blair, R. S. Bankar, M. C. Milovich-Goff, J. L. Wright, S. Bagnasco, P. Fulda, D. Hoyland, J. Casanueva Diaz, V. M. Bedakihale, P. Schale, C. Van Den Broeck, J. L. Willis, M. Eisenmann, E. Sowell, Ofek Birnholtz, J. Smetana, I. Dave, B. Hughey, P. Couvares, B. Idzkowski, V. Loriette, V. Skliris, S. T. Countryman, Surabhi Sachdev, Christopher J. Moore, Alec Mishkin, R. Cavalieri, A. K. Srivastava, A. E. Pace, A. Basti, Ryan N. Lang, Krzysztof Piotrzkowski, A. E. Tolley, J.-P. Coulon, E. A. Chase, Z. Frei, A. Macquet, Daichi Tsuna, D. L. Ferguson, M. J. Szczepańczyk, Denis Martynov, Marco Bazzan, C. Ingram, L. Pinard, Charalampos Markakis, F. Badaracco, T. T. Nguyen, Andrea Chincarini, Minkyun Noh, T. Z. Summerscales, E. Payne, T. Sadecki, M. Piendibene, S. Grunewald, R. Prasanna, Alessandra Corsi, D. Laghi, E. J. Daw, Maurizio Canepa, P. H. Nguyen, Antonio Marquina, Eric Hennes, A. S. Ubhi, T. A. Ferreira, K. D. Giardina, E. M. Santos, J. K. Wofford, M. A. Page, P. W. F. Forsyth, J. S. Lange, B. E. Ewing, M. C. Tringali, E. Massera, Y. Asali, S. Raja, S. Maliakal, C. Di Giorgio, J. Bidler, R. Dean, H. J. Bulten, D. B. Tanner, K. Rose, M. Pracchia, S. E. 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Kovalam, Spectroscopies optiques des matériaux verres, amorphes et à nanoparticules (SOPRANO), Institut Lumière Matière [Villeurbanne] (ILM), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-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), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut des Fonctions Optiques pour les Technologies de l'informatiON (Institut FOTON), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS)-Université Bretagne Loire (UBL)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Laboratoire Kastler Brossel (LKB [Collège de France]), Collège de France (CdF (institution))-Sorbonne Université (SU)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), 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), Laboratoire des matériaux avancés (LMA), 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)-Centre National de la Recherche Scientifique (CNRS), Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Nice, France., Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), Centre Scientifique de Monaco (CSM), Musee oceanographique de Monaco, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (INFN, Sezione di Torino), Istituto Nazionale di Fisica Nucleare (INFN), Museo Storico della Fisica e Centro di Studi e Ricerche 'Enrico Fermi', Roma, Institut des Hautes Etudes Scientifiques (IHES), IHES, Abbott, R., Abbott, T. 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C., Barker, D., Barneo, P., Barnum, S., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Bawaj, M., Bayley, J. C., Bazzan, M., Becher, B. R., Becsy, B., Bedakihale, V. M., Bejger, M., Belahcene, I., Beniwal, D., Benjamin, M. G., Bennett, T. F., Bentley, J. D., Bergamin, F., Berger, B. K., Bergmann, G., Bernuzzi, S., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhandare, R., Bhandari, A. V., Bhattacharjee, D., Bidler, J., Bilenko, I. A., Billingsley, G., Birney, R., Birnholtz, O., Biscans, S., Bischi, M., Biscoveanu, S., Bisht, A., Bitossi, M., Bizouard, M. -A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Blanch, O., Bobba, F., Bode, N., Boer, M., Boetzel, Y., Bogaert, G., Boldrini, M., Bondu, F., Bonnand, R., Booker, P., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bossilkov, V., Boudart, V., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Bramley, A., Branchesi, M., Brau, J. 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L., D'Antonio, S., Danzmann, K., Darsow-Fromm, C., Dasgupta, A., Datrier, L. E. H., Dattilo, V., Dave, I., Davier, M., Davies, G. S., Davis, D., Daw, E. J., Dean, R., Debra, D., Deenadayalan, M., Degallaix, J., De Laurentis, M., Deleglise, S., Del Favero, V., De Lillo, N., Del Pozzo, W., Demarchi, L. M., De Matteis, F., D'Emilio, V., Demos, N., Denker, T., Dent, T., Depasse, A., De Pietri, R., De Rosa, R., De Rossi, C., Desalvo, R., De Varona, O., Dhurandhar, S., Diaz, M. C., Diaz-Ortiz, M., Didio, N. A., Dietrich, T., Di Fiore, L., Difronzo, C., Di Giorgio, C., Di Giovanni, F., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Ding, B., Di Pace, S., Di Palma, I., Di Renzo, F., Divakarla, A. K., Dmitriev, A., Doctor, Z., D'Onofrio, L., Donovan, F., Dooley, K. L., Doravari, S., Dorrington, I., Downes, T. P., Drago, M., Driggers, J. C., Du, Z., Ducoin, J. -G., Dupej, P., Durante, O., D'Urso, D., Duverne, P. -A., Dwyer, S. E., Easter, P. J., Eddolls, G., Edelman, B., Edo, T. B., Edy, O., Effler, A., Eichholz, J., Eikenberry, S. S., Eisenmann, M., Eisenstein, R. A., Ejlli, A., Errico, L., Essick, R. C., Estelles, H., Estevez, D., Etienne, Z. B., Etzel, T., Evans, M., Evans, T. M., Ewing, B. E., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Farah, A. M., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fazio, M., Feicht, J., Fejer, M. M., Feng, F., Fenyvesi, E., Ferguson, D. L., Fernandez-Galiana, A., Ferrante, I., Ferreira, T. A., Fidecaro, F., Figura, P., Fiori, I., Fiorucci, D., Fishbach, M., Fisher, R. P., Fishner, J. M., Fittipaldi, R., Fitz-Axen, M., Fiumara, V., Flaminio, R., Floden, E., Flynn, E., Fong, H., Font, J. A., Forsyth, P. W. F., Fournier, J. -D., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fronze, G. G., Fulda, P., Fyffe, M., Gabbard, H. A., Gadre, B. U., Gaebel, S. M., Gair, J. 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Z., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hannuksela, O. A., Hannuksela, O., Hansen, H., Hansen, T. J., Hanson, J., Harder, T., Hardwick, T., Haris, K., Harms, J., Harry, G. M., Harry, I. W., Hartwig, D., Hasskew, R. K., Haster, C. -J., Haughian, K., Hayes, F. J., Healy, J., Heidmann, A., Heintze, M. C., Heinze, J., Heinzel, J., Heitmann, H., Hellman, F., Hello, P., Helmling-Cornell, A. F., Hemming, G., Hendry, M., Heng, I. S., Hennes, E., Hennig, J., Hennig, M. H., Vivanco, F. H., Heurs, M., Hild, S., Hill, P., Hines, A. S., Hochheim, S., Hofgard, E., Hofman, D., Hohmann, J. N., Holgado, A. M., Holland, N. A., Hollows, I. J., Holmes, Z. J., Holt, K., Holz, D. E., Hopkins, P., Horst, C., Hough, J., Howell, E. J., Hoy, C. G., Hoyland, D., Huang, Y., Hubner, M. T., Huddart, A. D., Huerta, E. A., Hughey, B., Hui, V., Husa, S., Huttner, S. H., Hutzler, B. M., Huxford, R., Huynh-Dinh, T., Idzkowski, B., Iess, A., Imperato, S., Inchauspe, H., Ingram, C., Intini, G., Isi, M., Iyer, B. R., Jaberianhamedan, V., Jacqmin, T., Jadhav, S. J., Jadhav, S. P., James, A. L., Jani, K., Janssens, K., Janthalur, N. N., Jaranowski, P., Jariwala, D., Jaume, R., Jenkins, A. C., Jeunon, M., Jiang, J., Johns, G. R., Jones, A. W., Jones, D. I., Jones, J. D., Jones, P., Jones, R., Jonker, R. J. G., Ju, L., Junker, J., Kalaghatgi, C. V., Kalogera, V., Kamai, B., Kandhasamy, S., Kang, G., Kanner, J. B., Kapadia, S. J., Kapasi, D. P., Karathanasis, C., Karki, S., Kashyap, R., Kasprzack, M., Kastaun, W., Katsanevas, S., Katsavounidis, E., Katzman, W., Kawabe, K., Kefelian, F., Keitel, D., Key, J. S., Khadka, S., Khalili, F. Y., Khan, I., Khan, S., Khazanov, E. A., Khetan, N., Khursheed, M., Kijbunchoo, N., Kim, C., Kim, G. J., Kim, J. C., Kim, K., Kim, W., Kim, W. S., Kim, Y. -M., Kimball, C., King, P. J., Kinley-Hanlon, M., Kirchhoff, R., Kissel, J. S., Kleybolte, L., Klimenko, S., Knowles, T. D., Knyazev, E., Koch, P., Koehlenbeck, S. M., Koekoek, G., Koley, S., Kolstein, M., Komori, K., Kondrashov, V., Kontos, A., Koper, N., Korobko, M., Korth, W. Z., Kovalam, M., Kozak, D. B., Kramer, C., Kringel, V., Krishnendu, N. V., Krolak, A., Kuehn, G., Kumar, A., Kumar, P., Kumar, R., Kuns, K., Kwang, S., Lackey, B. D., Laghi, D., Lalande, E., Lam, T. L., Lamberts, A., Landry, M., Lane, B. B., Lang, R. N., Lange, J., Lantz, B., Lanza, R. K., Rosa, I. L., Lartaux-Vollard, A., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lecoeuche, Y. K., Lee, H. M., Lee, H. W., Lee, J., Lee, K., Lehmann, J., Leon, E., Leroy, N., Letendre, N., Levin, Y., Li, A., Li, J., Li, K. J. L., Li, T. G. F., Li, X., Linde, F., Linker, S. D., Linley, J. N., Littenberg, T. B., Liu, J., Liu, X., Llorens-Monteagudo, M., Lo, R. K. L., Lockwood, A., London, L. T., Longo, A., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lousto, C. O., Lovelace, G., Lower, M., Luck, H., Lumaca, D., Lundgren, A. P., Ma, Y., Macas, R., Macinnis, M., Macleod, D. M., Macmillan, I. A. O., Macquet, A., Magana Hernandez, I., Magana-Sandoval, F., Magazzu, C., Magee, R. M., Majorana, E., Maksimovic, I., Maliakal, S., Malik, A., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Mapelli, M., Marchesoni, F., Marion, F., Marka, S., Marka, Z., Markakis, C., Markosyan, A. S., Markowitz, A., Maros, E., Marquina, A., Marsat, S., Martelli, F., Martin, I. W., Martin, R. M., Martinez, M., Martinez, V., Martynov, D. V., Masalehdan, H., Mason, K., Massera, E., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matas, A., Mateu-Lucena, M., Matichard, F., Matiushechkina, M., Mavalvala, N., Maynard, E., Mccann, J. J., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcculler, L., Mcguire, S. C., Mcisaac, C., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meacher, D., Meadors, G. 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Lasky, Pd, Lecoeuche, Yk, Lee, Hm, Lee, Hw, Li, Kjl, Li, Tgf, Linker, Sd, Linley, Jn, Littenberg, Tb, Lo, Rkl, London, Lt, Lough, Jd, Lousto, Co, Lundgren, Ap, Macleod, Dm, Macmillan, Iao, Hernandez, Im, Magee, Rm, Mansell, Gl, Martin, Iw, Martin, Rm, Martynov, Dv, Massinger, Tj, Mccann, Jj, Mcclelland, De, Mcguire, Sc, Mcmanus, Dj, Mcwilliams, St, Meadors, Gd, Mehta, Ak, Melchor, Da, Mercer, Ra, Merilh, El, Merritt, Jd, Meyers, Pm, Miller, Al, Mills, Jc, Milovich-Goff, Mc, Mir, Lm, Mitrofanov, Vp, Mohapatra, Srp, Mohite, Sr, Moore, Cj, Mow-Lowry, Cm, Muniz, Ea, Murray, Pg, Nadji, Sl, Nayak, Rk, Neil, Bf, Nelson, Tjn, Ng, Ky, Nichols, Sa, Nuttall, Lk, Ogin, Gh, Oh, Jj, Oh, Sh, Okada, Ma, Oram, Rj, Ormiston, Rg, Ortega, Lf, Ottaway, Dj, Owen, Bj, Pace, Ae, Page, Ma, Pai, Sa, Palamos, Jr, Panda, Pk, Pang, Th, Pant, Bc, Pechsiri, Tc, Perez, Cj, Pfeiffer, Hp, Pham, Ka, Piccinni, Oj, Pinto, Im, Pong, Dyt, Porter, Ek, Prajapati, Ak, Prodi, Ga, Quinonez, Pj, Raab, Fj, Rail, Sx, Ramirez, Ke, 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D., O’Dell, J., O’Reilly, B., O’Shaughnessy, R., Périgois, C., Perriès, S., Pinto, I. M., Pürrer, M., Rosińska, D., Roy, Santosh, Roy, Soumen, Schönbeck, A., Stolle-McAllister, G., Südbeck, J., Szczepańczyk, M. J., San Martin, E. N. Tapia, Tiwari, Shubhanshu, Tiwari, Srishti, Torres-Forné, A., e Melo, I. Tosta, Töyrä, D., Bakel, N. van, Beuzekom, M. van, van den Brand, J. F. J., Broeck, C. Van Den, Schaaf, L. van der, Heijningen, J. V. van, Vasúth, M., Viceré, A., Weßels, P., Yu, Hang, Yu, Haocun, Zadrożny, A., RS: FSE Grav. waves and fundamental physics, Grav. waves and fundamental physics, Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Collège de France (CdF (institution)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Joseph Louis LAGRANGE (LAGRANGE), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), LIGO Scientific, Virgo, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), 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), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut des Hautes Études Scientifiques (IHES), The LIGO Scientific Collaboration, The Virgo Collaboration, and Van Swinderen Institute for Particle Physics and G
Subjects: Gravitational waves, Neutron stars, Pulsars, Gravitational wave sources, 010504 meteorology & atmospheric sciences, Astronomy, Astrophysics, Vela, 01 natural sciences, General Relativity and Quantum Cosmology, [SPI]Engineering Sciences [physics], neutron, Millisecond pulsar, emission, 010303 astronomy & astrophysics, QC, QB, Settore FIS/01, Physics, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), [PHYS]Physics [physics], Astrophysics::Instrumentation and Methods for Astrophysics, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics - High Energy Astrophysical Phenomena, Gravitational-Waves, Pulsars, Neutron Stars, Gravitational wave, PROPER MOTION, Proper motion, gr-qc, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Neutron star, General Relativity and Quantum Cosmology (gr-qc), Gravitational-Waves, SEARCHES, Settore FIS/05 - Astronomia e Astrofisica, Pulsar, 0103 physical sciences, [CHIM]Chemical Sciences, Astrophysique, STFC, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, crab pulsar, Crab Pulsar, RCUK, Astronomy and Astrophysics, Neutron Stars, Gravitational waves, Neutron stars, Pulsars, Gravitational wave sources, LIGO, Space and Planetary Science, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time, we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limits on gravitational-wave emission from recycled pulsars inferred from their observed spin-downs, and constrain their equatorial ellipticities to be less than 10-8. For each of the five pulsars, we perform targeted searches that assume a tight coupling between the gravitational-wave and electromagnetic signal phase evolution. We also present constraints on PSR J0711-6830, the Crab pulsar, and the Vela pulsar from a search that relaxes this assumption, allowing the gravitational-wave signal to vary from the electromagnetic expectation within a narrow band of frequencies and frequency derivatives., 0, info:eu-repo/semantics/published
Published: 2020
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10. The IceCube Pie Chart: Relative Source Contributions to the Cosmic Neutrino Flux

Author: Imre Bartos, Z. Márka, Doğa Veske, Marek Kowalski, and S. Márka
Subjects: Active galactic nucleus, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Flux, Source type, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, neutrino: flux, IceCube, blazar, law.invention, law, AGN, Blazar, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, COSMIC cancer database, Astrophysics::Instrumentation and Methods for Astrophysics, Pie chart, Astronomy and Astrophysics, flux [neutrino], sensitivity, Unknown Source, Space and Planetary Science, fractional, ddc:520, Neutrino, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The astrophysical journal 921(1), 45 (2021). doi:10.3847/1538-4357/ac1c7b, Neutrino events from IceCube have recently been associated with multiple astrophysical sources. Interestingly, these likely detections represent three distinct astrophysical source types: active galactic nuclei (AGNs), blazars, and tidal disruption events (TDEs). Here, we compute the expected contributions of AGNs, blazars, and TDEs to the overall cosmic neutrino flux detected by IceCube based on the associated events, IceCube��s sensitivity, and the source types�� astrophysical properties. We find that, despite being the most commonly identified sources, blazars cannot contribute more than 11% of the total flux (90% credible level), consistent with existing limits from stacked searches. On the other hand, we find that either AGNs or TDEs could contribute more than 50% of the total flux (90% credible level), although stacked searches further limit the TDE contribution to ��30%. We also find that so-far unknown source types contribute at least 10% of the total cosmic flux with a probability of 80%. We assemble a pie chart that shows the most likely fractional contribution of each source type to IceCube��s total neutrino flux., Published by Univ., Chicago, Ill. [u.a.]
Published: 2021
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11. Have hierarchical three-body mergers been detected by LIGO/Virgo?

