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Related papers: Possible New Identifications for EGRET Sources

200 papers

We report on the likely detection of pulsed high-energy gamma-rays from the binary millisecond pulsar PSR J0218+4232 in 100-1000 MeV data from CGRO EGRET. Imaging analysis demonstrates that the highly significant gamma-ray source 2EG…

Astrophysics · Physics 2007-05-23 L. Kuiper , W. Hermsen , F. Verbunt , A. Lyne , I. Stairs , D. J. Thompson , G. Cusumano

We have analyzed all the archival X-ray data of 134 unidentified (unID) gammaray sources listed in the first Fermi/LAT (1FGL) catalog and subsequently followed up by Swift/XRT. We constructed the spectral energy distributions (SEDs) from…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Y. Takeuchi , J. Kataoka , K. Maeda , Y. Takahashi , T. Nakamori , M. Tahara

A unique transient bursting radio source, GCRT J1745-3009, has been discovered (Hyman et al. 2005a) near the direction of the Galactic center. It is still an open question to explain this phenomenon, although some efforts to understand its…

Astrophysics · Physics 2009-11-24 W. W. Zhu , R. X. Xu

We describe Chandra, HST, and radio observations that reveal a radio-quiet but magnetospherically active neutron star in the error circle of the high-energy gamma-ray source 3EG J1835+5918, the brightest of the unidentified EGRET sources at…

Astrophysics · Physics 2009-11-07 J. P. Halpern , E. V. Gotthelf , N. Mirabal , F. Camilo

In the time domain, the radio sky in particular along the Galactic plane direction may vary significantly because of various energetic activities associated with stars, stellar and supermassive black holes. Using multi-epoch Very Large…

High Energy Astrophysical Phenomena · Physics 2022-01-12 Jun Yang , Yongjun Chen , Leonid I. Gurvits , Zsolt Paragi , Aiyuan Yang , Xiaolong Yang , Zhiqiang Shen

We present the preliminary results from two new surveys of blazars that have direct implications on the GLAST detection of extragalactic sources from two different perspectives: microwave selection and a combined deep X-ray/radio selection.…

Despite the plethora of deep (sub-mJy) radio surveys there remains considerable doubt as to the exact nature of the galaxies contributing to the source counts. Current evidence suggests that starformation in moderately luminous 'normal'…

Astrophysics · Physics 2009-11-11 Nick Seymour , Derek Moss , Ian McHardy , Katherine Gunn , Mat Page , Nic Loaring , Tom Dwelly

We discuss the time-series behavior of 8 extragalactic 3FGL sources away from the Galactic plane (i.e., $\mid b\mid \geq 10^{\circ}$) whose uncertainty ellipse contains a single X-ray and one radio source. The analysis was done using the…

High Energy Astrophysical Phenomena · Physics 2021-07-14 P. Nkundabakura , J. D. Kamanzi , J. D. Mbarubucyeye , T. Mutabazi

Active galaxies, especially blazars, are among the most promising neutrino source candidates. To date, ANTARES searches for these objects considered GeV-TeV $\gamma$-ray bright blazars. Here, a statistically complete radio-bright blazar…

High Energy Astrophysical Phenomena · Physics 2024-03-13 ANTARES Collaboration , A. Albert , S. Alves , M. André , M. Ardid , S. Ardid , J. J. Aubert , J Aublin , B. Baret , S. Basa , Y. Becherini , B. Belhorma , M. Bendahman , F. Benfenati , V. Bertin , S. Biagi , M. Bissinger , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Brânzaş , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , L. Caramete , F. Carenini , J. Carr , V. Carretero , S. Celli , L. Cerisy , M. Chabab , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , J. A. B. Coelho , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , A. S. M. Cruz , A. F. Díaz , B. De Martino , C. Distefano , I. Di Palma , A. Domi , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , T. van Eeden , D. van Eijk , S. El Hedri , N. El Khayati , A. Enzenhöfer , P. Fermani , G. Ferrara , F. Filippini , L. Fusco , S. Gagliardini , J. García , C. Gatius Oliver , P. Gay , N. Geißelbrecht , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , L. Haegel , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , F. Huang , G. Illuminati , C. W. James , B. Jisse-Jung , M. de Jong , P. de Jong , M. Kadler , O. Kalekin , U. Katz , A. Kouchner , Y. A Kovalev , Y. Y Kovalev , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , M. Lamoureux , A. Lazo , D. Lefèvre , E. Leonora , G. Levi , S. Le Stum , D. Lopez-Coto , S. Loucatos , L. Maderer , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , P. Migliozzi , A. Moussa , R. Muller , S. Navas , E. Nezri , B. Ó Fearraigh , E. Oukacha , A. Păun , G. E. Păvălaş , S. Peña-Martínez , M. Perrin-Terrin , V. Pestel , P. Piattelli , A. Plavin , C. Poirè , V. Popa , T. Pradier , A. Pushkarev , N. Randazzo , D. Real , S. Reck , G. Riccobene , A. Romanov , A. Sánchez-Losa , A. Saina , F. Salesa Greus , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , J. Schumann , F. Schüssler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , S. J. Tingay , S. Troitsky , B. Vallage , G. Vannoye , V. Van Elewyck , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zúñiga , OVRO Collaboration , : , T. Hovatta , S. Kiehlmann , I. Liodakis , V. Pavlidou , A. C. S Readhead

