In-Flight Calibration of Hitomi Soft X-Ray Spectrometer. (1) Background

The X-Ray Spectrometer (XRS) instrument of Suzaku provided the first measurement of the non-X-ray background (NXB) of an X-ray calorimeter spectrometer, but the data set was limited. The Soft X-ray Spectrometer (SXS) instrument of Hitomi was able to provide a more detailed picture of X-ray calorimet...

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Veröffentlicht in:Publications of the Astronomical Society of Japan 2018-03, Vol.70 (2)
Hauptverfasser: Kilbourne, Caroline A., Sawada, Makoto, Tsujimoto, Masahiro, Angelini, Lorella, Boyce, Kevin R., Eckart, Megan, Fujimoto, Ryuichi, Ishisaki, Yoshitaka, Kelley, Richard, Koyama, Shu, Leutenegger, Maurice A., Loewenstein, Michael, McCammon, Dan, Mitsuda, Kazuhisa, Nakashima, Shinya, Porter, Frederick S., Seta, Hiromi, Takei, Yoh, Tashiro, Makoto S., Terada, Yukikatsu, Yamada, Shinya, Yamasaki, Noriko Y.
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container_title Publications of the Astronomical Society of Japan
container_volume 70
creator Kilbourne, Caroline A.
Sawada, Makoto
Tsujimoto, Masahiro
Angelini, Lorella
Boyce, Kevin R.
Eckart, Megan
Fujimoto, Ryuichi
Ishisaki, Yoshitaka
Kelley, Richard
Koyama, Shu
Leutenegger, Maurice A.
Loewenstein, Michael
McCammon, Dan
Mitsuda, Kazuhisa
Nakashima, Shinya
Porter, Frederick S.
Seta, Hiromi
Takei, Yoh
Tashiro, Makoto S.
Terada, Yukikatsu
Yamada, Shinya
Yamasaki, Noriko Y.
description The X-Ray Spectrometer (XRS) instrument of Suzaku provided the first measurement of the non-X-ray background (NXB) of an X-ray calorimeter spectrometer, but the data set was limited. The Soft X-ray Spectrometer (SXS) instrument of Hitomi was able to provide a more detailed picture of X-ray calorimeter background, with more than 360 ks of data while pointed at the Earth, and a comparable amount of blank-sky data. These data are important not only for analyzing SXS science data, but also for categorizing the contributions to the NXB in X-ray calorimeters as a class. In this paper, we present the contributions to the SXS NXB, the types and effectiveness of the screening, the interaction of the screening with the broad-band redistribution, and the residual background spectrum as a function of magnetic cut-off rigidity. The orbit-averaged SXS NXB in the range 0.3-12 keV was 4 × 10(exp −2) counts s(exp −1) -sq cm. This very low background in combination with groundbreaking spectral resolution gave SXS unprecedented sensitivity to weak spectral lines.
doi_str_mv 10.1093/pasj/psx139
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source Oxford University Press Journals All Titles (1996-Current); Freely Accessible Japanese Titles; NASA Technical Reports Server
subjects Instrumentation And Photography
title In-Flight Calibration of Hitomi Soft X-Ray Spectrometer. (1) Background
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