Author: Andrew G. Sullivan, Doğa Veske, Johan Samsing, Imre Bartos, Zsuzsa Márka, Szabolcs Marka, and K. Rainer Corley
Subjects: Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, BINARIES, General Relativity and Quantum Cosmology, Binary black hole, Frequentist inference, Time windows, GLOBULAR-CLUSTERS, 0103 physical sciences, LIGO, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Gravitational wave, Astronomy and Astrophysics, Observable, CATALOG, EVOLUTION, Black hole, ) black hole mergers [(transients], gravitational waves, Space and Planetary Science, TESTS, Astrophysics - High Energy Astrophysical Phenomena, Merge (version control), BLACK-HOLE MERGERS
Abstract: One of the proposed channels of binary black hole mergers involves dynamical interactions of three black holes. In such scenarios, it is possible that all three black holes merge in a so-called hierarchical merger chain, where two of the black holes merge first and then their remnant subsequently merges with the remaining single black hole. Depending on the dynamical environment, it is possible that both mergers will appear within the observable time window. Here we perform a search for such merger pairs in the public available LIGO and Virgo data from the O1/O2 runs. Using a frequentist p-value assignment statistics we do not find any significant merger pair candidates, the most significant being GW170809-GW151012 pair. Assuming no observed candidates in O3/O4, we derive upper limits on merger pairs to be $\sim11-110\ {\rm year^{-1}Gpc^{-3}}$, corresponding to a rate that relative to the total merger rate is $\sim 0.1-1.0$. From this we argue that both a detection and a non-detection within the next few years can be used to put useful constraints on some dynamical progenitor models., 7 pages, 4 figures
Published: 2020
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12. GW190521: A Binary Black Hole Merger with a Total Mass of 150 M⊙

