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相关论文: A survey for pulsars in EGRET error boxes

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We have conducted a radio pulsar survey of 56 unidentified gamma-ray sources from the 3rd EGRET catalog which are at intermediate Galactic latitudes (5 deg. < |b| < 73 deg.). For each source, four interleaved 35-minute pointings were made…

天体物理学 · 物理学 2008-11-26 F. Crawford , M. S. E. Roberts , J. W. T. Hessels , S. M. Ransom , M. Livingstone , C. R. Tam , V. M. Kaspi

We present a new survey for pulsars in the error boxes of the low-latitude EGRET sources 3EG J1027-5817, 3EG J1800-2338 and 3EG J1810-1032. Although all of these sources have been covered by previous pulsar surveys, the recent discovery of…

天体物理学 · 物理学 2009-11-13 M. J. Keith , S. Johnston , M. Kramer , P. Weltevrede , K. Watters , B. Stappers

At the end of the EGRET mission, only 6-8 Galactic sources had been identified as young pulsars. Since then, several energetic pulsars have been discovered in EGRET error boxes along the Galactic plane, as well as several pulsar wind…

天体物理学 · 物理学 2009-11-10 Mallory S. E. Roberts

The EGRET telescope on the Compton Gamma-Ray Observatory detected over 200 sources and the majority of these are still unidentified. At least three subpopulations of EGRET sources have been associated with the Galaxy: bright sources lying…

天体物理学 · 物理学 2009-11-10 A. K. Harding , P. L. Gonthier , I. A. Grenier , C. A. Perrot

We present the results of radio searches for pulsars within unidentified EGRET source error boxes. Using the Parkes multibeam system, we have surveyed 56 sources at Galactic latitudes |b| > 5 deg which do not appear to be associated with…

3EG J1835+5918 is the brightest of the so-called unidentified EGRET sources at intermediate galactic latitude (l,b)=(89,25). We obtained complete radio, optical, and X-ray coverage of its error box, discovering a faint ultrasoft X-ray…

天体物理学 · 物理学 2007-05-23 N. Mirabal , J. Halpern , R. Mukherjee , E. Gotthelf , F. Camilo

Pulsars discovered since the end of the EGRET mission coincident with unidentified high-energy gamma-ray sources are prime targets for AGILE. Both general surveys and targeted observations have been successful in finding energetic young…

天体物理学 · 物理学 2007-05-23 Mallory S. E. Roberts

We present a correlative study between all unidentified EGRET sources at low Galactic latitudes and the newly discovered pulsars in the released portion of the Parkes multibeam radio survey. We note 14 positional coincidences: eight of…

天体物理学 · 物理学 2009-11-07 Diego F. Torres , Yousaf M. Butt , Fernando Camilo

We present a catalog of point gamma-ray sources detected by the EGRET detector aboard the Compton Gamma Ray Observatory. We have used the whole gamma-ray dataset of reprocessed photons at energies above 100 MeV together with new Galactic…

天体物理学 · 物理学 2009-11-13 Jean-Marc Casandjian , Isabelle A. Grenier

The EGRET source 3EG J1835+5918 is the brightest and most accurately positioned of the as-yet unidentified high-energy gamma-ray sources at high Galactic latitude (l,b=89,25). We present a multiwavelength study of the region around it,…

天体物理学 · 物理学 2009-10-31 N. Mirabal , J. P. Halpern , M. Eracleous , R. H. Becker

The identity of the persistent EGRET sources in the Galactic plane is largely a mystery. For one of these, 3EG J2227+6122, our complete census of X-ray and radio sources in its error circle reveals a remarkable superposition of an…

天体物理学 · 物理学 2009-10-31 J. P. Halpern , E. V. Gotthelf , K. M. Leighly , D. J. Helfand

Using a likelihood analysis (updated since McLaughlin & Cordes 2000) and EGRET detections, upper limits and diffuse background measurements, we find a best-fit luminosity law for the gamma-ray pulsar population. We find that roughly 30 of…

天体物理学 · 物理学 2007-05-23 M. A. McLaughlin , J. M. Cordes

Radio pulsar PSR J1028-5819 was recently discovered in a high-frequency search (at 3.1 GHz)in the error circle of the EGRET source 3EG J1027-5817. The spin-down power of this young pulsar is great enough to make it very likely the…

高能天体物理现象 · 物理学 2011-02-11 LAT Collaboration

We investigate whether gamma-ray pulsars viewed at a large angle to the neutron star magnetic pole could contribute to the new population of galactic unidentified EGRET sources associated with the Gould Belt. The faint, soft nature of these…

天体物理学 · 物理学 2009-10-31 Alice K. Harding , Bing Zhang

We report the detection of radio and X-ray pulsations at a period of 51.6 ms from the X-ray source RX/AX J2229.0+6114 in the error box of the EGRET source 3EG J2227+6122. An ephemeris derived from a single ASCA observation and multiple…

天体物理学 · 物理学 2009-11-06 J. P. Halpern , F. Camilo , E. V. Gotthelf , D. J. Helfand , M. Kramer , A. G. Lyne , K. M. Leighly , M. Eracleous

At least three pulsars in supernova remnants were detected at E > 100 MeV by EGRET on the Compton Gamma Ray Observatory. Efforts to search for additional pulsars in the EGRET data have been unsuccessful due to limited statistics. An example…

天体物理学 · 物理学 2007-05-23 D. J. Thompson , S. W. Digel , P. L. Nolan , O. Reimer

The majority of Galactic high-energy gamma-ray sources continue to elude identification. Currently, we have a handful of firm pulsar identifications, one of which is radio quiet, and a few marginal detections, including one millisecond…

天体物理学 · 物理学 2007-05-23 Mallory S. E. Roberts

We present the discovery of PSR J1410-6132, a 50-ms pulsar found during a high-frequency survey of the Galactic plane, using a 7-beam 6.3-GHz receiver on the 64-m Parkes radio telescope. The pulsar lies within the error box of the…

In the error box of 3EG J1835+5918, the brightest as-yet unidentified EGRET source at intermediate Galactic latitude, we find a weak, ultrasoft X-ray source at energies E < 0.3 keV in the ROSAT All-Sky Survey. Deep optical imaging at the…

天体物理学 · 物理学 2009-10-31 N. Mirabal , J. P. Halpern

The 3rd EGRET Catalog of High-energy Gamma-ray Sources contains 170 unidentified sources, and there is great interest in the nature of these sources. One means of determining source class is the study of flux variability on time scales of…

天体物理学 · 物理学 2009-10-31 P. M. Wallace , D. L. Bertsch , S. D. Bloom , N. J. Griffis , R. C. Hartman , D. A. Kniffen , D. J. Thompson
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