E
Eric D. Miller
Researcher at Massachusetts Institute of Technology
Publications - 94
Citations - 5659
Eric D. Miller is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Galaxy cluster & Galaxy. The author has an hindex of 37, co-authored 94 publications receiving 5216 citations.
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Journal ArticleDOI
X-Ray Imaging Spectrometer (XIS) on Board Suzaku
Katsuji Koyama,Hiroshi Tsunemi,Tadayasu Dotani,Mark W. Bautz,Kiyoshi Hayashida,Takeshi Go Tsuru,Hironori Matsumoto,Yoshiaki Ogawara,George R. Ricker,John P. Doty,Steven E. Kissel,R. S. Foster,Hiroshi Nakajima,Hiroya Yamaguchi,Hideyuki Mori,Masaaki Sakano,Kenji Hamaguchi,Mamiko Nishiuchi,Emi Miyata,Ken'ichi Torii,M. Namiki,Satoru Katsuda,Daisuke Matsuura,Tomofumi Miyauchi,Naohisa Anabuki,Noriaki Tawa,Masanobu Ozaki,Hiroshi Murakami,Yoshitomo Maeda,Yoshinori Ichikawa,Gregory Y. Prigozhin,E. Boughan,Beverly LaMarr,Eric D. Miller,Barry E. Burke,J. A. Gregory,Allen D. Pillsbury,Aya Bamba,Junko S. Hiraga,Atsushi Senda,Haruyoshi Katayama,Shunji Kitamoto,Masahiro Tsujimoto,Takayoshi Kohmura,Yohko Tsuboi,Hisamitsu Awaki +45 more
TL;DR: The XIS is an X-ray imaging spectrometer system, consisting of state-of-the-art charge-coupled devices (CCDs) optimized for Xray detection, camera bodies, and control electronics as mentioned in this paper.
Journal ArticleDOI
Reproducibility of Non-X-ray Background for the X-ray Imaging Spectrometer aboard Suzaku
Noriaki Tawa,Kiyoshi Hayashida,Masaaki Nagai,Hajime Nakamoto,Hiroshi Tsunemi,Hiroya Yamaguchi,Yoshitaka Ishisaki,Eric D. Miller,Tsunefumi Mizuno,Tadayasu Dotani,Masanobu Ozaki,Haruyoshi Katayama +11 more
TL;DR: In this article, the authors constructed an X-ray non-X-ray background (NXB) database by collecting XIS events when the dark Earth covers the XIS FOV and found that the count rate of the NXB anti-correlates with the cut-off-rigidity and correlates with the PIN upper discriminator (PIN-UD).
Journal ArticleDOI
Reproducibility of Non-X-ray Background for the X-ray Imaging Spectrometer aboard Suzaku
Noriaki Tawa,Kiyoshi Hayashida,Masaaki Nagai,Hajime Nakamoto,Hiroshi Tsunemi,Hiroya Yamaguchi,Yoshitaka Ishisaki,Eric D. Miller,Tsunefumi Mizuno,Tadayasu Dotani,Masanobu Ozaki,Haruyoshi Katayama +11 more
TL;DR: In this paper, the authors constructed an X-ray non-X-ray background (NXB) database by collecting XIS events when the dark Earth covers the XIS FOV and found that the count rate of the NXB anti-correlates with the cut-off-rigidity and correlates with the PIN upper discriminator (PIN-UD).