Author: Will M. Farr, L. Xiao, A. M. Holgado, K. G. Arun, M. Montani, Nancy Aggarwal, Zahoor Ali Khan, Roman Schnabel, H. L. Griggs, J. E. Brau, A. A. van Veggel, Efim A. Khazanov, G. Ballardin, P. Fulda, J. Smetana, R. Kirchhoff, B. L. Pearlstone, S. P. Jadhav, Patrick Das Gupta, S. G. Crowder, J. Bosveld, V. Fafone, J. L. Willis, M. Eisenmann, Ofek Birnholtz, Sebastiano Bernuzzi, Simone Mozzon, I. Dave, B. Hughey, O. Halim, Laura Cadonati, Carl-Johan Haster, Kendall Ackley, R. K. Nayak, S. D. Linker, K. W. Tsang, L. Rolland, H. Y. Chia, Mark A. Scheel, R. S. Bankar, M. C. Milovich-Goff, L. Kleybolte, Gianluca Grignani, Fabrizio Barone, A. Allocca, M. F. Carney, M. Rakhmanov, M. Kasprzack, K. Rose, S. Leavey, Hai-Ping Cheng, A. Iess, J. L. Wright, N. Man, Ajay Kumar, F. Clara, Alessandra Corsi, C. Whittle, D. Laghi, Daniel R. George, K. Haughian, M. Boer, J. B. Kanner, M. Mondin, S. E. Gossan, S. Gaudio, L. K. Nuttall, R. Macas, G. Billingsley, S. Macfoy, Azadeh Keivani, A. R. Guimaraes, Susan M. Scott, V. B. Adya, J. S. Areeda, G. R. Johns, H. Fong, G. Greco, E. J. Daw, Maurizio Canepa, P. H. Nguyen, Moritz Mehmet, C. Darsow-Fromm, B. B. Lane, M. Vardaro, S. Mastrogiovanni, Chad Hanna, A. Bramley, Antonio Marquina, Eric Hennes, A. S. Ubhi, T. A. Ferreira, P. Kumar, Héctor Estellés, C. Kimball, J. Oberling, M. Pirello, Charalampos Markakis, Y. K. Lecoeuche, G. M. Harry, K. Venkateswara, R. Cotesta, A. Cumming, F. Di Renzo, E. Genin, T. R. Saravanan, J. Zhang, F. Baldaccini, L. F. Ortega, R. Cummings, D. W. Yeeles, Felice Sorrentino, D. Moraru, K. D. Giardina, E. M. Santos, J. K. Wofford, M. A. Page, P. W. F. Forsyth, C. De Rossi, J. K. Blackburn, F. L. Linde, E. Chassande-Mottin, Sylvain Marsat, Sheila Rowan, M. Pürrer, C. Di Giorgio, C. Chan, Hartmut Grote, G. Rutins, Graham Woan, Robert L. Byer, J. Bidler, C. L. Tinsman, M. Fitz-Axen, P. Bacon, Daniel E. Holz, David A. Williams, J. Jones, I. W. Harry, Z. A. Warden, R. Gouaty, S. Wang, B. Patricelli, D. S. Wu, Margaret Millhouse, S. G. Gaonkar, Haixing Miao, H. Ohta, F. Di Giovanni, N. Letendre, Matteo Breschi, K. L. Dooley, Aaron Zimmerman, D. Nothard, Fangchen Feng, Karsten Danzmann, Andrea H. Tapia, G. Losurdo, Lisa Barsotti, Serena Vinciguerra, Benno Willke, Anirban Dasgupta, R. J. G. Jonker, M. Kovalam, C. Di Fronzo, Yuri Levin, J. Gniesmer, Alessandro Nagar, J. S. Lange, B. E. Ewing, Yang Yang, Xing-Jiang Zhu, E. Floden, Gianpietro Cagnoli, Giuseppe Intini, M. Punturo, G. G. Fronzé, M. C. Tringali, Alec Mishkin, R. Cavalieri, W. Parker, Stuart Reid, F. J. Hayes, Jacob Scheuer, I. Michaloliakos, G. Koekoek, A. J. Weinstein, Anindita Ganguly, Slawomir Gras, S. W. S. Ng, S. L. Danilishin, F. Nocera, Alicia M. Sintes, M. Curyło, Kun Li, T. Zhang, C. Cahillane, J. Hennig, V. Gayathri, Neil J. Cornish, F. Vetrano, Parthanil Roy, S. E. Dwyer, David Keitel, Nathan K. Johnson-McDaniel, S. J. Cooper, Jay D. Tasson, M. Landry, F. Frasconi, S. Hochheim, N. A. Robertson, J. G. Bartlett, Márton Tápai, Thibaut Jacqmin, C. I. Torrie, G. Pagano, Bernard F. Schutz, Li Ju, A. K. Srivastava, A. E. Pace, W. H. Wang, A. Basti, Ryan N. Lang, Krzysztof Piotrzkowski, T. J. Slaven-Blair, Albert Lazzarini, S. Walsh, Miriam Cabero, Alessandra Buonanno, R. Metzdorff, A. Lartaux-Vollard, Daniel A. Shaddock, Brittany Kamai, C. V. Kalaghatgi, J. Hanson, M. J. Szczepańczyk, Denis Martynov, Marco Bazzan, D. Singh, R. Flaminio, C. Ingram, A. Tripathee, L. Di Fiore, B. Mours, Suvadeep Bose, Gabrielle Allen, A. C. Green, David Jonathan Hofman, A. V. Bhandari, Z. Márka, F. Meylahn, C. Austin, M. Barsuglia, M. Oliver, L. Pinard, Douglas Davis, Geraint Pratten, Liam Cunningham, M. Merzougui, I. M. Pinto, D. Bersanetti, I. La Rosa, Jean-René Cudell, W. Z. Korth, Torrey Cullen, R. Jaume, R. A. Eisenstein, B. J. J. Slagmolen, Hee-Suk Cho, Jishnu Suresh, G. D. Meadors, Francisco Hernandez Vivanco, Hang Yu, Fausto Acernese, R. Gray, G. Vajente, S. M. Gaebel, J.-P. Coulon, M. Haney, Samaya Nissanke, E. A. Chase, Z. Frei, M. A. Bizouard, B. K. Berger, N. V. Krishnendu, V. Sequino, S. Caride, I. Belahcene, M. Cieślar, A. K. Y. Li, C. Gray, G. H. Ogin, T. J. Shaffer, M. Mantovani, J.-D. Fournier, Jonathan Blackman, Hyang Woon Lee, A. Grant, F. Garufi, Surendra Nadh Somala, K. Toland, K. W. Chung, J. S. Kissel, Eric Thrane, Giacomo Bruno, D. Ugolini, Roberto Chierici, E. Maynard, C. Michel, A. Sur, H. M. Lee, Alessandro Bertolini, T. Hardwick, D. Steinmeyer, L. Zhang, E. Cesarini, F. Travasso, Michał Bejger, M. Croquette, D. Töyrä, O. Sauter, S. Márka, Philip F. Hopkins, R. P. Udall, N. Sennett, Francesco Pannarale, Soichiro Morisaki, I. Fiori, S. Koley, M. Brinkmann, Silvia Corezzi, S. Bae, D. Pascucci, José A. Font, Kenneth A. Strain, Jimin George, M. Sieniawska, W. Katzman, P. Thomas, M. Arène, J. Castañeda, B. U. Gadre, E. Coccia, P. Couvares, A. Balsamo, S. Khadka, A. Rocchi, N. Singh, David Jones, Maya Fishbach, T. D. Knowles, Marica Valentini, M. E. Zucker, B. A. Weaver, J. G. Rollins, E. Hofgard, T. Zelenova, Riccardo Bassiri, L.-W. Wei, Magnus Manske, T. A. Callister, N. Kijbunchoo, Edoardo Milotti, B. Lantz, R. L. Savage, A. S. Bell, M. Laxen, Anchal Gupta, Yu Huang, Tyson Littenberg, E. J. Fauchon-Jones, M. Lormand, D. J. Stops, Odylio D. Aguiar, J. S. H. Lee, G. Mendell, S. J. Jadhav, E. Lalande, Eyal Schwartz, B. Goncharov, R. Birney, Aldo Ejlli, A. Dmitriev, Gregory Ashton, K. Chakravarti, Fabio Marchesoni, Shawn Rosofsky, Archisman Ghosh, J.-G. Ducoin, A. K. Zadrożny, H. S. Chen, Kyungmin Kim, Debarati Chatterjee, B. O'Reilly, S. Katsanevas, P. Gruning, Rakesh Kumar, Gor Oganesyan, Mario Spera, Jan Harms, A. S. Sengupta, M. Khursheed, F. Brighenti, Aniello Grado, S. J. Rowlinson, R. C. Walet, D. Buskulic, E. Cuoco, Binlei Ding, A. Gupta, S. Meshkov, Seog Oh, Marco Cavaglia, E. Maros, A. L. James, V. P. Mitrofanov, Geert Raaijmakers, F. Y. Khalili, Ofelia Durante, G. Valdes, D. Fiorucci, A. K. Prajapati, T. Dal Canton, Felix Wellmann, J. Warner, R. Passaquieti, Alexander H. Nitz, C. Osthelder, M. Bawaj, A. Aich, D. Passuello, Stephane Perries, Sarp Akcay, C. Affeldt, E. Goetz, S. Penn, Subroto Mukherjee, Piotr Jaranowski, C. Rajan, Tania Regimbau, A. J. Tanasijczuk, J. D. E. Creighton, R. M. S. Schofield, A. Effler, J. Jiang, V. Hui, A. Perreca, G. Gemme, M. Drago, Jade Powell, V. Mangano, T. C. Pechsiri, Michela Mapelli, J. Li, M. Nery, Guenakh Mitselmakher, Kris Ryan, S. Y. Hoback, G. A. Prodi, Madeline Wade, F. Cleva, L. Milano, P. Leaci, M. Diaz-Ortiz, D. Huet, W. Del Pozzo, M. Thomas, Rajesh Kumar, M. P. Ross, P. F. Cohadon, A. Macquet, M. Bischi, S. B. Anderson, Tim Dietrich, T. B. Edo, M. Pichot, Peter Aufmuth, Ken K. Y. Ng, T. Di Girolamo, Jing Wang, A. R. Wade, Kiran Prasai, C. M. Mow-Lowry, Sergey P. Vyatchanin, A. Grimaldi, Chris A. Collins, N. Radulesco, Ettore Majorana, Maximiliano Isi, L. Aiello, Patrick Godwin, Nikhil Sarin, D. Bankar, L. Kuo, H. Yamamoto, J. C. Driggers, A. M. Baer, H. Vahlbruch, Gunnar Riemenschneider, J. C. Mills, K. Riles, H. Middleton, Maria Ilaria Del Principe, László Á. Gergely, H. Heitmann, D. Sawant, Piero Rettegno, K. A. Santiago, M. Agathos, Soumen Roy, Jürgen Heinze, S. Ponrathnam, Chunnong Zhao, Daichi Tsuna, R. Green, R. DeSalvo, B. F. Neil, Al Imran Malik, S. H. Huttner, O. Schwarm, Zachariah B. Etienne, G. L. Mansell, Jennifer Watchi, V. Dattilo, Pablo Cerdá-Durán, Vivien Raymond, S. Karki, J. D. Callaghan, Benjamin J. Owen, J. F. J. van den Brand, D. Verkindt, H. Rafferty, S. Sunil, M. Tacca, Martin Hendry, Cecilio García-Quirós, A. F. Brooks, P. J. Quinonez, A. Cirone, M. Fyffe, O. V. Palashov, Sean T. McWilliams, F. Piergiovanni, E. M. Gretarsson, Andrew Melatos, M. Lorenzini, A. Masserot, Ying Guo, Peter Fritschel, M. Weinert, H. A. G. Gabbard, F. Fidecaro, I. M. Romero-Shaw, G. M. Guidi, Safura Sharifi, M. Masso-Reid, B. F. Whiting, H. K. Gulati, Valeria Sipala, David H. Reitze, Rahul Kashyap, C. McIsaac, N. De Lillo, Sascha Husa, G. Venugopalan, S. R. Mohite, D.B. DeBra, L. Errico, C. Olivetto, Gabriela Gonzalez, J. Casanueva Diaz, P. Schale, K. R. Corley, J. Petermann, M. C. Araya, Srishti Tiwari, C. Lazzaro, B. A. Boom, A. M. Sergeev, Lindsay DeMarchi, Ellen S. Howell, J. Glanzer, B. Edelman, R. Taylor, R. Abbott, Giovanni Carapella, R. K. Lanza, A. Schönbeck, P. Dupej, B. Rajbhandari, V. D'Emilio, V. Kringel, Daniel Wysocki, M. Was, Patricia Schmidt, Eric B. Flynn, B. Gateley, A. Trovato, Vuk Mandic, J. H. Briggs, T. P. Downes, G. S. Wallace, A. Singha, Stefan Hild, Y. Ma, D. Lumaca, M. Pedraza, M. C. Díaz, K. Chatziioannou, R. Tso, M. Chan, Mairi Sakellariadou, G. Pillant, A. Lockwood, Terry G. McRae, S. H. R. Yuen, O. de Varona, L. Mereni, Patrick M. Koch, S. Antier, F. Cavalier, A. Bals, Antonios Kontos, Junwei Cao, P. Ehrens, Mark Hannam, M. M. Hanke, K. Chandra, A. Brillet, D. Rose, C. Van Den Broeck, E. Sowell, P. J. King, M. Davier, M. J. Yap, Alejandro Torres-Forné, L. E. Sanchez, K. Mason, J. T. Whelan, S. Banagiri, S. Galaudage, T. L. Lam, Tomasz Bulik, K. Siellez, Nicolas Sanchis-Gual, K. A. Thorne, Paul M. Ricker, S. Fairhurst, J. Feicht, Satya Mohapatra, Gregorio Carullo, Shreya Anand, I. A. O. MacMillan, Deep Jariwala, Howard Pan, Aaron Buikema, L. G. Prokhorov, C. C. Wipf, H. Vocca, C. Palomba, S. Ascenzi, Tanja Hinderer, A. Strunk, E. C. Ferreira, G. Baltus, Santosh Roy, Sanjeev Dhurandhar, Joey Shapiro Key, Samuele Cortese, Y. Boetzel, T. Etzel, Charlie Hoy, Alessandro Longo, Richard J. Oram, D. D'Urso, P. Booker, O. Edy, J. A. Giaime, J. R. Sanders, A. K. Divakarla, Xin Chen, R. M. Martin, David A. Nichols, D. Corre, Y. M. Kim, François Bondu, Edward K. Porter, Maher Yazback, Tenglin Li, M. S. Shahriar, Sheelu Abraham, Enrico Calloni, G. Traylor, S. Soni, J. D. Bentley, G. Vedovato, L. E. H. Datrier, D. B. Kozak, Thomas Corbitt, D. Stocks, C. Messenger, F. Robinet, C. Vorvick, S. Doravari, B. D. Lackey, Q. Chu, J. Baird, F. Muciaccia, Anupam Sharma, Lionel London, L. Salconi, C. A. Costa, Isabel Cordero-Carrión, Alexander C. Jenkins, F. Badaracco, Jonathan E. Thompson, J. Calderón Bustillo, P. Grassia, Kipp Cannon, M. Steinke, P. Ciecielag, C. S. Unnikrishnan, P. J. Veitch, M. J. Cowart, D. L. Ferguson, A. Markowitz, D. Estevez, P. Clearwater, I. C. F. Wong, Jonathan R. Gair, W. Kastaun, H. Qi, Lili Yang, Fabrizio Bobba, Stephan Grimm, B. C. Pant, C. Messick, M. Bitossi, Viola Sordini, G. Dálya, Rana X. Adhikari, M. Branchesi, Bruno Giacomazzo, D. M. Wilken, Om Sharan Salafia, Riccardo Buscicchio, F. Magaña-Sandoval, J. Neilson, D. J. McManus, C. Gier, N. Koper, K. Wette, R. P. Fisher, S. Mitra, John J. Oh, M. Standke, Otto A. Hannuksela, Sourav Ghosh, Albino Perego, F. Donovan, Imre Bartos, D. Y. T. Pong, E. Massera, Y. Asali, Carlos O. Lousto, B. Idzkowski, V. Loriette, V. Skliris, R. D. Rodriguez-Soto, Doğa Veske, J. P. Zendri, Edward Seidel, A. Viceré, F. Marion, N. 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M., Martinez, V., Martynov, D. V., Masalehdan, H., Mason, K., Massera, E., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matas, A., Matichard, F., Mavalvala, N., Maynard, E., Mccann, J. J., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcculler, L., Mcguire, S. C., Mcisaac, C., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meacher, D., Meadors, G. D., Mehmet, M., Mehta, A. K., Mejuto Villa, E., Melatos, A., Mendell, G., Mercer, R. A., Mereni, L., Merfeld, K., Merilh, E. L., Merritt, J. D., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. M., Meylahn, F., Mhaske, A., Miani, A., Miao, H., Michaloliakos, I., Michel, C., Middleton, H., Milano, L., Miller, A. L., Millhouse, M., Mills, J. C., Milotti, E., Milovich-Goff, M. C., Minazzoli, O., Minenkov, Y., Mishkin, A., Mishra, C., Mistry, T., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Mo, G., Mogushi, K., Mohapatra, S. R. P., Mohite, S. R., Molina-Ruiz, M., Mondin, M., Montani, M., Moore, C. J., Moraru, D., Morawski, F., Moreno, G., Morisaki, S., Mours, B., Mow-Lowry, C. M., Mozzon, S., Muciaccia, F., Mukherjee, A., Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Muniz, E. A., Murray, P. G., Nagar, A., Nardecchia, I., Naticchioni, L., Nayak, R. K., Neil, B. F., Neilson, J., Nelemans, G., Nelson, T. J. N., Nery, M., Neunzert, A., Ng, K. Y., Ng, S., Nguyen, C., Nguyen, P., Nichols, D., Nichols, S. A., Nissanke, S., Nitz, A., Nocera, F., Noh, M., North, C., Nothard, D., Nuttall, L. K., Oberling, J., O'Brien, B. D., Oganesyan, G., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Ohta, H., Okada, M. A., Oliver, M., Olivetto, C., Oppermann, P., Oram, R. J., O'Reilly, B., Ormiston, R. G., Ortega, L. F., O'Shaughnessy, R., Ossokine, S., Osthelder, C., Ottaway, D. J., Overmier, H., Owen, B. J., Pace, A. E., Pagano, G., Page, M. A., Pagliaroli, G., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pan, H., Panda, P. K., Pang, P. T. H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Parida, A., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Payne, E., Pearlstone, B. L., Pechsiri, T. C., Pedersen, A. J., Pedraza, M., Pele, A., Penn, S., Perego, A., Perez, C. J., Perigois, C., Perreca, A., Perries, S., Petermann, J., Pfeiffer, H. P., Phelps, M., Phukon, K. S., Piccinni, O. J., Pichot, M., Piendibene, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Piotrzkowski, K., Pirello, M., Pitkin, M., Plastino, W., Poggiani, R., Pong, D. Y. T., Ponrathnam, S., Popolizio, P., Porter, E. K., Powell, J., Prajapati, A. K., Prasai, K., Prasanna, R., Pratten, G., Prestegard, T., Principe, M., Prodi, G. A., Prokhorov, L., Punturo, M., Puppo, P., Purrer, M., Qi, H., Quetschke, V., Quinonez, P. J., Raab, F. 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K., Srivastava, V., Staats, K., Stachie, C., Standke, M., Steer, D. A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stevenson, S., Stocks, D., Stops, D. J., Stover, M., Strain, K. A., Stratta, G., Strunk, A., Sturani, R., Stuver, A. L., Sudhagar, S., Sudhir, V., Summerscales, T. Z., Sun, L., Sunil, S., Sur, A., Suresh, J., Sutton, P. J., Swinkels, B. L., Szczepanczyk, M. J., Tacca, M., Tait, S. C., Talbot, C., Tanasijczuk, A. J., Tanner, D. B., Tao, D., Tapai, M., Tapia, A., Tapia San Martin, E. N., Tasson, J. D., Taylor, R., Tenorio, R., Terkowski, L., Thirugnanasambandam, M. P., Thomas, M., Thomas, P., Thompson, J. E., Thondapu, S. R., Thorne, K. A., Thrane, E., Tinsman, C. L., Saravanan, T. R., Tiwari, S., Tiwari, V., Toland, K., Tonelli, M., Tornasi, Z., Torres-Forne, A., Torrie, C. I., Tosta E Melo, I., Toyra, D., Travasso, F., Traylor, G., Tringali, M. C., Tripathee, A., Trovato, A., Trudeau, R. J., Tsang, K. W., Tse, M., Tso, R., Tsukada, L., Tsuna, D., Tsutsui, T., Turconi, M., Ubhi, A. S., Udall, R., Ueno, K., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Utina, A. C., Vahlbruch, H., Vajente, G., Valdes, G., Valentini, M., Van Bakel, N., Van Beuzekom, M., Van Den Brand, J. F. J., Van Den Broeck, C., Vander-Hyde, D. C., Van Der Schaaf, L., Van Heijningen, J. V., Van Veggel, A. A., Vardaro, M., Varma, V., Vass, S., Vasuth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Venugopalan, G., Verkindt, D., Veske, D., Vetrano, F., Vicere, A., Viets, A. D., Vinciguerra, S., Vine, D. J., Vinet, J. -Y., Vitale, S., Vivanco, F. H., Vo, T., Vocca, H., Vorvick, C., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walet, R., Walker, M., Wallace, G. S., Wallace, L., Walsh, S., Wang, J. Z., Wang, S., Wang, W. H., Ward, R. L., Warden, Z. A., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L. -W., Weinert, M., Weinstein, A. J., Weiss, R., Wellmann, F., Wen, L., Wessels, P., Westhouse, J. W., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Wilken, D. M., Williams, D., Willis, J. L., Willke, B., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Wofford, J. K., Wong, I. C. F., Wright, J. L., Wu, D. S., Wysocki, D. M., Xiao, L., Yamamoto, H., Yang, L., Yang, Y., Yang, Z., Yap, M. J., Yazback, M., Yeeles, D. W., Yu, H., Yuen, S. H. R., Zadrozny, A. K., Zadrozny, A., Zanolin, M., Zelenova, T., Zendri, J. -P., Zevin, M., Zhang, J., Zhang, L., Zhang, T., Zhao, C., Zhao, G., Zhou, M., Zhou, Z., Zhu, X. J., Zimmerman, A. B., Zucker, M. E., Zweizig, J., Arène, M., Bécsy, B., Calderón Bustillo, J., Castañeda, J., Cavaglià, M., Cerdá-Durán, P., Cieślar, M., Cordero-Carrión, I., Canton, T. Dal, Dálya, G., D’Angelo, B., D’Antonio, S., Deléglise, S., D’Emilio, V., de Varona, O., Díaz, M. C., D’Urso, D., Fronzè, G., García-Quirós, C., Ghosh, Abhirup, Ghosh, Archisman, González, G., Guixé, G., Gupta, Anchal, Hübner, M. T., Johnson-McDaniel, N. K., Kéfélian, F., Kim, Chunglee, Królak, A., Kumar, Rahul, Kumar, Rakesh, Lück, H., Magaña Hernandez, I., Magaña-Sandoval, F., Márka, S., Márka, Z., Mukherjee, Arunava, Mukherjee, Subroto, Muñiz, E. A., O’Brien, B. D., Oram, Richard J., O’Reilly, B., O’Shaughnessy, R., Périgois, C., Perriès, S., Pürrer, M., Rana, Javed, Rosińska, D., Roy, Santosh, Roy, Soumen, Schönbeck, A., Szczepańczyk, M. J., Tápai, M., Tiwari, Shubhanshu, Torres-Forné, A., Tosta e Melo, I., Töyrä, D., van Bakel, N., van Beuzekom, M., van den Brand, J. F. J., van der Schaaf, L., van Veggel, A. A., Vasúth, M., Viceré, A., Vivanco, Francisco Hernandez, Weßels, P., Yu, Hang, Yu, Haocun, Zadrożny, A. 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Cohadon, P, Cohen, D, Colleoni, M, Collette, C, Collins, C, Colpi, M, Constancio, M, Conti, L, Cooper, S, Corban, P, Corbitt, T, Cordero-Carrion, I, Corezzi, S, Corley, K, Cornish, N, Corre, D, Corsi, A, Cortese, S, Costa, C, Cotesta, R, Coughlin, M, Coughlin, S, Coulon, J, Countryman, S, Couvares, P, Covas, P, Coward, D, Cowart, M, Coyne, D, Coyne, R, Creighton, J, Creighton, T, Cripe, J, Croquette, M, Crowder, S, Cudell, J, Cullen, T, Cumming, A, Cummings, R, Cunningham, L, Cuoco, E, Curylo, M, Canton, T, Dalya, G, Dana, A, Daneshgaran-Bajastani, L, D'Angelo, B, Danilishin, S, D'Antonio, S, Danzmann, K, Darsow-Fromm, C, Dasgupta, A, Datrier, L, Dattilo, V, Dave, I, Davier, M, Davies, G, Davis, D, Daw, E, Debra, D, Deenadayalan, M, Degallaix, J, De Laurentis, M, Deleglise, S, Delfavero, M, De Lillo, N, Del Pozzo, W, Demarchi, L, D'Emilio, V, Demos, N, Dent, T, De Pietri, R, De Rosa, R, De Rossi, C, Desalvo, R, de Varona, O, Dhurandhar, S, Diaz, M, Diaz-Ortiz, M, Dietrich, T, Di Fiore, L, Di Fronzo, C, Di Giorgio, C, Di Giovanni, F, Di Giovanni, M, Di Girolamo, T, Di Lieto, A, Ding, B, Di Pace, S, Di Palma, I, Di Renzo, F, Divakarla, A, Dmitriev, A, Doctor, Z, Donovan, F, Dooley, K, Doravari, S, Dorrington, I, Downes, T, Drago, M, Driggers, J, Du, Z, Ducoin, J, Dupej, P, Durante, O, D'Urso, D, Dwyer, S, Easter, P, Eddolls, G, Edelman, B, Edo, T, Edy, O, Effler, A, Ehrens, P, Eichholz, J, Eikenberry, S, Eisenmann, M, Eisenstein, R, Ejlli, A, Errico, L, Essick, R, Estelles, H, Estevez, D, Etienne, Z, Etzel, T, Evans, M, Evans, T, Ewing, B, Fafone, V, Fairhurst, S, Fan, X, Farinon, S, Farr, B, Farr, W, Fauchon-Jones, E, Favata, M, Fays, M, Fazio, M, Feicht, J, Fejer, M, Feng, F, Fenyvesi, E, Ferguson, D, Fernandez-Galiana, A, Ferrante, I, Ferreira, E, Ferreira, T, Fidecaro, F, Fiori, I, Fiorucci, D, Fishbach, M, Fisher, R, Fittipaldi, R, Fitz-Axen, M, Fiumara, V, Flaminio, R, Floden, E, Flynn, E, Fong, H, Font, J, Forsyth, P, Fournier, J, Frasca, S, Frasconi, F, Frei, 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Prodi, G, Prokhorov, L, Punturo, M, Puppo, P, Purrer, M, Qi, H, Quetschke, V, Quinonez, P, Raab, F, Raaijmakers, G, Radkins, H, Radulesco, N, Raffai, P, Rafferty, H, Raja, S, Rajan, C, Rajbhandari, B, Rakhmanov, M, Ramirez, K, Ramos-Buades, A, Rana, J, Rao, K, Rapagnani, P, Raymond, V, Razzano, M, Read, J, Regimbau, T, Rei, L, Reid, S, Reitze, D, Rettegno, P, Ricci, F, Richardson, C, Richardson, J, Ricker, P, Riemenschneider, G, Riles, K, Rizzo, M, Robertson, N, Robinet, F, Rocchi, A, Rodriguez-Soto, R, Rolland, L, Rollins, J, Roma, V, Romanelli, M, Romano, R, Romel, C, Romero-Shaw, I, Romie, J, Rose, C, Rose, D, Rose, K, Rosinska, D, Rosofsky, S, Ross, M, Rowan, S, Rowlinson, S, Roy, P, Roy, S, Ruggi, P, Rutins, G, Ryan, K, Sachdev, S, Sadecki, T, Sakellariadou, M, Salafia, O, Salconi, L, Saleem, M, Salemi, F, Samajdar, A, Sanchez, E, Sanchez, L, Sanchis-Gual, N, Sanders, J, Santiago, K, Santos, E, Sarin, N, Sassolas, B, Sathyaprakash, B, Sauter, O, Savage, R, Savant, V, Sawant, D, Sayah, S, Schaetzl, D, Schale, P, Scheel, M, Scheuer, J, Schmidt, P, Schnabel, R, Schofield, R, Schonbeck, A, Schreiber, E, Schulte, B, Schutz, B, Schwarm, O, Schwartz, E, Scott, J, Scott, S, Seidel, E, Sellers, D, Sengupta, A, Sennett, N, Sentenac, D, Sequino, V, Sergeev, A, Setyawati, Y, Shaddock, D, Shaffer, T, Sharifi, S, Shahriar, M, Sharma, A, Sharma, P, Shawhan, P, Shen, H, Shikauchi, M, Shink, R, Shoemaker, D, Shukla, K, Shyamsundar, S, Siellez, K, Sieniawska, M, Sigg, D, Singer, L, Singh, D, Singh, N, Singha, A, Singhal, A, Sintes, A, Sipala, V, Skliris, V, Slagmolen, B, Slaven-Blair, T, Smetana, J, Smith, J, Smith, R, Somala, S, Son, E, Soni, S, Sorazu, B, Sordini, V, Sorrentino, F, Souradeep, T, Sowell, E, Spencer, A, Spera, M, Srivastava, A, Srivastava, V, Staats, K, Stachie, C, Standke, M, Steer, D, Steinke, M, Steinlechner, J, Steinlechner, S, Steinmeyer, D, Stevenson, S, Stocks, D, Stops, D, Stover, M, Strain, K, Stratta, G, Strunk, A, Sturani, R, Stuver, A, Sudhagar, S, Sudhir, V, Summerscales, T, Sun, L, Sunil, S, Sur, A, Suresh, J, Sutton, P, Swinkels, B, Szczepanczyk, M, Tacca, M, Tait, S, Talbot, C, Tanasijczuk, A, Tanner, D, Tao, D, Tapai, M, Tapia, A, Tapia San Martin, E, Tasson, J, Taylor, R, Tenorio, R, Terkowski, L, Thirugnanasambandam, M, Thomas, M, Thomas, P, Thompson, J, Thondapu, S, Thorne, K, Thrane, E, Tinsman, C, Saravanan, T, Tiwari, S, Tiwari, V, Toland, K, Tonelli, M, Tornasi, Z, Torres-Forne, A, Torrie, C, Tosta E Melo, I, Toyra, D, Travasso, F, Traylor, G, Tringali, M, Tripathee, A, Trovato, A, Trudeau, R, Tsang, K, Tse, M, Tso, R, Tsukada, L, Tsuna, D, Tsutsui, T, Turconi, M, Ubhi, A, Udall, R, Ueno, K, Ugolini, D, Unnikrishnan, C, Urban, A, Usman, S, Utina, A, Vahlbruch, H, Vajente, G, Valdes, G, Valentini, M, van Bakel, N, van Beuzekom, M, van den Brand, J, Van Den Broeck, C, Vander-Hyde, D, van der Schaaf, L, Van Heijningen, J, van Veggel, A, Vardaro, M, Varma, V, Vass, S, Vasuth, M, Vecchio, A, Vedovato, G, Veitch, J, Veitch, P, Venkateswara, K, Venugopalan, G, Verkindt, D, Veske, D, Vetrano, F, Vicere, A, Viets, A, Vinciguerra, S, Vine, D, Vinet, J, Vitale, S, Vivanco, F, Vo, T, Vocca, H, Vorvick, C, Vyatchanin, S, Wade, A, Wade, L, Wade, M, Walet, R, Walker, M, Wallace, G, Wallace, L, Walsh, S, Wang, J, Wang, S, Wang, W, Ward, R, Warden, Z, Warner, J, Was, M, Watchi, J, Weaver, B, Wei, L, Weinert, M, Weinstein, A, Weiss, R, Wellmann, F, Wen, L, Wessels, P, Westhouse, J, Wette, K, Whelan, J, Whiting, B, Whittle, C, Wilken, D, Williams, D, Willis, J, Willke, B, Winkler, W, Wipf, C, Wittel, H, Woan, G, Woehler, J, Wofford, J, Wong, I, Wright, J, Wu, D, Wysocki, D, Xiao, L, Yamamoto, H, Yang, L, Yang, Y, Yang, Z, Yap, M, Yazback, M, Yeeles, D, Yu, H, Yuen, S, Zadrozny, A, Zanolin, M, Zelenova, T, Zendri, J, Zevin, M, Zhang, J, Zhang, L, Zhang, T, Zhao, C, Zhao, G, Zhou, M, Zhou, Z, Zhu, X, Zimmerman, A, Zucker, M, Zweizig, J, The LIGO Scientific Collaboration, The Virgo Collaboration, 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), 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), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut des Hautes Études Scientifiques (IHES), National Science Foundation (US), Science and Technology Facilities Council (UK), Agencia Estatal de Investigación (España), Generalitat de Catalunya, Govern de les Illes Balears, Generalitat Valenciana, European Commission, IoP (FNWI), Faculty of Science, Gravitation and Astroparticle Physics Amsterdam, Other Research IHEF (IoP, FNWI), Astroparticle Physics (IHEF, IoP, FNWI), and (Astro)-Particles Physics
Subjects: Astronomy, General Physics and Astronomy, detector: network, Astrophysics, Gravitational waves, Binary black holes, Intermediate mass black holes, 01 natural sciences, General Relativity and Quantum Cosmology, gravitational waves, black holes, GW190521, BBH, Intermediate mass black holes, LIGO, 10. No inequality, QC, QB, Settore FIS/01, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, PAIR-INSTABILITY, Settore FIS/05, statistical analysis: Bayesian, Supernova, Physical Sciences, Physique des particules élémentaires, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics - High Energy Astrophysical Phenomena, Gravitational wave, data analysis method, gr-qc, Physics, Multidisciplinary, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Physics and Astronomy(all), Gravitation and Astrophysics, pair-instability, Settore FIS/05 - Astronomia e Astrofisica, Binary black hole, Binary black holes, Neutron stars,gravitational waves, supernova, 0103 physical sciences, 010306 general physics, Luminosity distance, STFC, GW190521, Science & Technology, 9. Industry and infrastructure, gravitational radiation, RCUK, black hole: mass, gravitational waves, black hole, gravitational radiation detector, Redshift, Black hole, wave: model, VIRGO, black hole: binary, Intermediate-mass black hole, gravitational radiation: emission, BBH, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: LIGO Scientific Collaboration and Virgo Collaboration: et al., On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated false-alarm rate of 1 in 4900 yr using a search sensitive to generic transients. If GW190521 is from a quasicircular binary inspiral, then the detected signal is consistent with the merger of two black holes with masses of 85+21−14M⊙ and 66+17−18M⊙ (90% credible intervals). We infer that the primary black hole mass lies within the gap produced by (pulsational) pair-instability supernova processes, with only a 0.32% probability of being below 65M⊙. We calculate the mass of the remnant to be 142+28−16M⊙, which can be considered an intermediate mass black hole (IMBH). The luminosity distance of the source is 5.3+2.4−2.6Gpc corresponding to a redshift of 0.82+0.28−0.34. The inferred rate of mergers similar to GW190521 is 0.13+0.30−0.11Gpc−3yr−1., The authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigación, the Vicepresidencia i Conselleria d’Innovació, Recerca i Turisme and the Conselleria d’Educació i Universitat del Govern de les Illes Balears, the Conselleria d’Innovació, Universitats, Ciencia i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland, the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertees (ARC) and Fonds Wetenschappelijk Onderzoek–Vlaanderen (FWO), Belgium, the Paris Île-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and Communications, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTPSAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authorsgratefully acknowledge the support of the NSF, STFC, INFN and CNRS for provision of computational resources.
Published: 2020
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13. Neutrino emission upper limits with maximum likelihood estimators for joint astrophysical neutrino searches with large sky localizations

