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1SXPS: A Deep Swift X-Ray Telescope Point Source Catalog with Light Curves and Spectra
DOI: 10.1088/0067-0049/210/1/8 Bibcode: 2014ApJS..210....8E

Tagliaferri, G.; Gehrels, N.; Pagani, C. +9 more

We present the 1SXPS (Swift-XRT point source) catalog of 151,524 X-ray point sources detected by the Swift-XRT in 8 yr of operation. The catalog covers 1905 deg2 distributed approximately uniformly on the sky. We analyze the data in two ways. First we consider all observations individually, for which we have a typical sensitivity of ~3 …

2014 The Astrophysical Journal Supplement Series
XMM-Newton 151
X-Ray Emission from Magnetic Massive Stars
DOI: 10.1088/0067-0049/215/1/10 Bibcode: 2014ApJS..215...10N

Wade, Gregg A.; Nazé, Yaël; ud-Doula, Asif +4 more

Magnetically confined winds of early-type stars are expected to be sources of bright and hard X-rays. To clarify the systematics of the observed X-ray properties, we have analyzed a large series of Chandra and XMM-Newton observations, corresponding to all available exposures of known massive magnetic stars (over 100 exposures covering ~60% of star…

2014 The Astrophysical Journal Supplement Series
XMM-Newton 109
Chasing the Identification of ASCA Galactic Objects (ChIcAGO): An X-Ray Survey of Unidentified Sources in the Galactic Plane. I. Source Sample and Initial Results
DOI: 10.1088/0067-0049/212/1/13 Bibcode: 2014ApJS..212...13A

Drake, Jeremy J.; Chakrabarty, Deepto; Lee, Julia C. +18 more

We present the Chasing the Identification of ASCA Galactic Objects (ChIcAGO) survey, which is designed to identify the unknown X-ray sources discovered during the ASCA Galactic Plane Survey (AGPS). Little is known about most of the AGPS sources, especially those that emit primarily in hard X-rays (2-10 keV) within the Fx ~ 10-13

2014 The Astrophysical Journal Supplement Series
XMM-Newton 13
K-shell Photoabsorption of Magnesium Ions
DOI: 10.1088/0067-0049/214/1/8 Bibcode: 2014ApJS..214....8H

García, J.; Kallman, T. R.; Gatuzz, E. +4 more

X-ray photoabsorption cross sections have been computed for all magnesium ions with three or more electrons using the R-matrix method. A comparison with other available data for Mg II-Mg X shows good qualitative agreement in the resultant resonance shapes. However, for the lower ionization stages, and for singly ionized Mg II in particular, the pr…

2014 The Astrophysical Journal Supplement Series
XMM-Newton 12