We obtained new ROSAT HRI and optical observations in the field of the Einstein X-ray source E 0336-248, which we use to identify it as a 19th magnitude BL Lacertae object at z=0.251 with an X-ray luminosity of 10^45 erg/s. It is also a 14…

Astrophysics · Physics 2009-10-30 J. P. Halpern , M. Eracleous , K. Forster

High redshift blazars are among the most powerful non-explosive sources in the Universe and play a crucial role in understanding the evolution of relativistic jets. To understand these bright objects, we performed a detailed investigation…

High Energy Astrophysical Phenomena · Physics 2024-01-29 N. Sahakyan , G. Harutyunyan , S. Gasparyan , D. Israyelyan

(Abridged) We made use of X-ray observations with the X-ray telescope on-board the \swift observatory to refine the X-ray position to 3-5" accuracy of 12 INTEGRAL sources, so as to further identify their counterpart at optical, infrared,…

Astrophysics · Physics 2009-11-13 J. Rodriguez , J. A. Tomsick , S. Chaty

We present a multiwavelength study of the environment of the unidentified X-ray/gamma-ray sources IGR J18027-1455 and IGR J21247+5058, recently discovered by the IBIS/ISGRI instrument, onboard the INTEGRAL satellite. The main properties of…

Astrophysics · Physics 2007-05-23 J. A. Combi , M. Ribo , I. F. Mirabel

Since radio sources with Ultra Steep Spectra (USS; alpha <~ -1.30; S ~ nu^alpha) are efficient tracers of high redshift radio galaxies (HzRGs), we have defined three samples of such USS sources using the recently completed WENSS, TEXAS,…

Astrophysics · Physics 2011-05-23 Carlos De Breuck , Wil van Breugel , Huub Rottgering , George Miley

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…

Astrophysics · Physics 2007-05-23 D. J. Thompson , S. W. Digel , P. L. Nolan , O. Reimer

The error region of the INTEGRAL source, IGR J17448-3232, contains an X-ray point source at the edge of a ~3' radius extended X-ray source. It has been suggested that the extended emission is a young supernovae remnant (SNR) while the point…

High Energy Astrophysical Phenomena · Physics 2012-01-10 P. A. Curran , S. Chaty , J. A. Zurita Heras , J. A. Tomsick , T. J. Maccarone

We report on the results of X-ray and radio follow-up observations of two GeV gamma-ray sources 2FGL J0923.5+1508 and 2FGL J1502.1+5548, selected as candidates for high-redshift blazars from unassociated sources in the {\it Fermi} Large…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Y. Takahashi , J. Kataoka , K. Niinuma , M. Honma , Y. Inoue , T. Totani , S. Inoue , T. Nakamori , K. Maeda

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…

A significant fraction ($\sim 30$ %) of the gamma-ray sources listed in the second $\textit{Fermi}$ LAT (2FGL) catalog is still of unknown origin, being not yet associated with counterparts at lower energies. Using the available information…

Context. While searching the NRAO VLA Sky Survey (NVSS) for diffuse radio emission, we have serendipitously discovered extended radio emission close to the Galactic plane. The radio morphology suggests the presence of a previously unknown…

High Energy Astrophysical Phenomena · Physics 2014-09-05 F. de Gasperin , C. Evoli , M. Bruggen , A. Hektor , M. Cardillo , P. Thorman , W. A. Dawson , C. B. Morrison