Soft X-ray calibration for the NeXT X-ray Telescope

Yoshitomo Maeda; Takayuki Hayashi; Hideyuki Mori; Ryoko Nakamura; Takuro Satoh; Akiko Sekiguchi; Kentaro Someya; Kensuke Tamura; Manabu Ishida; Takeyuki Osawa; Takayuki Shirata; Masaki Suzuki; Yasushi Ogasaka; Akihiro Furuzawa; Yoshito Haba; Takuya Miyazawa; Hideyo Kunieda; Koujun Yamashita; Takashi Okajima

doi:10.1117/12.788652

Soft X-ray calibration for the NeXT X-ray Telescope

Yoshitomo Maeda, Takayuki Hayashi, Hideyuki Mori, Ryoko Nakamura, Takuro Satoh, Akiko Sekiguchi, Kentaro Someya, Kensuke Tamura, Manabu Ishida, Takeyuki Osawa, Takayuki Shirata, Masaki Suzuki, Yasushi Ogasaka, Akihiro Furuzawa, Yoshito Haba, Takuya Miyazawa, Hideyo Kunieda, Koujun Yamashita, Takashi Okajima

研究成果: Conference contribution

3 引用（Scopus）

抜粋

We present a plan on soft X-ray calibration for the New Exploration X-ray Telescope (NeXT). Two hard and two soft X-ray telescopes (HXTs/SXTs: see Ogasaka et al. 2008 in this volume) provide images up to 80 keV with a large effective area. Following to the Suzaku X-ray telescope, the mirrors on SXTs are tightly nested to maximize the aperture efficiency. To illuminate the mirrors at all, we plan to adopt a raster scan system using a pencil beam collimated from an X-ray generator. We summarize a current status of the soft X-ray ground calibration system at ISAS/JAXA. We also review the calibration of the Suzaku XRTs since the optics are very similar to the NeXT SXTs.

元の言語	English
ホスト出版物のタイトル	Space Telescopes and Instrumentation 2008
ホスト出版物のサブタイトル	Ultraviolet to Gamma Ray
巻	7011
DOI	https://doi.org/10.1117/12.788652
出版物ステータス	Published - 01-12-2008
外部発表	Yes
イベント	Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray - Marseille, France 継続期間: 23-06-2008 → 28-06-2008

Other

Other	Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray
国	France
市	Marseille
期間	23-06-08 → 28-06-08

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

文献にアクセス

10.1117/12.788652

フィンガープリント Soft X-ray calibration for the NeXT X-ray Telescope' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

これを引用

Maeda, Y., Hayashi, T., Mori, H., Nakamura, R., Satoh, T., Sekiguchi, A., Someya, K., Tamura, K., Ishida, M., Osawa, T., Shirata, T., Suzuki, M., Ogasaka, Y., Furuzawa, A., Haba, Y., Miyazawa, T., Kunieda, H., Yamashita, K., & Okajima, T. (2008). Soft X-ray calibration for the NeXT X-ray Telescope. ： Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray (巻 7011). [70112O] https://doi.org/10.1117/12.788652

Maeda, Yoshitomo ; Hayashi, Takayuki ; Mori, Hideyuki ; Nakamura, Ryoko ; Satoh, Takuro ; Sekiguchi, Akiko ; Someya, Kentaro ; Tamura, Kensuke ; Ishida, Manabu ; Osawa, Takeyuki ; Shirata, Takayuki ; Suzuki, Masaki ; Ogasaka, Yasushi ; Furuzawa, Akihiro ; Haba, Yoshito ; Miyazawa, Takuya ; Kunieda, Hideyo ; Yamashita, Koujun ; Okajima, Takashi. / Soft X-ray calibration for the NeXT X-ray Telescope. Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. 巻 7011 2008.

