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Related papers: A bright X-ray transient towards NGC 5128 (Centaur…

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We discovered the optical counterpart about 13 mag of a soft X-ray transient, XTE J1118+480 on 2000 March 30. We perform astrometry and provide the accurate position as R.A. = 11h18m10s.85, Decl. = +48o02'12".9. The outbursting object is…

AX J1745.6-2901 and GRS 1741-2853 are two transient neutron star low-mass X-ray binaries that are located within ~10' from the Galactic center. Multi-year monitoring observations with the Swift/XRT has exposed several accretion outbursts…

High Energy Astrophysical Phenomena · Physics 2015-06-19 N. Degenaar , R. Wijnands , M. T. Reynolds , J. M. Miller , J. Kennea , N. Gehrels

We report on the discovery and analysis of the transient X-ray pulsar XMMU J031747.5-663010 detected in the 2004 November 23 XMM-Newton observation of the spiral galaxy NGC 1313. The X-ray source exhibits pulsations with a period P~765.6 s…

Astrophysics · Physics 2012-09-17 Sergey Trudolyubov

We report on six Chandra and one HST/WFC3 observation of CXO J122518.6+144545, discovered by Jonker et al. (2010) as a candidate hyperluminous X-ray source (HLX), X-ray bright supernova or recoiling supermassive black hole at $L_X = 2.2…

High Energy Astrophysical Phenomena · Physics 2015-09-30 M. Heida , P. G. Jonker , M. A. P. Torres

The population of clearly identified anomalous X-ray pulsars has recently grown to seven, however, one candidate anomalous X-ray pulsar (AXP) still eludes re-confirmation. Here, we present a set of seven Chandra ACIS-S observations of the…

Astrophysics · Physics 2008-11-26 C. R. Tam , V. M. Kaspi , B. M. Gaensler , E. V. Gotthelf

The infrared spectrograph GNIRS on Gemini South unlocks new possibilities to study the central black holes in dusty galaxies that have been inaccessible to previous black hole studies. We exploit good near-infrared seeing to measure the…

Astrophysics · Physics 2009-11-10 Julia D. Silge , Karl Gebhardt , Marcel Bergmann , Douglas Richstone

Ultra-luminous X-Ray sources are extra-nuclear point sources in external galaxies with $L_X=10^{39}$--$10^{41}$ erg/s and are among the most poorly understood X-ray sources. To help understand their nature, we are trying to identify their…

Astrophysics · Physics 2009-11-10 Ji-Feng Liu Joel N. Bregman , Patrick Seitzer

ASCA observed the central region of the Small Magellanic Cloud, and found a hard X-ray source, AX J0051-733, at the position of the ROSAT source RX J0050.8-7316, which has an optical counterpart of a Be star. Coherent X-ray pulsations of…

Astrophysics · Physics 2015-06-24 Kensuke Imanishi , Jun Yokogawa , Masahiro Tsujimoto , Katsuji Koyama

On January 10 and 13, 2001, Venus was observed for the first time with an X-ray astronomy satellite. The observation, performed with the ACIS-I and LETG/ACIS-S instruments on Chandra, yielded data of high spatial, spectral, and temporal…

Astrophysics · Physics 2007-05-23 K. Dennerl , V. Burwitz , J. Englhauser , C. Lisse , S. Wolk

With enough X-ray flux to be detected in a 160s scan by SRG/eROSITA, the $z = 6.19$ quasar CFHQS J142952+544717 is, by far, the most luminous X-ray source known at $z > 6$. We present deep (245 ks) NuSTAR observations of this source; with…

We report the result of a new Chandra observation of the black hole X-ray transient H 1705-250 in quiescence. H 1705-250 was barely detected in the new 50 ks Chandra observation. With 5 detected counts, we estimate the source quiescent…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Yi-Jung Yang , Albert K. H. Kong , David M. Russell , Fraser Lewis , Rudy Wijnands

X-ray observations unveiled the existence of enigmatic point-like sources at the centre of young supernova remnants (SNRs). These sources, dubbed Central Compact Objects (CCOs), are thought to be neutron stars formed by the supernova…

Astrophysics · Physics 2009-11-13 R. P. Mignani , S. Zaggia , A. De Luca , R. Perna , N. Bassan , P. A. Caraveo

We present our analysis of Chandra observations obtained when the soft X-ray transient RX J170930.2-263927 (XTE J1709-267) returned to quiescence after an outburst. Using the type I burst peak luminosity found by Cocchi et al. (1998) and…

Astrophysics · Physics 2009-11-07 P. G. Jonker , M. Mendez , G. Nelemans , R. Wijnands , M. van der Klis

We report a deep optical imaging observation by the Subaru telescope for a very soft X-ray source RX J1836.2+5925, which has been suspected to be an isolated neutron star associated with the brightest as-yet unidentified EGRET source…

Astrophysics · Physics 2015-06-24 T. Totani , W. Kawasaki , N. Kawai

We report the detection of a potential cosmic radio transient source using the two stations of the Long Wavelength Array. The transient was detected on 18 October 2017 08:47 UTC near the celestial equator while reducing 10,240 hours of…

High Energy Astrophysical Phenomena · Physics 2020-06-29 S. S. Varghese , K. S. Obenberger , J. Dowell , G. B. Taylor

We report on the BeppoSAX/WFC observation of a strong type-I X-ray burst from the recently discovered transient source SAX J1810.8-2609. The observed event showed evidence of photospheric radius expansion due to super-Eddington burst…

AX J1949.8+2534 is a candidate supergiant fast X-ray transient (SFXT) observed in outburst by INTEGRAL (IGR J19498+2534). We report on the results of six Neil Gehrels Swift-XRT, one Chandra, and one NuSTAR observation of the source. We find…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Jeremy Hare , Jules P. Halpern , Maica Clavel , Jonathan E. Grindlay , Farid Rahoui , John A. Tomsick

Transitional millisecond pulsars are accreting millisecond pulsars that switch between accreting X-ray binary and millisecond radio pulsar states. Only a handful of these objects have been identified so far. Terzan 5 CX1 is a variable hard…

We report the serendipitous discovery of transient, point-like high energy gamma-ray emission coincident with the position of the suspected BL Lac object 5C 3.178. The source was detected using the Fermi Large Area Telescope (LAT) at a…

High Energy Astrophysical Phenomena · Physics 2013-04-18 Hugh Dickinson , Christian Farnier