Author: Doğa Veske, Imre Bartos, Szabolcs Márka, and Zsuzsa Márka
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Gravitational wave, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Estimator, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Upper and lower bounds, Neutrino detector, Sky, 0103 physical sciences, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Event (particle physics), Joint (geology), media_common
Abstract: Since the start of the gravitational wave observation era, no joint high energy neutrino and gravitational wave event has been found. These non-detections could be used for setting an upper bound on the neutrino emission properties for gravitational wave events individually or for a set of them. Although in the previous joint high energy neutrino and gravitational wave event searches upper limits have been found, there is a lack of consistent method for the calculation. The problem addressed in this paper is finding those limits for astrophysical events which are localized poorly in the sky where the sensitivities of the neutrino detectors change significantly and can also emit neutrinos, for example the gravitational wave detections. Here we describe methods for assigning limits for expected neutrino count, emission fluence and isotropically equivalent emission based on maximum likelihood estimators. Then we apply described methods on the three GW detections from aLIGO's first observing run (O1) and find upper limits for them., Comment: 15 pages, 2 figures
Published: 2020
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14. Search for Black Hole Merger Families

Author: Szabolcs Márka, K. Rainer Corley, Johan Samsing, Doğa Veske, Imre Bartos, Zsuzsa Márka, Andrew G. Sullivan, Riccardo Buscicchio, Veske, D, Sullivan, A, Marka, Z, Bartos, I, Corley, K, Samsing, J, Buscicchio, R, and Marka, S
Subjects: 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Binary number, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, Gravitational-wave astronomy, General Relativity and Quantum Cosmology, Gravitational wave astronomy (675), Binary black hole, 0103 physical sciences, Unified Astronomy Thesaurus concepts: Astrophysical black holes (98), 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Gravitational wave sources, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Mass distribution, Spins, Astrophysical black holes, Astronomy and Astrophysics, LIGO, First generation, Gravitational wave sources (677), Black hole, Space and Planetary Science, Gravitational wave astronomy, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The origin, environment, and evolution of stellar-mass black hole binaries are still a mystery. One of the proposed binary formation mechanisms is manifest in dynamical interactions between multiple black holes. A resulting framework of these dynamical interactions is the so-called hierarchical triple merger scenario, which happens when three black holes become gravitationally bound, causing two successive black hole mergers to occur. In such successive mergers, the black holes involved are directly related to each other, and hence this channel can be directly tested from the properties of the detected binary black hole mergers. Here we present a search for hierarchical triple mergers among events within the GWTC-1 and GWTC-2 catalogs of LIGO/Virgo, the eccentric localization of GW190521 and those found by the IAS-Princeton group. The search includes improved statistical quantification that also accounts for black hole spins. We perform our analysis for different upper bounds on the mass distribution of first generation BHs. Our results demonstrate the importance of the mass distributions' properties for constraining the hierarchical merger scenario. We present the individually significant merger pairs. The search yields interesting candidate families and hints of its future impact., Comment: 4 figures, 7 pages without references
Published: 2020
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15. GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