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title = "Soft X-ray calibration for the NeXT X-ray Telescope",

abstract = "We present a plan on soft X-ray calibration for the New Exploration X-ray Telescope (NeXT). Two hard and two soft X-ray telescopes (HXTs/SXTs: see Ogasaka et al. 2008 in this volume) provide images up to 80 keV with a large effective area. Following to the Suzaku X-ray telescope, the mirrors on SXTs are tightly nested to maximize the aperture efficiency. To illuminate the mirrors at all, we plan to adopt a raster scan system using a pencil beam collimated from an X-ray generator. We summarize a current status of the soft X-ray ground calibration system at ISAS/JAXA. We also review the calibration of the Suzaku XRTs since the optics are very similar to the NeXT SXTs.",

author = "Yoshitomo Maeda and Takayuki Hayashi and Hideyuki Mori and Ryoko Nakamura and Takuro Satoh and Akiko Sekiguchi and Kentaro Someya and Kensuke Tamura and Manabu Ishida and Takeyuki Osawa and Takayuki Shirata and Masaki Suzuki and Yasushi Ogasaka and Akihiro Furuzawa and Yoshito Haba and Takuya Miyazawa and Hideyo Kunieda and Koujun Yamashita and Takashi Okajima",

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doi = "10.1117/12.788652",

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Maeda, Y, Hayashi, T, Mori, H, Nakamura, R, Satoh, T, Sekiguchi, A, Someya, K, Tamura, K, Ishida, M, Osawa, T, Shirata, T, Suzuki, M, Ogasaka, Y, Furuzawa, A, Haba, Y, Miyazawa, T, Kunieda, H, Yamashita, K & Okajima, T 2008, Soft X-ray calibration for the NeXT X-ray Telescope. ： Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. 巻. 7011, 70112O, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, Marseille, France, 23-06-08. https://doi.org/10.1117/12.788652

Soft X-ray calibration for the NeXT X-ray Telescope. / Maeda, Yoshitomo; Hayashi, Takayuki; Mori, Hideyuki; Nakamura, Ryoko; Satoh, Takuro; Sekiguchi, Akiko; Someya, Kentaro; Tamura, Kensuke; Ishida, Manabu; Osawa, Takeyuki; Shirata, Takayuki; Suzuki, Masaki; Ogasaka, Yasushi; Furuzawa, Akihiro; Haba, Yoshito; Miyazawa, Takuya; Kunieda, Hideyo; Yamashita, Koujun; Okajima, Takashi.

Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. 巻 7011 2008. 70112O.

研究成果: Conference contribution

TY - GEN

T1 - Soft X-ray calibration for the NeXT X-ray Telescope

AU - Maeda, Yoshitomo

AU - Hayashi, Takayuki

AU - Mori, Hideyuki

AU - Nakamura, Ryoko

AU - Satoh, Takuro

AU - Sekiguchi, Akiko

AU - Someya, Kentaro

AU - Tamura, Kensuke

AU - Ishida, Manabu

AU - Osawa, Takeyuki

AU - Shirata, Takayuki

AU - Suzuki, Masaki

AU - Ogasaka, Yasushi

AU - Furuzawa, Akihiro

AU - Haba, Yoshito

AU - Miyazawa, Takuya

AU - Kunieda, Hideyo

AU - Yamashita, Koujun

AU - Okajima, Takashi

PY - 2008/12/1

Y1 - 2008/12/1

N2 - We present a plan on soft X-ray calibration for the New Exploration X-ray Telescope (NeXT). Two hard and two soft X-ray telescopes (HXTs/SXTs: see Ogasaka et al. 2008 in this volume) provide images up to 80 keV with a large effective area. Following to the Suzaku X-ray telescope, the mirrors on SXTs are tightly nested to maximize the aperture efficiency. To illuminate the mirrors at all, we plan to adopt a raster scan system using a pencil beam collimated from an X-ray generator. We summarize a current status of the soft X-ray ground calibration system at ISAS/JAXA. We also review the calibration of the Suzaku XRTs since the optics are very similar to the NeXT SXTs.

AB - We present a plan on soft X-ray calibration for the New Exploration X-ray Telescope (NeXT). Two hard and two soft X-ray telescopes (HXTs/SXTs: see Ogasaka et al. 2008 in this volume) provide images up to 80 keV with a large effective area. Following to the Suzaku X-ray telescope, the mirrors on SXTs are tightly nested to maximize the aperture efficiency. To illuminate the mirrors at all, we plan to adopt a raster scan system using a pencil beam collimated from an X-ray generator. We summarize a current status of the soft X-ray ground calibration system at ISAS/JAXA. We also review the calibration of the Suzaku XRTs since the optics are very similar to the NeXT SXTs.

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Y2 - 23 June 2008 through 28 June 2008

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