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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…

Astrophysics · Physics 2009-10-31 N. Mirabal , J. P. Halpern

The EGRET telescope aboard NASAs Compton GRO has repeatedly detected 3EG J1835+5918, a bright and steady source of high-energy gamma-ray emission with no identification suggested until recently. The long absence of any likely counterpart…

Astrophysics · Physics 2007-05-23 O. Reimer , K. T. S. Brazier , A. Carrami , G. Kanbach , P. L. Nolan , D. J. Thompson

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…

Astrophysics · Physics 2007-05-23 N. Mirabal , J. Halpern , R. Mukherjee , E. Gotthelf , F. Camilo

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

The EGRET telescope has repeatedly observed 3EG J1835+5918 as a bright and steady source of high-energy gamma-ray radiation which has not yet been indentified. EGRET data from CGRO observation cycle 1 to 7 have been reanalysed above 100 MeV…

Astrophysics · Physics 2009-11-06 O. Reimer , K. T. S. Brazier , A. Carraminana , G. Kanbach , P. L. Nolan , D. J. Thompson

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,…

Astrophysics · Physics 2009-10-31 N. Mirabal , J. P. Halpern , M. Eracleous , R. H. Becker

We report unsuccessful searches for pulsations from the neutron star RX J1836.2+5925 identified with the EGRET source 3EG J1835+5918. A 24 hr observation with the NRAO Green Bank Telescope at 820 MHz placed an upper limit on flux density of…

Astrophysics · Physics 2009-11-13 J. P. Halpern , F. Camilo , E. V. Gotthelf

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…

Astrophysics · Physics 2009-10-31 J. P. Halpern , E. V. Gotthelf , K. M. Leighly , D. J. Helfand

In search of the counterpart to the brightest unidentified gamma-ray source 3EG J2020+4017 we report on new X-ray and radio observations of the gamma-Cygni field with the Chandra X-ray Observatory and with the Green Bank Telescope. We also…

The X-ray source eRASSU J065715.3+260428 was identified as a likely thermally emitting isolated neutron star in a search in the SRG/eROSITA All-Sky Survey. We investigated the nature and evolutionary state of the source through a dedicated…

High Energy Astrophysical Phenomena · Physics 2025-01-14 J. Kurpas , A. M. Pires , A. D. Schwope , Z. C. Pan , Z. L. Zhang , L. Qian , F. Haberl , L. Ji , I. Traulsen

We present deep optical and X-ray follow-up observations of the bright unassociated Fermi-LAT gammaray source 1FGL J1311.7-3429. The source was already known as an unidentified EGRET source (3EG J1314-3431, EGR J1314-3417), hence its nature…

High Energy Astrophysical Phenomena · Physics 2015-06-11 J. Kataoka , Y. Yatsu , N. Kawai , Y. Urata , C. C. Cheung , Y. Takahashi , K. Maeda , T. Totani , R. Makiya , H. Hanayama , T. Miyaji , A. Tsai

With the XMM-Newton and Suzaku observations, for the first time, we acquired broad-band spectra of two unidentified X-ray sources towards the Galactic bulge: 1RXS J180556.1$-$343818 and 1RXS J173905.2$-$392615. The 1RXS J180556.1$-$343818…

High Energy Astrophysical Phenomena · Physics 2016-02-24 Hideyuki Mori , Yoshitomo Maeda , Yoshihiro Ueda

Following up on a faint detection of a near-infrared (NIR) source at the position of the X-ray thermal isolated neutron star RX J0806.4-4123, we present new Hubble Space Telescope observations in the H-band. The NIR source is unambiguously…

High Energy Astrophysical Phenomena · Physics 2018-09-24 B. Posselt , G. G. Pavlov , Ü. Ertan , S. Çalışkan , K. L. Luhman , C. C. Williams

We studied the soft-X-ray emission of five hard-X sources: IGR J08262-3736, IGR J17354-3255, IGR J16328-4726, SAX J1818.6-1703 and IGR J17348-2045. These sources are: a confirmed supergiant high mass X-ray binary (IGR J08262-3736);…

High Energy Astrophysical Phenomena · Physics 2013-03-20 L. Pavan , E. Bozzo , C. Ferrigno , M. Falanga , S. Campana , S. Paltani , L. Stella , R. Walter

We report observations with the Chandra X-ray Observatory of a field in the gamma$-Cygni supernova remnant (SNR78.2+2.1) centered on the cataloged location of the unidentified, bright gamma-ray source 3EG J2020+4017. In this search for an…

In the ROSAT Bright Survey (RBS) we have almost completely optically identified the brightest ~2000 high-galactic latitude sources from the ROSAT All-Sky Survey Bright Source Catalogue (1RXS). A small number of sources has empty X-ray error…

Astrophysics · Physics 2007-05-23 A. D. Schwope , G. Hasinger , R. Schwarz , F. Haberl , M. Schmidt

We have discovered with the Wide Field Cameras on board BeppoSAX the weak transient X-ray source SAXJ2239.3+6116 whose position coincides with that of 4U2238+60/3A2237+608 and is close to that of the fast transient AT2238+60 and the…

We report on the association of an X-ray source (WGA J2025.1+3342), serendipitously found with BeppoSAX in two separate observations, with the unidentified EGRET source 3EG J2027+3429. The source is detected from 1 keV up to about 100 keV,…

Astrophysics · Physics 2009-11-10 V. Sguera , A. Malizia , L. Bassani , J. B. Stephen , G. Di Cocco

We report the discovery of a remarkable gamma-ray transient source near the Galactic plane, GRO J1838-04. This source was serendipitously discovered by EGRET in June 1995 with a peak intensity of 4 E(-6) ph/cm/cm/s (for photon energies…

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