S
Stephen S. Holt
Researcher at Franklin W. Olin College of Engineering
Publications - 139
Citations - 6909
Stephen S. Holt is an academic researcher from Franklin W. Olin College of Engineering. The author has contributed to research in topics: Luminosity & Supernova remnant. The author has an hindex of 38, co-authored 139 publications receiving 6694 citations. Previous affiliations of Stephen S. Holt include Goddard Space Flight Center.
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The X-Ray Observatory Suzaku
Kazuhisa Mitsuda,Mark W. Bautz,Hajime Inoue,Richard L. Kelley,Katsuji Koyama,Hideyo Kunieda,Kazuo Makishima,Yoshiaki Ogawara,Robert Petre,Tadayuk Takahashi,Hiroshi Tsunemi,Nicholas E. White,Naohisa Anabuki,Lorella Angelini,Keith A. Arnaud,Hisamitsu Awaki,Aya Bamba,Kevin R. Boyce,Gregory V. Brown,Kai Wing Chan,Jean Cottam,Tadayasu Dotani,John P. Doty,Ken Ebisawa,Yuichiro Ezoe,Andrew C. Fabian,Enectali Figueroa,Ryuichi Fujimoto,Yasushi Fukazawa,Tae Furusho,Akihiro Furuzawa,Keith C. Gendreau,Richard E. Griffiths,Yoshito Haba,Kenji Hamaguchi,Ilana M. Harrus,Günther Hasinger,Isamu Hatsukade,Kiyoshi Hayashida,Patrick Henry,Junko S. Hiraga,Stephen S. Holt,Ann Hornschemeier,John P. Hughes,Una Hwang,Manabu Ishida,Yoshitaka Ishisaki,Naoki Isobe,Masayuki Itoh,Naoko Iyomoto,Steven M. Kahn,Tuneyoshi Kamae,Hideaki Katagiri,Jun Kataoka,Haruyoshi Katayama,Nobuyuki Kawai,Caroline Kllbourne,Kenzo Kinugasa,Steve Klssel,Shunji Kitamoto,Mitsuhiro Kohama,Takayoshi Kohmura,Motohide Kokubun,Taro Kotani,J. Kotoku,Aya Kubota,Greg Madejski,Yoshitomo Maeda,Fumiyoshi Makino,Alex Markowitz,Chiho Matsumoto,Hironori Matsumoto,Masaru Matsuoka,Kyoko Matsushita,Dan McCammon,Tatehiko Mihara,Kazutami Misakl,Emi Miyata,Tsunefumi Mizuno,Koji Mori,Hideyuki Mori,Mikio Morii,Harvey Moseley,Koji Mukai,Hiroshi Murakami,Toshio Murakami,Richard Mushotzky,Fumiaki Nagase,M. Namiki,Hitoshi Negoro,Kazuhiro Nakazawa,John A. Nousek,Takashi Okajima,Yasushi Ogasaka,Takaya Ohashi,T. Oshima,Naomi Ota,Masanobu Ozaki,H. Ozawa,Arvind Parmar,W. D. Pence,F. Scott Porter,James Reeves,George R. Ricker,Ikuya Sakurai,Wilton T. Sanders,Atsushi Senda,Peter J. Serlemitsos,Ryo Shibata,Yang Soong,Randall K. Smith,Motoko Suzuki,Andrew Szymkowiak,Hiromitsu Takahashi,Toru Tamagawa,Keisuke Tamura,Takayuki Tamura,Yasuo Tanaka,Makoto Tashiro,Yuzuru Tawara,Yukikatsu Terada,Yuichi Terashima,Hiroshi Tomida,Ken'ichi Torii,Yohko Tsuboi,Masahiro Tsujimoto,Takeshi Go Tsuru,Martin J. L. Turner,Yoshihiro Ueda,Shiro Ueno,M. Ueno,Shin'ichiro Uno,Yuji Urata,Shin Watanabe,Norimasa Yamamoto,Kazutaka Yamaoka,Noriko Y. Yamasaki,Koujun Yamashita,Makoto Yamauchi,Shigeo Yamauchi,Tahir Yaqoob,Daisuke Yonetoku,Atsumasa Yoshida +142 more
TL;DR: In this paper, the authors summarized the spacecraft, in-orbit performance, operations, and data processing that are related to observations of the Suzaku X-ray observatory, including high-sensitivity wide-band Xray spectroscopy.
Journal ArticleDOI
Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006
Katsuji Koyama,Robert Petre,Eric V. Gotthelf,Eric V. Gotthelf,Una Hwang,M. Matsuura,M. Ozaki,Stephen S. Holt +7 more
TL;DR: In this paper, X-ray observations of the remnant of supernova 1006, made by the ASCA satellite, indicate that emission from the edges of the supernova remnant shell is dominated by radiation from electrons accelerated to energies of ~ 100 TeV within the shock front.
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Accretion powered X-ray pulsars
TL;DR: In this article, a unified description of the properties of 14 X-ray pulsars is presented and compared with the current theoretical understanding of these systems, with the only trend in the phase averaged spectra being that the lower luminosity systems appear to have less abrupt high energy cutoffs.
Journal ArticleDOI
A complete X-ray sample of the high-latitude /absolute value of b greater than 20 deg/ sky from HEAO 1 A-2 - Log N-log S and luminosity functions
G. Piccinotti,Richard Mushotzky,Elihu Boldt,Stephen S. Holt,F. E. Marshall,Peter J. Serlemitsos,Rick Shafer +6 more
TL;DR: An all-sky survey of X-ray sources was performed, complete to a limiting sensitivity of 3.1 x 10 to the -11 ergs/sq cm/s in the 2-10 keV band.
Journal ArticleDOI
The Einstein /HEAO 2/ X-ray Observatory
Riccardo Giacconi,G. Branduardi,Ulrich G. Briel,A. Epstein,Daniel G. Fabricant,E. D. Feigelson,William R. Forman,Paul Gorenstein,J. E. Grindlay,H. Gursky,F. R. Harnden,J. P. Henry,C. Jones,E. M. Kellogg,D. Koch,S. S. Murray,Ethan J. Schreier,F. D. Seward,Harvey Tananbaum,K. Topka,L. van Speybroeck,Stephen S. Holt,Robert H. Becker,Elihu Boldt,Peter J. Serlemitsos,George W. Clark,Claude R. Canizares,Thomas H. Markert,Robert Novick,D. J. Helfand,Knox S. Long +30 more
TL;DR: The Einstein X-ray Observatory (HEAO 2) as mentioned in this paper is a fully imaging focusing Xray telescope with an angular resolution of a few arc sec, a field of view of up to one deg, and a sensitivity several hundred times greater than previously available in any Xray astronomy experiment.