Journal ArticleDOI
A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies
Michael McDonald,Matthew B. Bayliss,Bradford Benson,Ryan J. Foley,Jonathan Ruel,Peter Sullivan,Sylvain Veilleux,Sylvain Veilleux,K. A. Aird,M. L. N. Ashby,Marshall W. Bautz,G. Bazin,Lindsey Bleem,Mark Brodwin,John E. Carlstrom,C. L. Chang,C. L. Chang,H. M. Cho,Alejandro Clocchiatti,T. M. Crawford,A. T. Crites,T. de Haan,Shantanu Desai,Matt Dobbs,J. P. Dudley,Eiichi Egami,William R. Forman,Gordon P. Garmire,Elizabeth George,Michael D. Gladders,Anthony H. Gonzalez,N. W. Halverson,N. L. Harrington,F. W. High,Gilbert Holder,W. L. Holzapfel,S. Hoover,J. D. Hrubes,C. Jones,Marshall Joy,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Jiayi Liu,M. Lueker,M. Lueker,D. Luong-Van,Adam Mantz,Daniel P. Marrone,Jeff McMahon,Jeff McMahon,J. Mehl,S. S. Meyer,Eric D. Miller,L. M. Mocanu,Joseph J. Mohr,T. E. Montroy,S. S. Murray,T. Natoli,Stephen Padin,Stephen Padin,T. Plagge,C. Pryke,T. D. Rawle,Christian L. Reichardt,Armin Rest,M. Rex,J. E. Ruhl,Benjamin Saliwanchik,A. Saro,J. T. Sayre,K. K. Schaffer,K. K. Schaffer,L. Shaw,L. Shaw,Erik Shirokoff,Erik Shirokoff,Robert A. Simcoe,J. Song,Helmuth Spieler,B. Stalder,Z. K. Staniszewski,Antony A. Stark,K. T. Story,Christopher W. Stubbs,R. Šuhada,A. van Engelen,K. Vanderlinde,Joaquin Vieira,Joaquin Vieira,Alexey Vikhlinin,R. Williamson,Oliver Zahn,Oliver Zahn,A. Zenteno +96 more
TL;DR: An exceptionally luminous galaxy cluster that hosts an extremely strong cooling flow and a large star-formation rate implies that a significant fraction of the stars in the central galaxy of this cluster may form through accretion of the intracluster medium, rather than (as is currently thought) assembling entirely via mergers.
Journal ArticleDOI
THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 < z < 1.2 SELECTED FROM THE SPT-SZ SURVEY
Michael McDonald,Bradford Benson,Alexey Vikhlinin,B. Stalder,Lindsey Bleem,T. de Haan,Henry W. Lin,K. A. Aird,M. L. N. Ashby,Marshall W. Bautz,Matthew B. Bayliss,Sebastian Bocquet,Mark Brodwin,John E. Carlstrom,John E. Carlstrom,C. L. Chang,C. L. Chang,H. M. Cho,Alejandro Clocchiatti,T. M. Crawford,A. T. Crites,Shantanu Desai,M. A. Dobbs,J. P. Dudley,Ryan J. Foley,William R. Forman,Elizabeth George,D. Gettings,Michael D. Gladders,Anthony H. Gonzalez,N. W. Halverson,F. W. High,Gilbert Holder,W. L. Holzapfel,S. Hoover,J. D. Hrubes,C. Jones,Marshall Joy,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Jiayi Liu,M. Lueker,M. Lueker,D. Luong-Van,Adam Mantz,Daniel P. Marrone,Jeff McMahon,J. Mehl,J. Mehl,S. S. Meyer,Eric D. Miller,L. M. Mocanu,Joseph J. Mohr,T. E. Montroy,S. S. Murray,D. Nurgaliev,Stephen Padin,Stephen Padin,T. Plagge,C. Pryke,Christian L. Reichardt,Armin Rest,Jonathan Ruel,J. E. Ruhl,Benjamin Saliwanchik,A. Saro,J. T. Sayre,K. K. Schaffer,K. K. Schaffer,Erik Shirokoff,Erik Shirokoff,J. Song,R. Šuhada,Helmuth Spieler,S. A. Stanford,S. A. Stanford,Z. K. Staniszewski,Antony A. Stark,K. T. Story,A. van Engelen,K. Vanderlinde,Joaquin Vieira,Joaquin Vieira,R. Williamson,Oliver Zahn,Oliver Zahn,A. Zenteno +89 more
TL;DR: In this paper, Chandra X-ray observations of 83 high-redshift (0.3 0.5 ) galaxy clusters were used to study the cooling properties of galaxy clusters and showed that cool cores have been steadily growing over the 8 Gyr spanned by their sample, consistent with a constant cooling flow that is unable to cool below entropies of 10 keV cm^2 and, instead, accumulates in the cluster center.