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13 results on '"Chiu, I-Non"'

2. Groups and Protocluster Candidates in the CLAUDS and HSC-SSP Joint Deep Surveys

Author

Li, Qingyang, primary, Yang, Xiaohu, additional, Liu, Chengze, additional, Jing, Yipeng, additional, He, Min, additional, Huang, Jia-Sheng, additional, Dai, Y. Sophia, additional, Sawicki, Marcin, additional, Arnouts, Stephane, additional, Gwyn, Stephen, additional, Moutard, Thibaud, additional, Mo, H. J., additional, Wang, Kai, additional, Katsianis, Antonios, additional, Cui, Weiguang, additional, Han, Jiaxin, additional, Chiu, I-Non, additional, Gu, Yizhou, additional, and Xu, Haojie, additional

Published
2022
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4. Weak-lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data

Author

Umetsu, Keiichi, primary, Sereno, Mauro, additional, Lieu, Maggie, additional, Miyatake, Hironao, additional, Medezinski, Elinor, additional, Nishizawa, Atsushi J., additional, Giles, Paul, additional, Gastaldello, Fabio, additional, McCarthy, Ian G., additional, Kilbinger, Martin, additional, Birkinshaw, Mark, additional, Ettori, Stefano, additional, Okabe, Nobuhiro, additional, Chiu, I-Non, additional, Coupon, Jean, additional, Eckert, Dominique, additional, Fujita, Yutaka, additional, Higuchi, Yuichi, additional, Koulouridis, Elias, additional, Maughan, Ben, additional, Miyazaki, Satoshi, additional, Oguri, Masamune, additional, Pacaud, Florian, additional, Pierre, Marguerite, additional, Rapetti, David, additional, and Smith, Graham P., additional

Published
2020
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5. X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton

Author

Bulbul, Esra, primary, Chiu, I-Non, additional, Mohr, Joseph J., additional, McDonald, Michael, additional, Benson, Bradford, additional, Bautz, Mark W., additional, Bayliss, Matthew, additional, Bleem, Lindsey, additional, Brodwin, Mark, additional, Bocquet, Sebastian, additional, Capasso, Raffaella, additional, Dietrich, Jörg P., additional, Forman, Bill, additional, Hlavacek-Larrondo, Julie, additional, Holzapfel, W. L., additional, Khullar, Gourav, additional, Klein, Matthias, additional, Kraft, Ralph, additional, Miller, Eric D., additional, Reichardt, Christian, additional, Saro, Alex, additional, Sharon, Keren, additional, Stalder, Brian, additional, Schrabback, Tim, additional, and Stanford, Adam, additional

Published
2019
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7. The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters

Author

Umetsu, Keiichi, primary, Sereno, Mauro, additional, Tam, Sut-Ieng, additional, Chiu, I-Non, additional, Fan, Zuhui, additional, Ettori, Stefano, additional, Gruen, Daniel, additional, Okumura, Teppei, additional, Medezinski, Elinor, additional, Donahue, Megan, additional, Meneghetti, Massimo, additional, Frye, Brenda, additional, Koekemoer, Anton, additional, Broadhurst, Tom, additional, Zitrin, Adi, additional, Balestra, Italo, additional, Benítez, Narciso, additional, Higuchi, Yuichi, additional, Melchior, Peter, additional, Mercurio, Amata, additional, Merten, Julian, additional, Molino, Alberto, additional, Nonino, Mario, additional, Postman, Marc, additional, Rosati, Piero, additional, Sayers, Jack, additional, and Seitz, Stella, additional

Published
2018
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9. First Results on the Cluster Galaxy Population from the Subaru Hyper Suprime-Cam Survey. III. Brightest Cluster Galaxies, Stellar Mass Distribution, and Active Galaxies

Author

Lin, Yen-Ting, primary, Hsieh, Bau-Ching, additional, Lin, Sheng-Chieh, additional, Oguri, Masamune, additional, Chen, Kai-Feng, additional, Tanaka, Masayuki, additional, Chiu, I-Non, additional, Huang, Song, additional, Kodama, Tadayuki, additional, Leauthaud, Alexie, additional, More, Surhud, additional, Nishizawa, Atsushi J., additional, Bundy, Kevin, additional, Lin, Lihwai, additional, and Miyazaki, Satoshi, additional

