In-flight calibration of the Hitomi Soft X-ray Spectrometer. (2) Point spread function-Reference-Cited by-同舟云学术

In-flight calibration of the Hitomi Soft X-ray Spectrometer. (2) Point spread function

Published:2018-03-01 Issue:2 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Maeda Yoshitomo¹²,Sato Toshiki³,Hayashi Takayuki⁴⁵,Iizuka Ryo¹,Angelini Lorella⁴,Asai Ryota³,Furuzawa Akihiro⁶,Kelley Richard⁴⁷,Koyama Shu¹,Kurashima Sho³,Ishida Manabu¹²,Mori Hideyuki⁴,Nakaniwa Nozomi³,Okajima Takashi⁴,Serlemitsos Peter J⁴,Tsujimoto Masahiro¹,Yaqoob Tahir⁴⁷

Affiliation:

1. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan

2. The Graduate University for Advanced Studies, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan

3. Tokyo Metropolitan University, 1-1 Minami-Osawa, Hachioji, Tokyo 192-0397, Japan

4. NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA

5. Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan

6. Fujita Health University, 1-98 Dengakugakubo, Kutsukake-cho, Toyoake, Aichi 470-1192, Japan

7. Department of Physics, University of Maryland Baltimore County, 1000 Hilltop Circle, MD 21250, USA

Funder

Japan Society for the Promotion of Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/2/19/24612313/psx146.pdf

Reference29 articles.

1. Astro-H/Hitomi data analysis, processing, and archive

2. Upgrade of the 30-m x-ray pencil beam line at the Institute of Space and Astronautical Science

3. The quiescent intracluster medium in the core of the Perseus cluster

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