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

Yoshitomo Maeda, Toshiki Sato, Takayuki Hayashi, Ryo Iizuka, Lorella Angelini, Ryota Asai, Akihiro Furuzawa, Richard Kelley, Shu Koyama, Sho Kurashima, Manabu Ishida, Hideyuki Mori, Nozomi Nakaniwa, Takashi Okajima, Peter J. Serlemitsos, Masahiro Tsujimoto, Tahir Yaqoob

研究成果: Article

1 引用 (Scopus)

抄録

We present results of inflight calibration of the point spread function of the Soft X-ray Telescope that focuses X-rays onto the pixel array of the Soft X-ray Spectrometer system. We make a full array image of a point-like source by extracting a pulsed component of the Crab nebula emission. Within the limited statistics afforded by an exposure time of only 6.9 ks and limited knowledge of the systematic uncertainties, we find that the raytracing model of 1.2 half-power-diameter is consistent with an image of the observed event distributions across pixels. The ratio between the Crab pulsar image and the raytracing shows scatter from pixel to pixel that is 40% or less in all except one pixel. The pixel-to-pixel ratio has a spread of 20%, on average, for the 15 edge pixels, with an averaged statistical error of 17% (1 σ). In the central 16 pixels, the corresponding ratio is 15% with an error of 6%.

元の言語English
記事番号psx146
ジャーナルPublications of the Astronomical Society of Japan
70
発行部数2
DOI
出版物ステータスPublished - 01-03-2018

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point spread functions
pixel
spectrometer
pixels
flight
spectrometers
calibration
x rays
crab
Crab nebula
crabs
pulsars
point sources
statistics
telescopes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

これを引用

Maeda, Y., Sato, T., Hayashi, T., Iizuka, R., Angelini, L., Asai, R., ... Yaqoob, T. (2018). In-flight calibration of the Hitomi Soft X-ray Spectrometer. (2) Point spread function. Publications of the Astronomical Society of Japan, 70(2), [psx146]. https://doi.org/10.1093/pasj/psx146
Maeda, Yoshitomo ; Sato, Toshiki ; Hayashi, Takayuki ; Iizuka, Ryo ; Angelini, Lorella ; Asai, Ryota ; Furuzawa, Akihiro ; Kelley, Richard ; Koyama, Shu ; Kurashima, Sho ; Ishida, Manabu ; Mori, Hideyuki ; Nakaniwa, Nozomi ; Okajima, Takashi ; Serlemitsos, Peter J. ; Tsujimoto, Masahiro ; Yaqoob, Tahir. / In-flight calibration of the Hitomi Soft X-ray Spectrometer. (2) Point spread function. :: Publications of the Astronomical Society of Japan. 2018 ; 巻 70, 番号 2.
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abstract = "We present results of inflight calibration of the point spread function of the Soft X-ray Telescope that focuses X-rays onto the pixel array of the Soft X-ray Spectrometer system. We make a full array image of a point-like source by extracting a pulsed component of the Crab nebula emission. Within the limited statistics afforded by an exposure time of only 6.9 ks and limited knowledge of the systematic uncertainties, we find that the raytracing model of 1.2 half-power-diameter is consistent with an image of the observed event distributions across pixels. The ratio between the Crab pulsar image and the raytracing shows scatter from pixel to pixel that is 40{\%} or less in all except one pixel. The pixel-to-pixel ratio has a spread of 20{\%}, on average, for the 15 edge pixels, with an averaged statistical error of 17{\%} (1 σ). In the central 16 pixels, the corresponding ratio is 15{\%} with an error of 6{\%}.",
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Maeda, Y, Sato, T, Hayashi, T, Iizuka, R, Angelini, L, Asai, R, Furuzawa, A, Kelley, R, Koyama, S, Kurashima, S, Ishida, M, Mori, H, Nakaniwa, N, Okajima, T, Serlemitsos, PJ, Tsujimoto, M & Yaqoob, T 2018, 'In-flight calibration of the Hitomi Soft X-ray Spectrometer. (2) Point spread function', Publications of the Astronomical Society of Japan, 巻. 70, 番号 2, psx146. https://doi.org/10.1093/pasj/psx146

In-flight calibration of the Hitomi Soft X-ray Spectrometer. (2) Point spread function. / Maeda, Yoshitomo; Sato, Toshiki; Hayashi, Takayuki; Iizuka, Ryo; Angelini, Lorella; Asai, Ryota; Furuzawa, Akihiro; Kelley, Richard; Koyama, Shu; Kurashima, Sho; Ishida, Manabu; Mori, Hideyuki; Nakaniwa, Nozomi; Okajima, Takashi; Serlemitsos, Peter J.; Tsujimoto, Masahiro; Yaqoob, Tahir.

:: Publications of the Astronomical Society of Japan, 巻 70, 番号 2, psx146, 01.03.2018.

研究成果: Article

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T1 - In-flight calibration of the Hitomi Soft X-ray Spectrometer. (2) Point spread function

AU - Maeda, Yoshitomo

AU - Sato, Toshiki

AU - Hayashi, Takayuki

AU - Iizuka, Ryo

AU - Angelini, Lorella

AU - Asai, Ryota

AU - Furuzawa, Akihiro

AU - Kelley, Richard

AU - Koyama, Shu

AU - Kurashima, Sho

AU - Ishida, Manabu

AU - Mori, Hideyuki

AU - Nakaniwa, Nozomi

AU - Okajima, Takashi

AU - Serlemitsos, Peter J.

AU - Tsujimoto, Masahiro

AU - Yaqoob, Tahir

PY - 2018/3/1

Y1 - 2018/3/1

N2 - We present results of inflight calibration of the point spread function of the Soft X-ray Telescope that focuses X-rays onto the pixel array of the Soft X-ray Spectrometer system. We make a full array image of a point-like source by extracting a pulsed component of the Crab nebula emission. Within the limited statistics afforded by an exposure time of only 6.9 ks and limited knowledge of the systematic uncertainties, we find that the raytracing model of 1.2 half-power-diameter is consistent with an image of the observed event distributions across pixels. The ratio between the Crab pulsar image and the raytracing shows scatter from pixel to pixel that is 40% or less in all except one pixel. The pixel-to-pixel ratio has a spread of 20%, on average, for the 15 edge pixels, with an averaged statistical error of 17% (1 σ). In the central 16 pixels, the corresponding ratio is 15% with an error of 6%.

AB - We present results of inflight calibration of the point spread function of the Soft X-ray Telescope that focuses X-rays onto the pixel array of the Soft X-ray Spectrometer system. We make a full array image of a point-like source by extracting a pulsed component of the Crab nebula emission. Within the limited statistics afforded by an exposure time of only 6.9 ks and limited knowledge of the systematic uncertainties, we find that the raytracing model of 1.2 half-power-diameter is consistent with an image of the observed event distributions across pixels. The ratio between the Crab pulsar image and the raytracing shows scatter from pixel to pixel that is 40% or less in all except one pixel. The pixel-to-pixel ratio has a spread of 20%, on average, for the 15 edge pixels, with an averaged statistical error of 17% (1 σ). In the central 16 pixels, the corresponding ratio is 15% with an error of 6%.

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