Author: T. D. Abbott, A. Królak, E. A. Muñiz, M. C. Heintze, Benno Willke, L. Rei, L. McCuller, X. Liu, T. B. Littenberg, B. D'Angelo, B. Edelman, V. Gayathri, S. Di Pace, S. Walsh, Miriam Cabero, Alessandra Buonanno, R. Metzdorff, Gabrielle Allen, C. J. Moore, A. S. Sengupta, M. J. Yap, S. H. R. Yuen, O. de Varona, M. Fishbach, R. Benkel, P. Fulda, Antoine Heidmann, E. A. Chase, M. Bejger, S. Morisaki, F. Marion, K. Toland, R. Tenorio, N. A. Holland, J. B. Camp, R. Macas, D. Estevez, M. Gosselin, Y. K. Lecoeuche, F. Clara, R. G. Ormiston, R. Taylor, Y. Ma, D. Schaetzl, M. Phelps, N. Gohlke, G. Valdes, S. E. Dwyer, J. Blackman, M. Haney, Archisman Ghosh, Patrick Brady, T. J. Cullen, D. J. Vine, R. Passaquieti, C. Wong, Fabien Kéfélian, J. H. Hough, N. Kijbunchoo, S. R. Thondapu, R. Chierici, A. Grimaldi, O. Durante, F. Meylahn, B. B. Lane, Carl-Johan Haster, C. Kimball, L. Rolland, Jade Powell, D. Mukherjee, D. J. Stops, V. Mangano, Fabrizio Barone, M. T. Hübner, N. Man, F. J. Hayes, T. Dal Canton, H. K. Gulati, I. Magaña Hernandez, C. McIsaac, N. De Lillo, S. Banagiri, Sascha Husa, J. Li, A. K. Zadrożny, H. Estelles, S. Galaudage, A. M. Baer, P. Leaci, F. Feng, K. R. Corley, D. J. McManus, X. Li, H. Fong, Nergis Mavalvala, Jerome Degallaix, A. Mullavey, D. Steinmeyer, C. Casentini, S. Anand, G. D. Hammond, Javed Rana, Stefan Grimm, V. Kondrashov, O. A. Hannuksela, B. F. Neil, P. Weßels, J. A. Clark, M. Di Giovanni, A. W. Jones, R. M. Martin, A. Ananyeva, R. De Pietri, N. Letendre, Nikhil Sarin, H. Qi, J. Calderón Bustillo, D. Lumaca, M. Walker, P. J. Veitch, David A. Williams, I. W. Harry, Z. A. Warden, O. Palashov, Rocco Romano, M. Kinley-Hanlon, S. G. Crowder, Jinsook Kim, D. C. Coyne, K. Mason, C. J. Perez, C. K. Cheong, M. Vasúth, Xin Chen, David A. Nichols, M. Mondin, S. Karki, Sean T. McWilliams, F. Piergiovanni, J. C. Mills, A. Di Lieto, M. Saleem, Chang-Hwan Lee, D. E. Cohen, A. M. Holgado, K. G. Arun, D. M. Wilken, F. Aubin, G. Stratta, Jesper Munch, S. Grunewald, T. Vo, F. Wellmann, T. Zhang, K. Merfeld, Thibaut Jacqmin, P. Kumar, R. D. Rodriguez-Soto, Doğa Veske, J. Feicht, C. Messick, M. Delfavero, G. Pagliaroli, A. K. Y. Li, Jonathan Cripe, M. De Laurentis, M. Fitz-Axen, A. Mhaske, R. Bork, M. Sakellariadou, Daniel E. Holz, M. Rizzo, A. Viceré, Yi Chen, B. W. Schulte, T. Mistry, G. Pratten, F. Vetrano, J. R. Smith, R. L. Savage, S. Khan, A. L. Stuver, G. Pillant, B. Patricelli, D. S. Wu, Margaret Millhouse, M. Davier, W. Parker, M. Favata, A. Basti, Ryan N. Lang, M. Fazio, K. Holt, A. S. Ubhi, N. Demos, Francisco Hernandez Vivanco, T. Prestegard, P. J. Easter, L. M. DeMarchi, Chunglee Kim, O. J. Piccinni, A. Cirone, A. A. van Veggel, D. Barta, V. Bossilkov, H. Cao, P. Raffai, Francesco Pannarale, D. Meacher, A. Rocchi, S. Raja, Olivier Minazzoli, Eyal Schwartz, B. Goncharov, M. Razzano, B. Grace, E. Genin, S. M. Aronson, S. McCormick, Aldo Ejlli, Z. Yang, F. Bergamin, N. Mukund, D. Tsuna, Roger Jones, J.-D. Fournier, Eric Thrane, X. Fan, C. Michel, M. Kasprzack, Sarah Caudill, P. Hopkins, Francesco Chiadini, P. Charlton, F. Badaracco, J. G. Rollins, R. M. Magee, Haixing Miao, J. W. Westhouse, H. Ohta, F. Di Giovanni, J. Lee, K. L. Dooley, Aaron Zimmerman, D. Nothard, P. Barneo, N. Singh, Samuele Cortese, Haocun Yu, E. Z. Hamilton, Lisa Barsotti, A. P. Spencer, K. Chakravarti, D. D. Brown, E. Biggs, K. Barkett, R. S. Bankar, S. S. Eikenberry, Marica Valentini, T. Di Girolamo, D. H. Reitze, Y. Setyawati, Vicky Kalogera, O. Halim, M. Tonelli, G. González, J. H. Briggs, M. M. Fejer, Guoying Zhao, I. Cordero-Carrión, H. M. Lee, M. C. Milovich-Goff, Anthony A. Amato, N. van Bakel, E. C. Ferreira, R. K. Lanza, J. D. Merritt, A. Masserot, F. Y. Khalili, J. Zweizig, K. Kawabe, Karan Jani, R. Shink, Gijs Nelemans, F. Nocera, E. D. Hall, Jolien D. E. Creighton, P. Booker, R. Bhandare, A. Bisht, V. Kringel, W. Kastaun, L. Yang, B. C. Pant, K. Ueno, Maximiliano Isi, C. G. Hoy, N. N. Janthalur, E. M. Gretarsson, Ying Guo, Peter Fritschel, P. Godwin, G. Oganesyan, T. A. Callister, Maria Ilaria Del Principe, K. W. Tsang, K. Siellez, J. H. Romie, I. Ferrante, Nicolas Sanchis-Gual, D. Huet, B. D. Lackey, B. L. Swinkels, Z. Frei, T. R. Corbitt, P. Grassia, E. J. Daw, M. Punturo, P. H. Nguyen, S. G. Rosofsky, W. M. Farr, Sebastian Steinlechner, C. A. Rose, C. J. Richardson, M. Agathos, V. Martinez, Soumen Roy, G. Greco, E. Floden, Gianpietro Cagnoli, Andrew Lundgren, W. S. Kim, J. Baird, Rana X. Adhikari, T. Tsutsui, F. Donovan, K. Y. Ng, Stephane Perries, A. Balsamo, S. Khadka, C. I. Torrie, Jan Harms, V. Dattilo, H. S. Cho, G. Moreno, A. Effler, R. DeSalvo, J. Petermann, H. Wittel, J. J. Oh, L. E. Sanchez, J. C. Barayoga, R. Cavalieri, J. Bosveld, Z. Zhou, K. Haughian, Antonio Marquina, Edoardo Milotti, E. Lalande, H. Radkins, S. M. Aston, B. Idzkowski, M. Canepa, T. A. Ferreira, E. M. Santos, W. Z. Korth, O. Schwarm, Geoffrey Lovelace, Satyanarayan Ray Pitambar Mohapatra, P. Rettegno, F. Baldaccini, A. Allocca, M. Nery, A. K. Srivastava, Enrico Calloni, V. Sordini, L. Salconi, D. V. Martynov, R. Goetz, G. S. Wallace, A. Singha, M. Croquette, G. Vedovato, Z. Doctor, J. Gniesmer, R. M. S. Schofield, M. Curylo, J. Jiang, S. Marsat, V. Hui, M. Drago, M. Cho, M. A. Page, Richard J. Oram, Samuel Deléglise, R. Huxford, K. Shukla, E. A. Trail, B. A. Boom, D. Sigg, P. Puppo, F. Cleva, C. Vorvick, J. Bartlett, P. W. F. Forsyth, M. Khursheed, F. Brighenti, Aniello Grado, Andrew Melatos, M. Lorenzini, S. Chung, Ellen S. Howell, I. A. Bilenko, L. Haegel, T. B. Edo, A. Sharma, M. G. Benjamin, Parthanil Roy, F. Linde, Laura Cadonati, M. Zanolin, A. Perreca, S. D. Linker, J. C. Driggers, M. Zevin, S. M. Gaebel, S. R. Mohite, V. D'Emilio, R. Sturani, G. Riemenschneider, K. AultONeal, G. Venugopalan, I. Belahcene, David Keitel, Benjamin J. Owen, D. M. Wysocki, Andrew Mehta, J. F. J. van den Brand, I. A. O. MacMillan, S. Meshkov, N. Krupinski, J. S. Lange, B. E. Ewing, P. A. Altin, M. Stover, S. Miller, E. A. Huerta, K. Prasai, L. Cunningham, B. C. Barish, B. Sassolas, Yang Yang, F. Ohme, Xing-Jiang Zhu, M. Rakhmanov, V. Sipala, L. Naticchioni, R. P. Fisher, Nathan K. Johnson-McDaniel, S. P. Vyatchanin, I. Khan, T. Dietrich, V. B. Adya, Tristan Briant, Chad Hanna, V. Tiwari, G. Carullo, C. Pankow, P. M. Meyers, J. Neilson, D. George, David J. Ottaway, A. Ain, L. Sun, M. Tápai, C. L. Romel, Fiodor Sorrentino, Y. Boetzel, Mark Hannam, Binlei Ding, A. Gupta, A. Lartaux-Vollard, M. Pürrer, O. D. Aguiar, M. Tacca, P. Ehrens, Wolfango Plastino, Seog Oh, A. Cumming, M. Laxen, Martin Hendry, Cecilio García-Quirós, M. C. Díaz, K. Chatziioannou, F. Di Renzo, Suvadeep Bose, T. R. Saravanan, D. Rose, F. Garufi, R. Jaume, R. A. Eisenstein, B. J. J. Slagmolen, C. Di Giorgio, S. Caride, R. Gouaty, J. Hanks, S. E. Gossan, Carlos O. Lousto, H. Masalehdan, Salvatore Vitale, J. Zhang, L. F. Ortega, V. Srivastava, A. Strunk, M. Oliver, Surendra Nadh Somala, M. Fyffe, D. Bersanetti, C. North, R. Schnabel, Thomas Dent, P. Corban, S. J. Cooper, G. H. Ogin, James Whelan, H. Pan, D. Buskulic, A. V. Bhandari, C. Zhao, Alicia M. Sintes, R. Kashyap, Jishnu Suresh, B. L. Pearlstone, R. Fittipaldi, G. D. Meadors, S. W. Ballmer, J. Z. Wang, T. Souradeep, T. Hardwick, Junwei Cao, A. A. Ciobanu, John Veitch, J. Lehmann, B. Rajbhandari, P. Ajith, L. Zhang, T. Zelenova, C. De Rossi, C. Périgois, C. Whittle, M. Masso-Reid, Sheelu Abraham, E. Chassande-Mottin, S. A. Usman, D. Singh, M. Manske, R. A. Mercer, Zhihui Du, G. Ciani, G. Gemme, T. D. Creighton, P. Jones, Leopoldo Milano, M. P. Ross, A. Parida, A. E. Pace, T. M. Evans, A. Bozzi, Sheila Rowan, S. Sunil, Giovanni Carapella, A. Corsi, M. Colleoni, A. Dasgupta, A. K. Prajapati, A. R. Wade, Rosa Poggiani, C. M. Mow-Lowry, A. Markowitz, J. A. Giaime, S. Soni, S. Farinon, E. Mejuto Villa, A. Lazzarini, F. Carbognani, C. Gray, T. Z. Summerscales, K. A. Thorne, S. Antier, M. Chan, E. Katsavounidis, S. J. Jadhav, S. C. Tait, R. Flaminio, J.-P. Coulon, S. H. Huttner, N. Arnaud, R. K. L. Lo, V. Sequino, C. Affeldt, J. D. Lough, J. Casanueva Diaz, S. B. Coughlin, M. MacInnis, E. Cesarini, P. Rapagnani, Colm Talbot, M. Colpi, R. Birney, Andreas Freise, Paul D. Lasky, Z. Márka, W. H. Wang, F. Travasso, R. L. Byer, C. Van Den Broeck, Y.-J. Huang, E. Sowell, G. Vajente, D. M. Macleod, Piotr Jaranowski, M. Llorens-Monteagudo, Soma Mukherjee, J. R. Sanders, A. Aich, A. Gopakumar, David Coward, A. Miani, J. Castañeda, T. J. Hansen, P. Brockill, S. Sayah, V. V. Frolov, Tania Regimbau, A. J. Tanasijczuk, Sebastien Clesse, N. Bode, A. Macquet, Matthew Pitkin, T. Sadecki, J. M. Isac, M. C. Araya, H. S. Chen, T. G. F. Li, Michela Mapelli, C. Collins, S. Mastrogiovanni, S. Y. Hoback, N. Radulesco, L.-W. Wei, Shao-Jiang Wang, R. Bonnand, Zachariah B. Etienne, L. Kuo, Jennifer Watchi, S. A. Pai, H. Shen, Fausto Acernese, F. 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Pinard, C. Di Fronzo, L. Kleybolte, L. Mereni, Patrick M. Koch, F. Ricci, Hang Yu, G. Bogaert, V. Savant, A. Pasqualetti, F. Martelli, Cesare Barbieri, Walter Winkler, M. Montani, M. Weinert, S. Ossokine, A. J. Weinstein, Surabhi Sachdev, R. Cotesta, M. Steinke, J. V. Van Heijningen, Harald Lück, E. Knyazev, D. Verkindt, Nancy Aggarwal, Zahoor Ali Khan, S. Koley, O. S. Salafia, D. Jariwala, I. La Rosa, Jean-René Cudell, S. Vass, J. Healy, A. Torres-Forné, A. Singhal, G. Kang, A. F. Brooks, P. B. Covas, T. D. Knowles, David Blair, M. W. Coughlin, K. Haris, T. Huynh-Dinh, Y. Levin, I. Maksimovic, R. L. Ward, G. Hemming, Bernard F. Whiting, M. Pichot, C. Palomba, G. J. Kim, K. Rose, G. Raaijmakers, A. Gennai, J. L. Willis, Christopher P. L. Berry, T. Harder, E. K. Porter, A. J. Pedersen, Marco Cavaglia, Matthew Evans, C. C. Wipf, Sushanta K. Mitra, Stanislav Babak, A. Bramley, M. Merzougui, M. Shikauchi, R. C. Essick, C. Stachie, Subroto Mukherjee, Jürgen Heinze, Vivien Raymond, P. J. 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Töyrä, O. Sauter, M. Arène, B. U. Gadre, D. Sentenac, M. Bawaj, Rajesh Kumar, H. Vahlbruch, H. Middleton, A. Tapia, D. Sellers, F. Fidecaro, J. D. Bentley, T. J. N. Nelson, G. Mo, P. Aufmuth, H. L. Griggs, J. E. Brau, Efim A. Khazanov, G. Ballardin, Mark A. Scheel, J. Liu, B. R. Iyer, G. Billingsley, S. M. Koehlenbeck, M. J. Szczepańczyk, Marco Bazzan, C. Ingram, G. Bergmann, K. W. Chung, Angela Delli Paoli, E. L. Merilh, S. Ascenzi, M. E. Zucker, C. Austin, Alessandro Bertolini, R. P. Udall, Azadeh Keivani, A. R. Guimaraes, S. Klimenko, J.-G. Ducoin, John George, I. M. Pinto, M. Vardaro, R. C. Walet, V. P. Mitrofanov, M. Diaz-Ortiz, W. Del Pozzo, P. F. Cohadon, A. L. Urban, C. Chan, A. Matas, H. Heitmann, D. Sawant, K. A. Santiago, F. J. Raab, Sebastiano Bernuzzi, Hartmut Grote, G. Losurdo, G. G. Fronzé, M. Tse, Simone Mozzon, A. Pele, A. Ramos-Buades, Gianluca Grignani, E. Goetz, Neil J. Cornish, P. G. Murray, B. Lantz, M. Boer, R. J. Trudeau, E. J. Sanchez, S. D'Antonio, K.S.J. 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A., Thrane, E., Tinsman, C. L., Saravanan, T. R., Tiwari, Shubhanshu, Tiwari, S., Tiwari, V., Toland, K., Tonelli, M., Tornasi, Z., Torres-Forné, A., Torrie, C. I., Tosta e Melo, I., Töyrä, D., Trail, E. A., Travasso, F., Traylor, G., Tringali, M. C., Tripathee, A., Trovato, A., Trudeau, R. J., Tsang, K. W., Tse, M., Tso, R., Tsukada, L., Tsuna, D., Tsutsui, T., Turconi, M., Ubhi, A. S., Udall, R., Ueno, K., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Utina, A. C., Vahlbruch, H., Vajente, G., Valdes, G., Valentini, M., van Bakel, N., van Beuzekom, M., van den Brand, J. F. J., Van Den Broeck, C., Vander-Hyde, D. C., van der Schaaf, L., Van Heijningen, J. V., van Veggel, A. A., Vardaro, M., Varma, V., Vass, S., Vasúth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Venugopalan, G., Verkindt, D., Veske, D., Vetrano, F., Viceré, A., Viets, A. D., Vinciguerra, S., Vine, D. J., Vinet, J. -Y., Vitale, S., Vivanco, Francisco Hernandez, Vo, T., Vocca, H., Vorvick, C., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walet, R., Walker, M., Wallace, G. S., Wallace, L., Walsh, S., Wang, J. Z., Wang, S., Wang, W. H., Ward, R. L., Warden, Z. A., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L. -W., Weinert, M., Weinstein, A. J., Weiss, R., Wellmann, F., Wen, L., Weßels, P., Westhouse, J. W., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Wilken, D. M., Williams, D., Willis, J. L., Willke, B., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Wofford, J. K., Wong, C., Wright, J. L., Wu, D. S., Wysocki, D. M., Xiao, L., Yamamoto, H., Yang, L., Yang, Y., Yang, Z., Yap, M. J., Yazback, M., Yeeles, D. W., Yu, Hang, Yu, Haocun, Yuen, S. H. R., Zadrożny, A. K., Zadrożny, A., Zanolin, M., Zelenova, T., Zendri, J. -P., Zevin, M., Zhang, J., Zhang, L., Zhang, T., Zhao, C., Zhao, G., Zhou, M., Zhou, Z., Zhu, X. J., Zimmerman, A. B., Zucker, M. E., Zweizig, J., Laboratoire des matériaux avancés (LMA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, 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), 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), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Institut des Fonctions Optiques pour les Technologies de l'informatiON (Institut FOTON), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Laboratoire Kastler Brossel (LKB [Collège de France]), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Collège de France (CdF (institution)), Institut Lumière Matière [Villeurbanne] (ILM), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), Institut Pluridisciplinaire Hubert Curien (IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Institut des Hautes Etudes Scientifiques (IHES), IHES, LIGO Scientific, Virgo, The LIGO Scientific Collaboration, The Virgo Collaboration, 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), 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), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut des Hautes Études Scientifiques (IHES), RS: FSE Grav. waves and fundamental physics, Grav. waves and fundamental physics, RS: FSE MSP, IoP (FNWI), Gravitation and Astroparticle Physics Amsterdam, Other Research IHEF (IoP, FNWI), Faculty of Science, Astroparticle Physics (IHEF, IoP, FNWI), Arene, M., Becsy, B., Calderon Bustillo, J., Castaneda, J., Cavaglia, M., Cerda-Duran, P., Cieslar, M., Cordero-Carrion, I., Dalya, G., D'Angelo, B., D'Antonio, S., Deleglise, S., D'Emilio, V., De Varona, O., Diaz, M. C., D'Urso, D., Fronze, G., Garcia-Quiros, C., Ghosh, A., Gonzalez, G., Guixe, G., Hubner, M. T., Johnson-Mcdaniel, N. K., Kefelian, F., Kim, C., Krolak, A., Kumar, R., Luck, H., Magana Hernandez, I., Magana-Sandoval, F., Marka, S., Marka, Z., Mukherjee, A., Muniz, E. A., O'Brien, B. D., Oram, R. J., O'Reilly, B., O'Shaughnessy, R., Perigois, C., Perries, S., Purrer, M., Rana, J., Rosinska, D., Roy, S., Schonbeck, A., Szczepanczyk, M. J., Tapai, M., Torres-Forne, A., Tosta E Melo, I., Toyra, D., Van Bakel, N., Van Beuzekom, M., Van Den Brand, J. F. J., Van Der Schaaf, L., Van Veggel, A. A., Vasuth, M., Vicere, A., Vivanco, F. H., Wessels, P., Yu, H., Zadrozny, A. K., Zadrozny, A., National Science Foundation (US), Science and Technology Facilities Council (UK), Agencia Estatal de Investigación (España), Generalitat de Catalunya, Govern de les Illes Balears, Generalitat Valenciana, European Commission, Sub Subatomic Physics (SAP), Subatomic Physics, Université Nice Sophia Antipolis (... - 2019) (UNS), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), (Astro)-Particles Physics, LIGO Scientific Collaboration, and Virgo Collaboration
Subjects: Physics and Astronomy (miscellaneous), Astronomy, Gravitational wave detection, Gravitational wave sources, Gravitational waves, Astronomical black holes, agn discs, Astrophysics, detector: network, 01 natural sciences, General Relativity and Quantum Cosmology, Physics, Particles & Fields, star-clusters, gravitational waves, black holes, gravitational waves, black holes, AGN DISCS, LIGO, Virgo, black hole, general relativity, gravitational wave, QC, QB, Physics, Settore FIS/01, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), GRAVITATIONAL WAVE-FORMS, PROGENITORS, COMPACT BINARIES, black hole: spin, PERTURBATIONS, Physical Sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Gravitational wave detection, Astrophysics - High Energy Astrophysical Phenomena, METALLICITY, mass: asymmetry, metallicity, data analysis method, General relativity, MERGERS, gr-qc, Astrophysics::High Energy Astrophysical Phenomena, multipole, PREDICTIONS, FOS: Physical sciences, gravitational waves,black holes, General Relativity and Quantum Cosmology (gr-qc), Astronomy & Astrophysics, gravitational radiation: direct detection, Gravitational waves, Theory of relativity, Binary black hole, Settore FIS/05 - Astronomia e Astrofisica, Astronomical black holes, binary: coalescence, 0103 physical sciences, numerical methods, ddc:530, STAR-CLUSTERS, 010306 general physics, numerical calculations, STFC, Astrophysique, Gravitational wave sources, Science & Technology, mass: solar, 010308 nuclear & particles physics, Gravitational wave, gravitational radiation, RCUK, black hole: mass, Mass ratio, EVOLUTION, gravitational radiation detector, Black hole, detector: sensitivity, Physics and Astronomy, black hole: binary, relativity theory, gravitational radiation: emission, mass ratio, Multipole expansion, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics and astroparticle physics
Abstract: LIGO Scientific Collaboration and Virgo Collaboration: et al., We report the observation of gravitational waves from a binary-black-hole coalescence during the first two weeks of LIGO’s and Virgo’s third observing run. The signal was recorded on April 12, 2019 at 05∶30∶44 UTC with a network signal-to-noise ratio of 19. The binary is different from observations during the first two observing runs most notably due to its asymmetric masses: a ∼30 M⊙ black hole merged with a ∼8M⊙ black hole companion. The more massive black hole rotated with a dimensionless spin magnitude between 0.22 and 0.60 (90% probability). Asymmetric systems are predicted to emit gravitational waves with stronger contributions from higher multipoles, and indeed we find strong evidence for gravitational radiation beyond the leading quadrupolar order in the observed signal. A suite of tests performed on GW190412 indicates consistency with Einstein’s general theory of relativity. While the mass ratio of this system differs from all previous detections, we show that it is consistent with the population model of stellar binary black holes inferred from the first two observing runs., The authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigación, the Vicepresidencia i Conselleria d’Innovació, Recerca i Turisme and the Conselleria d’Educació i Universitat del Govern de les Illes Balears, the Conselleria d’Innovació, Universitats, Ciencia i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland, the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertees (ARC) and Fonds Wetenschappelijk Onderzoek–Vlaanderen (FWO), Belgium, the Paris Île-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and Communications, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTPSAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authorsgratefully acknowledge the support of the NSF, STFC, INFN and CNRS for provision of computational resources.
Published: 2020
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16. Constraining Black Hole Populations in Globular Clusters using Microlensing: Application to Omega Centauri

