The X-Ray Telescope onboard Suzaku

By P. Serlemitsos, Y. Soong, Kai-wing Chan, T. Okajima, J. Lehan, Y. Maeda, K. Itoh, H. Mori, R. Iizuka, A. Itoh and 24 more. 2007

436 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Radiation

View Paper: https://www.semanticscholar.org/paper/3b4c552c4a6eaff1bb7fcb2dea1477663b007bba

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In Astronomy and Astrophysics

1. J. Redondo
2. Igor G. Irastorza
3. A. Ringwald
4. K. Saikawa
5. G. Raffelt
6. A. Lindner
7. D. Horns
8. J. Jaeckel

In Radiation

1. F. Avignone
2. T. Yaqoob
3. Mattias Marklund
4. Padma Kant Shukla

Citations in the corpus

• Energy spectra of the soft X-ray diffuse emission in fourteen fields observed with Suzaku (2009, background): “By virtue of the good energy response function of the CCD camera (Koyama et al. 2007) and the high sensitivity when combined with the X-ray mirror (Serlemitsos et al. 2007), we clearly detected Ovii emission from all the fields, and Oviii emission from most of them.”
• The X-Ray Observatory Suzaku (2007, neutral): “Please see Serlemitsos et al. (2007) for details.”
• The nature of the Compton-thick X-ray reprocessor in NGC 4945 (2012, background): “Each XIS consists of four CCD detectors at the focal plane of its own thin-foil X-ray telescope (XRT – Serlemitsos et al. 2007), and has a field-of-view (FOV) of 17.8′ × 17.8′.”
• THE CONSTANT INNER-DISK RADIUS OF LMC X-3: A BASIS FOR MEASURING BLACK HOLE SPIN (2010, neutral): “(1) Serlemitsos et al. 2007; (2) http://heasarc.gsfc.nasa.gov/docs/ suzaku/prop_tools/suzaku_td.html; (3) Godet et al. 2009; (4) Guainazzi et al. 2009; (5) Stuhlinger et al. 2006; (6) I. de la Calle 2009, private communication; (7) Fiore et al. 1999; (8) Makishima et al. 1996; (9) Ebisawa 1996;…”
• Conceptual design of the International Axion Observatory (IAXO) (2014, methodology): “Later missions that used the same approach included: ASCA [39], launched in 1993; SODART [40], completed in 1995 but never launched; InFocµs [41], a hard x-ray balloon-borne instrument flown in 2004; and Suzaku [42], launched in 2005.”
• Study of Nonthermal Emission from SNR RX J1713.7–3946 with Suzaku (2008, background): “The XIS consists of four X-ray CCD cameras which are located in the foci of X-ray telescopes (XRT; Serlemitsos et al. 2007).”
• Towards a new generation axion helioscope (2011, methodology): “Later missions that used the same approach included ASCA [98], launched in 1993, SODART [99], completed in 1995 but never launched, the hard x-ray, balloon-borne InFocµs [100], flown in 2004, Astro-E [101], destroyed on launch in 2000, and Suzaku [102], launched in 2005.”
• X-Ray Imaging Spectrometer (XIS) on Board Suzaku (2007, background): “The IA, combined with the XRT, covers an 18′ × 18′ region on the sky.”