Published
2017
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10. Velocity Segregation and Systematic Biases in Velocity Dispersion Estimates with the SPT-GMOS Spectroscopic Survey

Author

Bayliss, Matthew. B., primary, Zengo, Kyle, additional, Ruel, Jonathan, additional, Benson, Bradford A., additional, Bleem, Lindsey E., additional, Bocquet, Sebastian, additional, Bulbul, Esra, additional, Brodwin, Mark, additional, Capasso, Raffaella, additional, Chiu, I-non, additional, McDonald, Michael, additional, Rapetti, David, additional, Saro, Alex, additional, Stalder, Brian, additional, Stark, Antony A., additional, Strazzullo, Veronica, additional, Stubbs, Christopher W., additional, and Zenteno, Alfredo, additional

Published
2017
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13. X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton

Author

Matthias Klein, Bill Forman, W. L. Holzapfel, Tim Schrabback, B. Stalder, Sebastian Bocquet, Mark W. Bautz, Mark Brodwin, Christian L. Reichardt, Eric D. Miller, Michael McDonald, Matthew B. Bayliss, A. Saro, Lindsey Bleem, R. Capasso, G. Khullar, Joseph J. Mohr, Ralph P. Kraft, I-Non Chiu, Keren Sharon, Esra Bulbul, Julie Hlavacek-Larrondo, J. P. Dietrich, Adam Stanford, Bradford Benson, Bulbul, Esra, Chiu, I. -Non, Mohr, Joseph J., Mcdonald, Michael, Benson, Bradford, Bautz, Mark W., Bayliss, Matthew, Bleem, Lindsey, Brodwin, Mark, Bocquet, Sebastian, Capasso, Raffaella, Dietrich, Jörg P., Forman, Bill, Hlavacek-Larrondo, Julie, Holzapfel, W. L., Khullar, Gourav, Klein, Matthia, Kraft, Ralph, Miller, Eric D., Reichardt, Christian, Saro, Alex, Sharon, Keren, Stalder, Brian, Schrabback, Tim, and Stanford, Adam

Subjects
large-scale structure of universe, Physics, X-rays: galaxies: clusters, Astrophysics - Cosmology and Nongalactic Astrophysics, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Halo mass function, Astronomy and Astrophysics, Observable, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Redshift, galaxies: cluster [X-rays], Luminosity, South Pole Telescope, Space and Planetary Science, 0103 physical sciences, Halo, 010303 astronomy & astrophysics, Scaling, Astrophysics::Galaxy Astrophysics, Galaxy cluster, 0105 earth and related environmental sciences
Abstract

We present measurements of the X-ray observables of the intra-cluster medium (ICM), including luminosity $L_X$, ICM mass $M_{ICM}$, emission-weighted mean temperature $T_X$, and integrated pressure $Y_X$, that are derived from XMM-Newton X-ray observations of a Sunyaev-Zel'dovich Effect (SZE) selected sample of 59 galaxy clusters from the South Pole Telescope SPT-SZ survey that span the redshift range of $0.20 < z < 1.5$. We constrain the best-fit power law scaling relations between X-ray observables, redshift, and halo mass. The halo masses are estimated based on previously published SZE observable to mass scaling relations, calibrated using information that includes the halo mass function. Employing SZE-based masses in this sample enables us to constrain these scaling relations for massive galaxy clusters ($M_{500}\geq 3 \times10^{14}$ $M_\odot$) to the highest redshifts where these clusters exist without concern for X-ray selection biases. We find that the mass trends are steeper than self-similarity in all cases, and with $\geq 2.5{\sigma}$ significance in the case of $L_X$ and $M_{ICM}$. The redshift trends are consistent with the self-similar expectation, but the uncertainties remain large. Core-included scaling relations tend to have steeper mass trends for $L_X$. There is no convincing evidence for a redshift-dependent mass trend in any observable. The constraints on the amplitudes of the fitted scaling relations are currently limited by the systematic uncertainties on the SZE-based halo masses, however the redshift and mass trends are limited by the X-ray sample size and the measurement uncertainties of the X-ray observables., Comment: Accepted for publication in ApJ. 29 pages, 11 figures, 5 tables

Published
2019
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