Author: Zsuzsa Márka, Szabolcs Márka, Johan Samsing, Doğa Veske, Imre Bartos, and John Zaris
Subjects: 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational microlensing, 01 natural sciences, Omega, 0103 physical sciences, Cluster (physics), Astrophysics::Solar and Stellar Astrophysics, Omega Centauri, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Globular star clusters, 0105 earth and related environmental sciences, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Black holes, Astronomy and Astrophysics, Black hole, Stars, Space and Planetary Science, Globular cluster, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Event (particle physics)
Abstract: We estimate the rate of gravitational microlensing events of cluster stars due to black holes (BHs) in the globular cluster NGC 5139 ($\omega Cen$). Theory and observations both indicate that $\omega Cen$ may contain thousands of BHs, but their mass spectrum and exact distribution are not well constrained. In this Letter we show that one may observe microlensing events on a timescale of years in $\omega Cen$, and such an event sample can be used to infer the BH distribution. Direct detection of BHs will, in the near future, play a major role in distinguishing binary BH merger channels. Here we explore how gravitational microlensing can be used to put constraints on BH populations in globular clusters., Comment: 6 pages, 2 figures, published in ApJL
Published: 2019
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17. Bayesian multimessenger search method for common sources of gravitational waves and high-energy neutrinos

Author: Imre Bartos, Zsuzsa Márka, S. T. Countryman, Doğa Veske, Azadeh Keivani, E. Blaufuss, Chad Finley, and Szabolcs Marka
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Gravitational wave, Detector, FOS: Physical sciences, Astronomy, 01 natural sciences, Signal, Coincidence, Constant false alarm rate, 0103 physical sciences, Prior probability, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics, Event (particle physics)
Abstract: Multi-messenger astrophysics is undergoing a transition towards low-latency searches based on signals that could not individually be established as discoveries. The rapid identification of signals is important in order to initiate timely follow-up observations of transient emission that is only detectable for short time periods. Joint searches for gravitational waves and high-energy neutrinos represent a prime motivation for this strategy. Both gravitational waves and high-energy neutrinos are typically emitted over a short time frame of seconds to minutes during the formation or evolution of compact objects. In addition, detectors searching for both messengers observe the whole sky continuously, making observational information on potential transient sources rapidly available to guide follow-up electromagnetic surveys. The direction of high-energy neutrinos can be reconstructed to sub-degree precision, making a joint detection much better localized than a typical gravitational wave signal. Here we present a search strategy for joint gravitational wave and high-energy neutrino events that allows the incorporation of astrophysical priors and detector characteristics following a Bayesian approach. We aim to determine whether a multi-messenger correlated signal is a real event, a chance coincidence of two background events or the chance coincidence of an astrophysical signal and a background event. We use an astrophysical prior that is model agnostic and takes into account mostly geometric factors. Our detector characterization in the search is mainly empirical, enabling detailed realistic accounting for the sensitivity of the detector that can depend on the source properties. By this means, we will calculate the false alarm rate for each multi-messenger event which is required for initiating electromagnetic follow-up campaigns., 12 pages. Accepted in PRD
Published: 2019
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18. Multi-messenger Gravitational-Wave + High-Energy Neutrino Searches with LIGO, Virgo and IceCube

Author: Doğa Veske, K. Rainer Corely, Imre Bartos, Azadeh Keivani, S. T. Countryman, Szabolcs Marka, and Zsuzsa Márka
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010504 meteorology & atmospheric sciences, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy, Binary number, 01 natural sciences, 7. Clean energy, LIGO, IceCube Neutrino Observatory, Particle acceleration, General Relativity and Quantum Cosmology, Neutron star, Coincident, 0103 physical sciences, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: Multi-messenger searches for gravitational waves and high-energy neutrinos provide important insights into the dynamics of and particle acceleration by black holes and neutron stars. With LIGO's third observing period (O3), the number of gravitational wave detections has been substantially increased. The rapid identification of joint signals is crucial for electromagnetic follow-up observations of transient emission that is only detectable for short periods of time. High-energy neutrino direction can be reconstructed to sub-degree precision, making a joint detection far better localized than a standalone gravitational-wave signal. We present the latest sensitivity of joint searches and discuss the Low-Latency Algorithm for Multi-messenger Astrophysics (LLAMA) that combines LIGO/Virgo gravitational-wave candidates and searches in low-latency for coincident high-energy neutrinos from the IceCube Neutrino Observatory. We will further discuss future prospects of joint searches from the perspective of better understanding the interaction of relativistic and sub-relativistic outflows from binary neutron star mergers., Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributions
Published: 2019
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19. An Archival Search for Neutron-star Mergers in Gravitational Waves and Very-high-energy Gamma Rays

Author: M. Lundy, Lucy Fortson, Reshmi Mukherjee, M. K. Daniel, A. Weinstein, C. Giuri, P. Kaaret, David Kieda, Olivier Hervet, C. E. McGrath, S. Márka, Wystan Benbow, Martin Pohl, A. D. Falcone, Alasdair E. Gent, P. Moriarty, R. A. Ong, James Ryan, S. Kumar, J. H. Buckley, R. R. Prado, P. T. Reynolds, M. Kertzman, Amy Furniss, M. Nievas-Rosillo, Nahee Park, A. J. Chromey, Doğa Veske, G. H. Sembroski, M. Capasso, Q. Feng, E. Pueschel, Imre Bartos, Jodi Christiansen, A. Brill, Daniel Nieto, David A. Williams, Marcos Santander, A. N. Otte, K. Pfrang, C. B. Adams, D. S. Hanna, G. Hughes, J. P. Finley, Jamie Holder, K. R. Corley, K. Ragan, R. Shang, T. J. Williamson, Z. Márka, S. O'Brien, E. Roache, K. A. Farrell, Tarek M. Hassan, John L. Quinn, D. Ribeiro, W. Jin, M. J. Lang, Manel Errando, S. Patel, T. B. Humensky, and Gernot Maier
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy, Astronomy and Astrophysics, IACT, Gamma-ray astronomy, Cherenkov Telescope Array, 030226 pharmacology & pharmacy, 01 natural sciences, LIGO, 03 medical and health sciences, Neutron star, 0302 clinical medicine, Space and Planetary Science, 0103 physical sciences, Astrophysics - High Energy Astrophysical Phenomena, Gamma-ray burst, 010303 astronomy & astrophysics, Cherenkov radiation
Abstract: The recent discovery of electromagnetic signals in coincidence with neutron-star mergers has solidified the importance of multimessenger campaigns in studying the most energetic astrophysical events. Pioneering multimessenger observatories, such as LIGO/Virgo and IceCube, record many candidate signals below the detection significance threshold. These sub-threshold event candidates are promising targets for multimessenger studies, as the information provided by them may, when combined with contemporaneous gamma-ray observations, lead to significant detections. Here we describe a new method that uses such candidates to search for transient events using archival very-high-energy gamma-ray data from imaging atmospheric Cherenkov telescopes (IACTs). We demonstrate the application of this method to sub-threshold binary neutron star (BNS) merger candidates identified in Advanced LIGO's first observing run. We identify eight hours of archival VERITAS observations coincident with seven BNS merger candidates and search them for TeV emission. No gamma-ray emission is detected; we calculate upper limits on the integral flux and compare them to a short gamma-ray burst model. We anticipate this search method to serve as a starting point for IACT searches with future LIGO/Virgo data releases as well as in other sub-threshold studies for multimessenger transients, such as IceCube neutrinos. Furthermore, it can be deployed immediately with other current-generation IACTs, and has the potential for real-time use that places minimal burden on experimental operations. Lastly, this method may serve as a pilot for studies with the Cherenkov Telescope Array, which has the potential to observe even larger fields of view in its divergent pointing mode.
Published: 2021
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20. How to Search for Multiple Messengers—A General Framework Beyond Two Messengers

Author: Doğa Veske, Szabolcs Márka, Imre Bartos, and Zsuzsa Márka
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Astrostatistics, Theoretical computer science, 010504 meteorology & atmospheric sciences, Gravitational wave, High-energy astronomy, Astrophysics::High Energy Astrophysical Phenomena, Model selection, Event (relativity), FOS: Physical sciences, Astronomy and Astrophysics, 01 natural sciences, Bayesian statistics, Space and Planetary Science, 0103 physical sciences, Neutrino, Neutrino astronomy, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: Quantification of the significance of a candidate multi-messenger detection of cosmic events is an emerging need in the astrophysics and astronomy communities. In this paper we show that a model-independent optimal search does not exist, and we present a general Bayesian method for the optimal model-dependent search, which is scalable to any number and any kind of messengers, and applicable to any model. In the end, we demonstrate it through an example for a joint gravitational wave, high-energy neutrino, short gamma-ray burst event search; which has not been examined heretofore., 8 pages
Published: 2021
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21. Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?

Author: Andrew G. Sullivan, Doğa Veske, Peter Shawhan, Zsuzsa Márka, Szabolcs Márka, S. W. Ballmer, and Imre Bartos
Subjects: Time delay and integration, Physics, Physics and Astronomy (miscellaneous), Einstein Telescope, 010308 nuclear & particles physics, General relativity, Gravitational wave, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, Shapiro delay, General Relativity and Quantum Cosmology, LIGO, Computational physics, Amplitude, Tests of general relativity, 0103 physical sciences, Astrophysics - Instrumentation and Methods for Astrophysics, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract: Shapiro time delay is one of the fundamental tests of general relativity and post-Newtonian theories of gravity. Consequently, its measurements can be used to probe the parameter $\gamma$ which is related to spacetime curvature produced by a unit mass in the post-Newtonian formalism of gravity. To date all measurements of time delay have been conducted on astronomical scales. It was asserted in 2010 that gravitational wave detectors on Earth could be used to measure Shapiro delay on a terrestrial scale via massive rotating systems. Building on that work, we consider how measurements of Shapiro delay can be made using next-generation gravitational wave detectors. We perform an analysis for measuring Shapiro delay with the next-generation gravitational wave detectors Cosmic Explorer and Einstein Telescope to determine how precisely the effect can be measured. Using a rotating mass unit design, we find that Cosmic Explorer and Einstein Telescope can measure the Shapiro delay signal with amplitude signal to noise ratios upwards of $\sim28 $ and $\sim43$ in 1 year of integration time, respectively. By measuring Shapiro delay with this technique, next-generation interferometers will allow for terrestrial measurements of $\gamma$ in the paramaterized post-Newtonian formalism of gravity with sub-percent precision., Comment: 15 pages, 5 figures, Version accepted to Classical and Quantum Gravity, includes modified figures
Published: 2020
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22. Pretest setup installation of the METU-DBL project to perform space radiation tests

Author: Pelin Uslu, Aysenur Gencer, Doğa Veske, Gamze Kilicerkan Baslar, Attilio Milanese, Selcen Uzun Duranz, Baran Bodur, Akanay Avaroglu, Ilker Sahin, M. Bilge Demirkoz, Ramazan Uzel, Merve Yigitoglu, Ilias Efthymiopoulos, and M. Serdar Aydin
Subjects: Physics, Large Hadron Collider, Solar energetic particles, Spacecraft, 010308 nuclear & particles physics, business.industry, Electrical engineering, Cosmic ray, 01 natural sciences, Atmosphere of Earth, Beamline, Physics::Space Physics, 0103 physical sciences, Electromagnetic shielding, Satellite, Aerospace engineering, 010306 general physics, business
Abstract: Satellites and spacecrafts are exposed to space radiation environment during their mission. This environment consists of cosmic rays, solar particles and trapped particles. Cosmic rays are coming from the outside of our solar system. Solar particles are produced by the Sun. These particles can be trapped around the Earth's magnetic field lines when they approach the Earth's atmosphere. These particles can affect performance and robustness of electronic components or materials used in space and such effects can be classified as Total Ionising Dose (TID), Single Event Effect (SEE) and Displacement Damage (DD). To ensure the performance of innovative components or materials that will be used in space, they must be tested before they are launched to space. Currently, only TID tests can be realized in Turkey but others cannot be performed yet. METU is building a beamline to perform some types of SEE tests. METU-DBL (Defocusing Beam Line) project supported by the Ministry of Development started in August 2015 is funded with 7 million TL. This project is conducted in collaboration with CERN for knowledge and technology transfer to Turkey. After this 10 meter long beamline is built, SEE tests can be performed with 15–30 MeV protons. As a part of this project, solar cells and Li-Ion battery of the IMECE satellite will be tested by METU-DBL.
Published: 2017
Full Text: View/download PDF

23. Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo

Author: Rich Abbott, Thomas D. Abbott, Sheelu Abraham, Fausto Acernese, Kendall Ackley, Carl Adams, Rana X. Adhikari, Vaishali B. Adya, Christoph Affeldt, Michalis Agathos, Kazuhiro Agatsuma, Nancy Aggarwal, Odylio D. Aguiar, Amit Aich, Lorenzo Aiello, Anirban Ain, Ajith Parameswaran, Gabrielle Allen, Annalisa Allocca, Paul A. Altin, Alex Amato, Shreya Anand, Alena Ananyeva, Stuart B. Anderson, Warren G. Anderson, Svetoslava V. Angelova, Stefano Ansoldi, Sarah Antier, Stephen Appert, Koji Arai, Melody C. Araya, Joseph S. Areeda, Marc Arène, Nicolas Arnaud, Scott M. Aronson, Kg G. Arun, Stefano Ascenzi, Gregory Ashton, Stuart M. Aston, Pia Astone, Florian Aubin, Peter Aufmuth, Kellie AultONeal, Corey Austin, Valerie Avendano, Stanislav Babak, Philippe Bacon, Francesca Badaracco, Maria K.M. Bader, Sangwook Bae, Anne M. Baer, Jonathon Baird, Francesca Baldaccini, Giulio Ballardin, Stefan W. Ballmer, Anna-marie Bals, Alexander Balsamo, Gregory Baltus, Sharan Banagiri, Deepak Bankar, Rameshwar S. Bankar, Juan C. Barayoga, Claudio Barbieri, Barry C. Barish, David Barker, Kevin Barkett, Pablo Barneo, Fabrizio Barone, Bryan Barr, Lisa Barsotti, Matteo Barsuglia, Daniel Barta, Jeffrey Bartlett, Imre Bartos, Riccardo Bassiri, Andrea Basti, Mateusz Bawaj, Joseph C. Bayley, Marco Bazzan, Bence Bécsy, Michal Bejger, Imene Belahcene, Angus S. Bell, Deeksha Beniwal, Michael G. Benjamin, Joe D. Bentley, Fabio Bergamin, Beverly K. Berger, Gerald Bergmann, Sebastiano Bernuzzi, Christopher P.L. Berry, Diego Bersanetti, Alessandro Bertolini, Joseph Betzwieser, Rohan Bhandare, Ankit V. Bhandari, Jeffrey Bidler, Edward Biggs, Igor A. Bilenko, Garilynn Billingsley, Imogen Birney, Ofek Birnholtz, Sebastien Biscans, Matteo Bischi, Sylvia Biscoveanu, Aparna Bisht, Guldauren Bissenbayeva, Massimiliano Bitossi, Marieanne A. Bizouard, Kent K. Blackburn, Jonathan Blackman, Carl D. Blair, David G. Blair, Ryan M. Blair, Fabrizio Bobba, Nina Bode, Michel Boer, Yannick Boetzel, Gilles Bogaert, Francois Bondu, Edgard Bonilla, Romain Bonnand, Phillip Booker, Boris A. Boom, Rolf Bork, Valerio Boschi, Sukanta Bose, Vladimir Bossilkov, Joel Bosveld, Yann Bouffanais, Antonella Bozzi, Carlo Bradaschia, Patrick R. Brady, Alyssa Bramley, Marica Branchesi, Jim E. Brau, Matteo Breschi, Tristan Briant, Joseph H. Briggs, Francesco Brighenti, Alain Brillet, Marc Brinkmann, Patrick Brockill, Aidan F. Brooks, Jonathan Brooks, Daniel D. Brown, Sharon Brunett, Giacomo Bruno, Robert Bruntz, Aaron Buikema, Tomasz Bulik, Henk J. Bulten, Alessandra Buonanno, Damir Buskulic, Robert L. Byer, Miriam Cabero, Laura Cadonati, Giampietro Cagnoli, Craig Cahillane, Juan Calderón Bustillo, Jack D. Callaghan, Thomas A. Callister, Enrico Calloni, Jordan B. Camp, Maurizio Canepa, Kipp C. Cannon, Huy-tuong Cao, Junwei Cao, Giovanni Carapella, Franco Carbognani, Santiago Caride, Matthew F. Carney, Gregorio Carullo, Julia Casanueva Diaz, Claudio Casentini, Javier Castañeda, Sarah Caudill, Marco Cavaglià, Fabien Cavalier, Roberto Cavalieri, Giancarlo Cella, Pablo Cerdá-Durán, Elisabetta Cesarini, Oualid Chaibi, Kabir Chakravarti, Chiwai Chan, Manleong Chan, Shiuh Chao, Philip Charlton, Eve A. Chase, Eric Chassande-Mottin, Deep Chatterjee, Mayank Chaturvedi, Hsin-yu Y. Chen, Xu Chen, Yanbei Chen, Hai-ping Cheng, Chi-kit K. Cheong, Hanyu Y. Chia, Francesco Chiadini, Roberto Chierici, Andrea Chincarini, Antonino Chiummo, Gihyuk Cho, Heesuk S. Cho, Min-a Cho, Nelson Christensen, Qi Chu, Sheon Chua, Ka-wai W. Chung, Shinkee Chung, Giacomo Ciani, Pawel Ciecielag, Marek Cieślar, Alexei A. Ciobanu, Riccardo Ciolfi, Francesco Cipriano, Alessio Cirone, Filiberto Clara, James A. Clark, Patrick Clearwater, Sebastien Clesse, Frederic Cleva, Eugenio Coccia, Pierre-francois Cohadon, David Cohen, Marta Colleoni, Christophe G. Collette, Christopher Collins, Monica Colpi, Marcio Constancio Jr., Livia Conti, Sam J. Cooper, Paul Corban, Thomas R. Corbitt, Isabel Cordero-Carrión, Silvia Corezzi, Kenneth R. Corley, Neil Cornish, David Corre, Alessandra Corsi, Stefano Cortese, Cesar A. Costa, Roberto Cotesta, Michael W. Coughlin, Scott B. Coughlin, Jeanpierre Coulon, Stefan T. Countryman, Peter Couvares, Pep B. Covas, David M. Coward, Matthew J. Cowart, Dennis C. Coyne, Robert Coyne, Jolien D. E. Creighton, Teviet D. Creighton, Jonathan Cripe, Michael Croquette, Sgwynne G. Crowder, Jean-rene Cudell, Torrey J. Cullen, Alan Cumming, Rebecca Cummings, Liam Cunningham, Elena Cuoco, Malgorzata Curylo, Tito Dal Canton, Gergely Dálya, Aykutlu Dana, Lara M. Daneshgaran-Bajastani, Beatrice D’Angelo, Stefan L. Danilishin, Sabrina D’Antonio, Karsten Danzmann, Christian Darsow-Fromm, Arnab Dasgupta, Laurence E. H. Datrier, Vincenzo Dattilo, Ishant Dave, Michel Davier, Gareth S. Davies, Derek Davis, Edward J. Daw, Dan DeBra, Malathi Deenadayalan, Jerome Degallaix, Martina De Laurentis, Samuel Deléglise, Matthew Delfavero, Nicola De Lillo, Walter Del Pozzo, Lindsay M. DeMarchi, Virginia D’Emilio, Nicholas Demos, Thomas Dent, Roberto De Pietri, Rosario De Rosa, Camilla De Rossi, Riccardo DeSalvo, Omar de Varona, Sanjeev Dhurandhar, Mario C. Díaz, Mauricio Diaz-Ortiz Jr., Tim Dietrich, Luciano Di Fiore, Chiara Di Fronzo, Cinzia Di Giorgio, Fabrizio Di Giovanni, Matteo Di Giovanni, Tristano Di Girolamo, Alberto Di Lieto, Binlei Ding, Sibilla Di Pace, Irene Di Palma, Francesco Di Renzo, Atul K. Divakarla, Artemiy Dmitriev, Zoheyr Doctor, Fred Donovan, Katherine L. Dooley, Suresh Doravari, Iain Dorrington, Thomas P. Downes, Marco Drago, Jenne C. Driggers, Zhihui Du, Jean-gregoire Ducoin, Peter Dupej, Ofelia Durante, Domenico D’Urso, Sheila E. Dwyer, Paul J. Easter, Graeme Eddolls, Bruce Edelman, Tega B. Edo, Oliver Edy, Anamaria Effler, Phil Ehrens, Johannes Eichholz, Stephen S. Eikenberry, Marc Eisenmann, Robert A. Eisenstein, Aldo Ejlli, Lucianolucianikerrico Errico, Reed C. Essick, Hector Estelles, Dimitri Estevez, Zachariah B. Etienne, Todd Etzel, Matthew Evans, Tom M. Evans, Rebecca E. Ewing, Viviana Fafone, Stephen Fairhurst, Xilong Fan, Stefania Farinon, Benjamin Farr, Will M. Farr, Edward J. Fauchon-Jones, Marc Favata, Maxime Fays, Mariana Fazio, Jon Feicht, Martin M. Fejer, Fangchen Feng, Edit Fenyvesi, Deborah L. Ferguson, Alvaro Fernandez-Galiana, Isidoro Ferrante, Elvis C. Ferreira, Tabata A. Ferreira, Francesco Fidecaro, Irene Fiori, Donatella Fiorucci, Maya Fishbach, Ryan P. Fisher, Rosalba Fittipaldi, Margot Fitz-Axen, Vincenzo Fiumara, Raffaele Flaminio, Erik Floden, Eric Flynn, Heather Fong, Antonio A. Font, Perry Forsyth, Jean-daniel Fournier, Sergio Frasca, Franco Frasconi, Zsolt Frei, Andreas Freise, Raymond Frey, Valentin Frey, Peter Fritschel, Valery V. Frolov, Gabriele Fronzè, Paul Fulda, Michael Fyffe, Hunter A. Gabbard, Bhooshan U. Gadre, Sebastian M. Gaebel, Jonathan R. Gair, Shanika Galaudage, Dhruva Ganapathy, Sharad G. Gaonkar, Cecilio García-Quirós, Fabio Garufi, Bubba Gateley, Sergio Gaudio, Gayathri Gayathri, Gianluca Gemme, Eric Genin, Alberto Gennai, Daniel George, Jogy George, Laszlo Gergely, Sudarshan Ghonge, Abhirup Ghosh, Archisman Ghosh, Shaon Ghosh, Bruno Giacomazzo, Joe A. Giaime, Dwayne D. Giardina, Des R. Gibson, Chalisa Gier, Kiranjyot Gill, Jane Glanzer, Jan Gniesmer, Patrick Godwin, Evan Goetz, Ryan Goetz, Niklas Gohlke, Boris Goncharov, Gabriela González, Gopakumar Gopakumar, Sarah E. Gossan, Matthieu Gosselin, Romain Gouaty, Benjamin Grace, Aniello Grado, Massimo Granata, Alastair Grant, Slawomir Gras, Philippe Grassia, Corey Gray, Rachel Gray, Giuseppe Greco, Anna C. Green, Rhys Green, Elizabeth M. Gretarsson, Hannah L. Griggs, G. Grignani, Andrea Grimaldi, Stefan J. Grimm, Hartmut Grote, Steffen Grunewald, Pierre Gruning, Gianluca M. Guidi, Andre R. Guimaraes, Gerard Guixé, Hitesh K. Gulati, Yuefan Guo, Anuradha Gupta, Anchal Gupta, Pawan Gupta, Eric K. Gustafson, Dick Gustafson, Leila Haegel, Odysse Halim, Evan D. Hall, Eleanor Z. Hamilton, Giles Hammond, Maria Haney, Manuela M. Hanke, Jonathan Hanks, Chad Hanna, Mark D. Hannam, Otto A. Hannuksela, Travis J. Hansen, Joe Hanson, Thomas Harder, Terra Hardwick, Haris Haris, Jan Harms, Gregg M. Harry, Ian W. Harry, Raine K. Hasskew, Carl-johan Haster, Karen Haughian, Fergus J. Hayes, James Healy, Antoine Heidmann, Matthew C. Heintze, Joscha Heinze, Henrich Heitmann, Frances Hellman, Patrice Hello, Gary Hemming, Martin Hendry, Siong S. Heng, Eric Hennes, Jan-simon Hennig, Michele Heurs, Stefan Hild, Tanja Hinderer, Sarah Y. Hoback, Sven Hochheim, Elyssa Hofgard, David Hofman, Aaron M. Holgado, Nathan A. Holland, Kathy Holt, Daniel E. Holz, Paul Hopkins, Christian Horst, James Hough, Eric J. Howell, Charlie G. Hoy, Yiwen Huang, Moritz T. Hübner, Eliu A. Huerta, Dominique Huet, Brennan Hughey, Victor Hui, Sascha Husa, Sabina H. Huttner, Rachael Huxford, Tien Huynh-Dinh, Bartosz Idzkowski, Alberto Iess, Henri Inchauspe, Craig Ingram, Giuseppe Intini, Isac, Jean M., Max Isi, Bala R. Iyer, Thibaut Jacqmin, Sameer J. Jadhav, Shreejit P. Jadhav, Alasdair L. James, Karan Jani, Nagaraj N. Janthalur, Piotr Jaranowski, Deep Jariwala, Rafel Jaume, Alex C. Jenkins, Jun Jiang, Grace R. Johns, Aaron W. Jones, Ian I. Jones, Jeff D. Jones, Philip Jones, Russell Jones, Reinier J. G. Jonker, Ju Ju, Jonas Junker, Chinmay V. Kalaghatgi, Vassiliki Kalogera, Brittany Kamai, Shivaraj Kandhasamy, Gungwon Kang, Jonah B. Kanner, Shasvath J. Kapadia, Sudarshan Karki, Rahul Kashyap, Marie Kasprzack, Wolfgang Kastaun, Stavros Katsanevas, Erik Katsavounidis, William Katzman, Steffen Kaufer, Keita Kawabe, Fabien Kéfélian, David Keitel, Azadeh Keivani, Ross Kennedy, Joey S. Key, Sudiksha Khadka, Farit Y. Khalili, Imran Khan, Sebastian Khan, Zaki A. Khan, Efim A. Khazanov, Nandita Khetan, Mohammad Khursheed, Nutsinee Kijbunchoo, Chunglee Kim, Grace J. Kim, Jeongcho C. Kim, Kyungmin Kim, Won Kim, Whansun S. Kim, Young-min Kim, Charles Kimball, Peter J. King, Maya Kinley-Hanlon, Robin Kirchhoff, Jeffrey S. Kissel, Lisa Kleybolte, Sergei Klimenko, Tyler D. Knowles, Philip Koch, Sina M. Koehlenbeck, Gideon Koekoek, Soumen Koley, Veronica Kondrashov, Antonios Kontos, Nico Koper, Mikhail Korobko, William Z. Korth, Manoj Kovalam, Dan B. Kozak, Volker Kringel, Nv V. Krishnendu, Andrzej Królak, Natalie Krupinski, Gerrit Kuehn, Anil Kumar, Prayush Kumar, Rahul Kumar, Rakesh Kumar, Sumit Kumar, Ling-chi Kuo, Adam Kutynia, Benjamin D. Lackey, Danny Laghi, Emile Lalande, Lam L. Lam, Astrid Lamberts, Michael Landry, Benjamin B. Lane, Ryan N. Lang, Jacob Lange, Brian Lantz, Robert K. Lanza, Iuri La Rosa, Angelique Lartaux-Vollard, Paul D. Lasky, Michael Laxen, Albert Lazzarini, Claudia Lazzaro, Paola Leaci, Sean Leavey, Yannick K. Lecoeuche, Chang-hwan H. Lee, Hyung-mok M. Lee, Hyungwon W. Lee, Joongoo Lee, Kyung-ha Lee, Johannes Lehmann, Nicolas Leroy, Nicolas Letendre, Yuri Levin, Alvin K. Y. Li, Jin Li, Kaye li, Tjonnie G. F. Li, Xiang Li, Frank Linde, Seth D. Linker, Jethro N. Linley, Tyson B. Littenberg, Liu Liu, Xiaoshu Liu, Miquel Llorens-Monteagudo, Ka-lok Lo, Alexandra Lockwood, Lionel T. London, Alessandro Longo, Matteo Lorenzini, Vincent Loriette, Marc Lormand, Giovanni Losurdo, James D. Lough, Carlos O. Lousto, Geoffrey Lovelace, Harald Lück, Diana Lumaca, Andrew P. Lundgren, Ma Yiqiu, Ronaldas Macas, Sean Macfoy, Myron MacInnis, Duncan M. Macleod, Ian O. MacMillan, Adrian Macquet, Ignacio Magaña Hernandez, Fabian Magaña-Sandoval, Ryan M. Magee, Ettore Majorana, Ivan Maksimovic, Asmita Malik, Catherine Man, Vuk Mandic, Valentina Mangano, Georgia L. Mansell, Michael Manske, Maddalena Mantovani, Michela Mapelli, Fabio Marchesoni, Frederique Marion, Szabolcs Márka, Zsuzsanna Márka, Charalampos Markakis, Ashot S. Markosyan, Aaron Markowitz, Ed Maros, Antonio Marquina, Sylvain Marsat, Filippo Martelli, Ian W. Martin, Rodica M. Martin, Valerie Martinez, Denis V. Martynov, Hossein Masalehdan, Ken Mason, Elena Massera, Alain Masserot, Thomas J. Massinger, Mariela Masso-Reid, Simone Mastrogiovanni, Andrew Matas, Fabrice Matichard, Nergis Mavalvala, Emily Maynard, Joshua J. McCann, Richard McCarthy, David E. McClelland, Scott McCormick, Lee McCuller, Stephen C. McGuire, Connor McIsaac, Jessica McIver, David J. McManus, Terry McRae, Sean T. McWilliams, Duncan Meacher, Grant D. Meadors, Moritz Mehmet, Ajit K. Mehta, Elena Mejuto Villa, Andrew Melatos, Gregory Mendell, Adam A. Mercer, Lorenzo Mereni, Kara Merfeld, Edmond L. Merilh, Jonathan D. Merritt, Mourad Merzougui, Syd Meshkov, Chris Messenger, Cody Messick, Remi Metzdorff, Patrick M. Meyers, Fabian Meylahn, Ashish Mhaske, Andrea Miani, Haixing Miao, Ioannis Michaloliakos, Christophe Michel, Hannah Middleton, Leopoldo Milano, Andrewlawrence L. Miller, Meg Millhouse, Joseph C. Mills, Edoardo Milotti, Michael C. Milovich-Goff, Olivier Minazzoli, Yuri Minenkov, Alec Mishkin, Chandra Mishra, Timesh Mistry, Sanjit Mitra, Valery P. Mitrofanov, Guenakh Mitselmakher, Richard Mittleman, Geoffrey Mo, Kentaro Mogushi, Satyanarayan R. P. Mohapatra, Siddharth R. Mohite, Manel Molina-Ruiz, Marina Mondin, Matteo Montani, Christopher J. Moore, Dan Moraru, Filip Morawski, Gerardo Moreno, Soichiro Morisaki, Benoit Mours, Conor M. Mow-Lowry, Simone Mozzon, Federico Muciaccia, Arunava Mukherjee, Debnandini Mukherjee, Soma Mukherjee, Subroto Mukherjee, Nikhil Mukund, Adam Mullavey, Jesper Munch, Erik A. Muñiz, Peter G. Murray, Alessandro Nagar, Ilaria Nardecchia, Luca Naticchioni, Rajesh K. Nayak, Benjamin F. Neil, Joshua Neilson, Gijs Nelemans, Timothy J. N. Nelson, Marina Nery, Ansel Neunzert, Kwan-yeung Y. Ng, Sebastian Ng, Catherine Nguyen, Philippe Nguyen, David Nichols, Shania A. Nichols, Samaya Nissanke, Flavio Nocera, Minkyun Noh, Chris North, Devon Nothard, Laura K. Nuttall, Jason Oberling, Brendan D. O’Brien, Gor Oganesyan, Greg H. Ogin, John J. Oh, Sanghoon H. Oh, Frank Ohme, Hiroaki Ohta, Marcos A. Okada, Miquel Oliver, Christian Olivetto, Patrick Oppermann, Richard Oram, Brian O’Reilly, Rich G. Ormiston, Luis F. Ortega, Richard O’Shaughnessy, Serguei Ossokine, Charles Osthelder, David J. Ottaway, Harry Overmier, Ben J. Owen, Alexander E. Pace, Giulia Pagano, Michael A. Page, Giulia Pagliaroli, Archana Pai, Siddhesh A. Pai, Jordan R. Palamos, Oleg Palashov, Cristiano Palomba, Howard Pan, Pratap K. Panda, Tsun-ho Pang, Chris Pankow, Francesco Pannarale, Brijesh C. Pant, Federico Paoletti, Andrea Paoli, Abhishek Parida, William Parker, Daniela Pascucci, Antonio Pasqualetti, Roberto Passaquieti, Diego Passuello, Barbara Patricelli, Ethan Payne, Brynley L. Pearlstone, Thida C. Pechsiri, Ari J. Pedersen, Mike Pedraza, Arnaud Pele, Steven Penn, Albino Perego, Carlos J. Perez, Perigois Périgois, Antonio Perreca, Stephane Perriès, Jan Petermann, Harald P. Pfeiffer, Margot Phelps, Khun S. Phukon, Ornella J. Piccinni, Mikhael Pichot, Marco Piendibene, Francesco Piergiovanni, Vincenzo Pierro, Gabriel Pillant, Laurent Pinard, Innocenzo M. Pinto, Krzysztof Piotrzkowski, Marc Pirello, Matthew Pitkin, Wolfango Plastino, Rosa Poggiani, Yat-tung T. Pong, Sarah Ponrathnam, Pasquale Popolizio, Ed K. Porter, Jade Powell, Atul K. Prajapati, Kiran Prasai, Raghurama Prasanna, Geraint Pratten, Tanner Prestegard, Maria Principe, Giovanni A. Prodi, Leonid Prokhorov, Michele Punturo, Paola Puppo, Michael Pürrer, Hong Qi, Volker Quetschke, Pedro J. Quinonez, Fred J. Raab, Geert Raaijmakers, Hugh Radkins, Nicholas Radulesco, Peter Raffai, Hanna Rafferty, Sendhil Raja, Rajan Rajan, Binod Rajbhandari, Malik Rakhmanov, Karla E. Ramirez, Antoni Ramos-Buades, Javed Rana, Kaushik Rao, Piero Rapagnani, Vivien Raymond, Massimiliano Razzano, Jocelyn Read, Tania Regimbau, Luca Rei, Stuart Reid, David H. Reitze, Piero Rettegno, Fulvio Ricci, Colter J. Richardson, Jonathan W. Richardson, Paul M. Ricker, Gunnar Riemenschneider, Keith Riles, Monica Rizzo, Norna A. Robertson, Florent Robinet, Alessio Rocchi, Ramon D. Rodriguez-Soto, Loic Rolland, Jameson G. Rollins, Vincent J. Roma, Marco Romanelli, Rocco Romano, Chandra L. Romel, Isobel M. Romero-Shaw, Janeen H. Romie, Caitlin A. Rose, Dakota Rose, Kyle Rose, Dorota Rosińska, Shawn G. Rosofsky, Michael P. Ross, Sheila Rowan, Samuel J. Rowlinson, Palash K. Roy, Santosh Roy, Soumen Roy, Paolo Ruggi, Guntis Rutins, Kyle Ryan, Surabhi Sachdev, Travis Sadecki, Mairi Sakellariadou, Om S. Salafia, Livio Salconi, Muhammed Saleem, Anuradha Samajdar, Eduardo J. Sanchez, Luis E. Sanchez, Nicolas Sanchis-Gual, Jaclyn R. Sanders, Kevin A. Santiago, Edison Santos, Nikhil Sarin, Benoit Sassolas, B S. Sathyaprakash, Orion Sauter, Richard L. Savage, Vaibhav Savant, Disha Sawant, Sihem Sayah, Dean Schaetzl, Paul Schale, Mark Scheel, Jacob Scheuer, Patricia Schmidt, Roman Schnabel, Robert M. S. Schofield, Axel Schönbeck, Emil Schreiber, Bernd W. Schulte, Bernard F. Schutz, Otto Schwarm, Eyal Schwartz, Jamie Scott, Susan M. Scott, Ed Seidel, Danny Sellers, Anand S. Sengupta, Noah Sennett, Daniel Sentenac, Valeria Sequino, Alexander Sergeev, Yoshinta Setyawati, Daniel A. Shaddock, Thomas Shaffer, Selim S. Shahriar, A. Sharma, Priyanka Sharma, Peter Shawhan, Hongyu Shen, Minori Shikauchi, Rosalie Shink, David H. Shoemaker, Deirdre M. Shoemaker, Keerti Shukla, Shyamsundar ShyamSundar, Karelle Siellez, Magdalena Sieniawska, Daniel Sigg, Leo P. Singer, Divya Singh, Neha Singh, Ayatri Singha, Akshat Singhal, Alicia M. Sintes, Valeria Sipala, Vasileios Skliris, Bram J. J. Slagmolen, Teresa J. Slaven-Blair, Jiri Smetana, Joshua R. Smith, Rory J. E. Smith, Surendranadh Somala, Edwin J. Son, Siddharth Soni, Borja Sorazu, Viola Sordini, Fiodor Sorrentino, Tarun Souradeep, Eric Sowell, Andrew P. Spencer, Mario Spera, Amit K. Srivastava, Varun Srivastava, Kai Staats, Cosmin Stachie, Mark Standke, Daniele A. Steer, Michael Steinke, Jessica Steinlechner, Sebastian Steinlechner, Daniel Steinmeyer, Dane Stocks, David J. Stops, Madeline Stover, Ken A. Strain, Giulia Stratta, Amber Strunk, Riccardo Sturani, Amber L. Stuver, Sudhagar Sudhagar, Vivishek Sudhir, Tiffany Z. Summerscales, Ling Sun, Sunil Sunil, Ankan Sur, Jishnu Suresh, Patrick J. Sutton, Bas L. Swinkels, Marek J. Szczepańczyk, Matteo Tacca, Simon C. Tait, Colm Talbot, Andres J. Tanasijczuk, David B. Tanner, Duo Tao, Marton Tápai, Amauri Tapia, Enzo N. Tapia San Martin, Jay D. Tasson, Robert Taylor, Rodrigo Tenorio, Lukas Terkowski, Manasadevi P. Thirugnanasambandam, Michael Thomas, Patrick Thomas, Jonathan E. Thompson, Sivananda R. Thondapu, Keith A. Thorne, Eric Thrane, Calley L. Tinsman, Saravanan R. Saravanan, Shubhanshu Tiwari, Srishti Tiwari, Vaibhav Tiwari, Karl Toland, Mauro Tonelli, Zeno Tornasi, Alejandro Torres-Forné, Calum I. Torrie, Iara Tosta e Melo, Daniel Töyrä, Emily A. Trail, Flavio Travasso, Gary Traylor, Maria C. Tringali, Aashish Tripathee, Agata Trovato, Randy J. Trudeau, Ka-wa W. Tsang, Maggie Tse, Rhondale Tso, Leo Tsukada, Daichi Tsuna, Takuya Tsutsui, Margherita Turconi, Amit S. Ubhi, Koh Ueno, Dennis Ugolini, Cs S. Unnikrishnan, Alexander L. Urban, Samantha A. Usman, Andrei C. Utina, Henning Vahlbruch, Gabriele Vajente, Guillermo Valdes, Michele Valentini, M. Vallisneri, Niels van Bakel, Martin van Beuzekom, Jo F. J. van den Brand, Chris Van Den Broeck, Daniel C. Vander-Hyde, Laura van der Schaaf, Joris V. Van Heijningen, Marielle A. van Veggel, Marco Vardaro, Vijay Varma, Steve Vass, Matyas Vasúth, Alberto Vecchio, Gabriele Vedovato, John Veitch, Peter J. Veitch, Krishna Venkateswara, Gautam Venugopalan, Didier Verkindt, Doga Veske, Flavio Vetrano, Andrea Viceré, Aaron D. Viets, Serena Vinciguerra, David J. Vine, Jeanyves Vinet, Salvatore Vitale, Francisco Hernandez Vivanco, Thomas Vo, Helios Vocca, Cheryl Vorvick, Sergey P. Vyatchanin, Andrew R. Wade, Leslie E. Wade, Madeline Wade, Rob Walet, Marissa Walker, Gavin S. Wallace, Larry Wallace, Sinead Walsh, Jonathan Z. Wang, Sibo Wang, Wenhui H. Wang, Yifan F. Wang, Robert L. Ward, Zane A. Warden, Jim Warner, Michal Was, Jennifer Watchi, Betsy Weaver, Li-wei Wei, Michael Weinert, Alan J. Weinstein, Rainer Weiss, Felix Wellmann, Linqing Wen, Peter Weßels, Jonathan W. Westhouse, Karl Wette, John T. Whelan, Bernard F. Whiting, Chris Whittle, Dennis M. Wilken, Daniel Williams, Williams, Roy D., Andrew R. Williamson, Joshua L. Willis, Benno Willke, Walter Winkler, Christopher C. Wipf, Holger Wittel, Graham Woan, Janis Woehler, Jared K. Wofford, Chun-fung Wong, Jennifer L. Wright, David S. Wu, Daniel M. Wysocki, Liting Xiao, Hiro Yamamoto, Le Yang, Yang Yang, Ziyan Yang, Min-jet J. Yap, Maher Yazback, David W. Yeeles, Hang Yu, Haocun Yu, Shingheirobin Yuen, Adam K. Zadrożny, Adam Zadrożny, Michele Zanolin, Tatiana Zelenova, Jean-pierre Zendri, Michael Zevin, Jue Zhang, Liyuan Zhang, Teng Zhang, Chunnong Zhao, Guoying Zhao, Minchuan Zhou, Zifan Zhou, Xingjiang J. Zhu, Aaron B. Zimmerman, Michael E. Zucker, and John Zweizig
Published: 2021
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23 results on '"Doğa Veske"'

