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FERMI LARGE AREA TELESCOPE FIRST SOURCE CATALOG
We present a catalog of high-energy gamma-ray sources detected by the Large Area Telescope (LAT), the primary science instrument on the Fermi Gamma-ray Space Telescope (Fermi), during the first 11Expand
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Fermi Large Area Telescope Second Source Catalog
We present the second catalog of high-energy γ-ray sources detected by the Large Area Telescope (LAT), the primary science instrument on the Fermi Gamma-ray Space Telescope (Fermi), derived from dataExpand
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X-ray background measurements with XMM-Newton EPIC
We discuss the methods used to compile a high signal-to-noise dataset representative of both the instrumental and cosmic background signal measured at high galactic latitude by the XMM-Newton EPICExpand
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The 2-8 keV Cosmic x-ray background spectrum as observed with XMM - Newton
We have measured the spectrum of the Cosmic X-ray Background (CXB) in the 2–8 keV range with the high throughput EPIC/MOS instrument onboard XMM-Newton. A large sample of high galactic latitudeExpand
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THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
This catalog summarizes 117 high-confidence > 0.1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half are neutron starsExpand
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The First Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
The dramatic increase in the number of known gamma-ray pulsars since the launch of the Fermi Gamma-ray Space Telescope (formerly GLAST) offers the first opportunity to study a population of theseExpand
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The magnetic field of an isolated neutron star from X-ray cyclotron absorption lines
Isolated neutron stars are highly magnetized, fast-rotating objects that form as an end point of stellar evolution. They are directly observable in X-ray emission, because of their high surfaceExpand
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Discovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13
NGC 7793 P13 is a variable (luminosity range ∼100) ultraluminous X-ray source proposed to host a stellar-mass black hole of less than 15 M⊙ in a binary system with orbital period of 64 d and a 18-23Expand
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Pulse phase variations of the X-ray spectral features in the radio-quiet neutron star 1E 1207-5209
We present the results of an XMM-Newton observation of the radio-quiet X-ray pulsar 1E 1207� 5209 located at the center of the shell-like supernova remnant G296.5+10.0. The X-ray spectrum isExpand
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On the Polar Caps of the Three Musketeers
XMM-Newton EPIC observations of PSR B0656+14, PSR B1055-52, and Geminga have substantially increased the collection of statistics available for these three isolated neutron stars, so apparentlyExpand
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