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The X-Ray Observatory Suzaku
High-sensitivity wide-band X-ray spectroscopy is the key feature of the Suzaku X-ray observatory, launched on 2005 July 10. This paper summarizes the spacecraft, in-orbit performance, operations, andExpand
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The synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era
We present a detailed and self-consistent modeling of the cosmic X-ray background (XRB) based on the most up-to-date X-ray luminosity functions (XLF) and evolution of Active Galactic Nuclei (AGN).Expand
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The Chandra COSMOS Survey. I. Overview and Point Source Catalog
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central 0.5 deg^2 of the COSMOS field (centered at 10 ^h , +02 ^o ) with an effective exposure of ~160 ks,Expand
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The Pan-STARRS1 Database and Data Products
This paper describes the organization of the database and the catalog data products from the Pan-STARRS1 $3\pi$ Steradian Survey. The catalog data products are available in the form of an SQL-basedExpand
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The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM-Newton deep fields
We extend our earlier work on X-ray source stacking in the deep XMM-Newton observation of the Lockman Hole, to the 2-Ms Chandra Deep Field North (CDF-N) and the 1-Ms Chandra Deep Field South (CDF-S).Expand
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The AGN contribution to mid-infrared surveys. X-ray counterparts of the mid-IR sources in the Lockman Hole and HDF-N
We provide constraints on the AGN contribution to the mid-IR extragalactic background light from a correlation analysis of deep X-ray and mid-IR observations in two regions centred on the LockmanExpand
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The X-Ray Spectrum of Supernova Remnant 1987A
We discuss the X-ray emission observed from supernova remnant 1987A with the Chandra X-Ray Observatory. We analyze a high-resolution spectrum obtained in 1999 October with the high-energyExpand
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The ROSAT Deep Survey I. X-ray sources in the Lockman Field
The ROSAT Deep Survey in the Lockman Hole is the most sensitive X-ray survey performed to date, encompassing an exposure time of 207 ksec with the PSPC and a total of 1.32 Msec with the HRI aboardExpand
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Xmm-newton observation of a distant x-ray selected cluster of galaxies at z=1.26 with possible cluster interaction
We report on the XMM-Newton observation of RX J1053.7+5735, one of the most distant $(z = 1.26)$ selected clusters of galaxies, which also shows an unusual double-lobed X-ray morphology, indicativeExpand
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