1. Probing the dark Solar system: detecting binary asteroids with a space-based interferometric asteroid explorer

2. Swift Follow-up Observations of Gravitational-wave and High-energy Neutrino Coincident Signals

3. Multi-messenger Emission from Tidal Waves in Neutron Star Oceans

4. Generalized approach to matched filtering using neural networks

5. An Archival Search for Very-High-Energy Counterparts to Sub-Threshold Neutron-Star Merger Candidates

6. Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs

7. All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

8. Characterizing the observation bias in gravitational-wave detections and finding structured population properties

9. Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars

10. The IceCube Pie Chart: Relative Source Contributions to the Cosmic Neutrino Flux

11. Have hierarchical three-body mergers been detected by LIGO/Virgo?

12. GW190521: A Binary Black Hole Merger with a Total Mass of 150 M⊙

13. Neutrino emission upper limits with maximum likelihood estimators for joint astrophysical neutrino searches with large sky localizations

14. Search for Black Hole Merger Families

15. GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

16. Constraining Black Hole Populations in Globular Clusters using Microlensing: Application to Omega Centauri

17. Bayesian multimessenger search method for common sources of gravitational waves and high-energy neutrinos

18. Multi-messenger Gravitational-Wave + High-Energy Neutrino Searches with LIGO, Virgo and IceCube

19. An Archival Search for Neutron-star Mergers in Gravitational Waves and Very-high-energy Gamma Rays

20. How to Search for Multiple Messengers—A General Framework Beyond Two Messengers

21. Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?

22. Pretest setup installation of the METU-DBL project to perform space radiation tests

23. Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo

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