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Chandra and XMM-Newton Observations of RDCS 1252.9-2927, A Massive Cluster at z=1.24
DOI: 10.1086/379857 Bibcode: 2004AJ....127..230R

Demarco, R.; Lidman, C.; Tozzi, P. +10 more

We present deep Chandra and XMM-Newton observations of the galaxy cluster RDCS 1252.9-2927, which was selected from the ROSAT Deep Cluster Survey (RDCS) and confirmed by extensive spectroscopy with the Very Large Telescope at redshift z=1.237. With the Chandra data, the X-ray emission from the intracluster medium is well resolved and traced out to…

2004 The Astronomical Journal
XMM-Newton 122
X-ray-Underluminous Active Galactic Nuclei Relative to Broad Emission Lines in Ultraluminous Infrared Galaxies
DOI: 10.1086/381069 Bibcode: 2004AJ....127..758I

Imanishi, Masatoshi; Terashima, Yuichi

We present X-ray spectra of four ultraluminous infrared galaxies (ULIRGs) with detectable broad near-infrared emission lines produced by active galactic nuclei (AGNs): Mrk 463, PKS 1345+12, IRAS 05189-2524, and IRAS 07598+6508. With the exception of IRAS 07598+6508, high-quality X-ray spectra obtained with XMM or Chandra show modest (30-340 eV) eq…

2004 The Astronomical Journal
XMM-Newton 39
Markarian 1239: A Highly Polarized Narrow-Line Seyfert 1 Galaxy with a Steep X-Ray Spectrum and Strong Ne IX Emission
DOI: 10.1086/421002 Bibcode: 2004AJ....127.3161G

Komossa, S.; Grupe, D.; Mathur, S.

We report the results of an XMM-Newton observation of the narrow-line Seyfert 1 galaxy Mrk 1239. This optically highly polarized AGN has one of the steepest X-ray spectra found in AGNs, with αX=+3.0 based on ROSAT PSPC data. The XMM-Newton EPIC pn and MOS data confirm this steep X-ray spectrum. The pn data are best fitted by a power law…

2004 The Astronomical Journal
IUE XMM-Newton 36
XMM-Newton Observations of Two High-Redshift Quasars: RX J1028-0844 and BR 0351-1034
DOI: 10.1086/380615 Bibcode: 2004AJ....127....1G

Elvis, M.; Grupe, D.; Mathur, S. +1 more

We report the results of XMM-Newton observations of two high-redshift quasars, one radio-loud, RX J1028.6-0844 (z=4.276) and one radio-quiet, BR 0351-1034 (z=4.351). We find that the evidence for strong excess absorption toward RX J1028-0844 is marginal at best, contrary to previous claims. The superior sensitivity and broader, softer energy range…

2004 The Astronomical Journal
XMM-Newton 27
XMM-Newton Observations of the Extremely Low Accretion Rate Polars SDSS J155331.12+551614.5 and SDSS J132411.57+032050.5
DOI: 10.1086/424540 Bibcode: 2004AJ....128.2443S

Anderson, Scott F.; Brinkmann, J.; Szkody, Paula +6 more

XMM-Newton observations of the polar SDSS J155331.12+551614.5 reveal that all the X-ray flux emerges at energies less than 2 keV. The best fit to the spectrum is with a thermal plasma with kT=0.8 keV plus a 20-90 eV black body, yielding a thermal X-ray luminosity of (8.0-9.5)×1028 ergs s-1. The low temperature and X-ray lumin…

2004 The Astronomical Journal
XMM-Newton 26
Multiwavelength Properties of the X-Ray Sources in the Groth-Westphal Strip Field
DOI: 10.1086/420807 Bibcode: 2004AJ....127.3180M

Yamada, Toru; Griffiths, Richard E.; Sarajedini, Vicki +4 more

We summarize the multiwavelength properties of X-ray sources detected in the 80 ks XMM-Newton observation of the Groth-Westphal strip, a contiguous strip of 28 Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2) images. Among the ~150 X-ray sources detected in the XMM-Newton field of view, 23 are within the WFPC2 fields. Ten spectroscopic…

2004 The Astronomical Journal
XMM-Newton eHST 14