X-Ray Imaging Spectrometer (XIS) on Board Suzaku

By K. Koyama, H. Tsunemi, T. Dotani, M. Bautz, K. Hayashida, T. Tsuru, H. Matsumoto, Y. Ogawara, G. Ricker, J. Doty and 36 more. 2007

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Citations in the corpus

Black hole accretion discs in the canonical low‐hard state (2009, methodology): “The three operating detectors constituting the X-ray Imaging Spectrometer (XIS; Koyama et al. 2007) were operated in the ‘burst’ clock mode in both observations and employed the ‘1/4 window’ mode.”
Study of Nonthermal Emission from SNR RX J1713.7–3946 with Suzaku (2008, background): “This is because the contamination on the optical blocking filters of the XIS (Koyama et al. 2007) significantly changed the detector response to lowenergy X-rays between 2005 and 2006.”
On why the iron K-shell absorption in AGN is not a signature of the local warm/hot intergalactic medium (2008, methodology): “In this paper we discuss data taken with the 4 XIS (X-ray Imaging Spectrometer; Koyama et al. 2007) CCDs. Events files from official version 2.0 of the Suzaku pipeline processing were used.”
Suzaku Observations of Active Galactic Nuclei Detected in the Swift BAT Survey: Discovery of a “New Type” of Buried Supermassive Black Holes (2007, methodology): “Suzaku, the 5th Japanese X-ray satellite, carries four sets of X-ray mirrors each with a focal plane X-ray CCD camera, the X-ray Imaging Spectrometer (XIS-0, XIS-1, XIS-2, and XIS-3; Koyama et al. 2007), and a non-imaging instrument called the Hard X-ray Detector (HXD; Takahashi et al. 2007), which ”
FERMI LARGE AREA TELESCOPE VIEW OF THE CORE OF THE RADIO GALAXY CENTAURUS A (2010, methodology): “Data were taken with two instruments on the255 Swift spacecraft (Gehrels et al. 2004) and two instruments on the Suzaku spacecraft (Mitsuda et al.256 2007; Koyama et al. 2007; Takahashi et al. 2007).”
BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog (2017, methodology): “Suzaku Suzaku (Mitsuda et al. 2007) X-ray Imaging Spectrometer (XIS, Koyama et al. 2007) data were used to complement Swift/BAT spectra for ten source.”
An absorption origin for the X-ray spectral variability of MCG-6-30-15 (2008, methodology): “In the subsequent analysis, the flux has been decreased by a factor 1.09 to be consistent for observations at the pointing position with the cross-calibration study of Koyama et al. (2007), revised for theSuzaku revision 2 analysis pipeline.1”
DISCOVERY OF ULTRA-FAST OUTFLOWS IN A SAMPLE OF BROAD-LINE RADIO GALAXIES OBSERVED WITH SUZAKU (2010, methodology): “The data were taken from the X-ray Imaging Spectrometer (XIS, Koyama et al. 2007) and processed using v2 of the Suzaku pipeline.”
The nature of the Compton-thick X-ray reprocessor in NGC 4945 (2012, background): “Residual uncertainties in the XIS energy scale are on the order of 0.2% or less (or ∼ 13 eV at 6.4 keV – see Koyama et al. 2007).”