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Approximately one-third of the gamma-ray sources in the third Fermi-LAT catalog are unidentified or unassociated with objects at other wavelengths. Observations with Swift-XRT have yielded possible counterparts in $\sim$30% of these source…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Amanpreet Kaur , Abraham D Falcone , Michael D Stroh , Jamie A Kennea , Elizabeth C Ferrara

Binary neutron star (NS) mergers are among the most promising astrophysical sources of gravitational wave emission for Advanced LIGO and Advanced Virgo, expected to be operational in 2015. Finding electromagnetic counterparts to these…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 Jonah Kanner , Jordan Camp , Judith Racusin , Neil Gehrels , Darren White

Population studies of the extragalactic objects are a major part of the universe large-scale structure study. Apart from radio, infrared, and visible wavelength bands, observations and further identification of extragalactic objects such as…

Astrophysics of Galaxies · Physics 2020-01-08 A. Tugay , S. Shevchenko

We present the results of a study of the variability of X-ray sources in the central 30' of the nearby Andromeda Galaxy (M31) based on XMM Performance Verification observations. Two observations of this field, with a total exposure time of…

The radio-quiet neutron star 1E1207.4-5209 has been the target of several XMM-Newton observations, with a total exposure of ~350 ks. The source is located at intermediate galactic latitude (b~10 degrees), i.e. in a sky region with an…

High Energy Astrophysical Phenomena · Physics 2015-05-13 G. Novara , N. La Palombara , R. P. Mignani , E. Hatziminaoglou , M. Schirmer , A. De Luca , P. A. Caraveo

The Chandra ACIS Survey of M33 (ChASeM33) has acquired 7 fields of ACIS data covering M33 with 200 ks of exposure in each field. A catalog from the first 10 months of data, along with archival Chandra observations dating back to the year…

We report the results of an optical campaign carried out by the XMM-Newton Survey Science Centre with the specific goal of identifying the brightest X-ray sources in the XMM-Newton Galactic Plane Survey of Hands et al. (2004). In addition…

High Energy Astrophysical Phenomena · Physics 2015-05-14 C. Motch , R. Warwick , M. S. Cropper , F. Carrera , P. Guillout , F. X. Pineau , M. W. Pakull , S. Rosen , A. Schwope , J. Tedds , N. Webb , I. Negueruela , M. G. Watson

We have created a new, clean catalogue of extragalactic non-nuclear X-ray sources by correlating the 3XMM-DR4 data release of the XMM-Newton Serendipitous Source Catalogue with the Third Reference Catalogue of Bright Galaxies and the…

High Energy Astrophysical Phenomena · Physics 2019-01-09 H. P. Earnshaw , T. P. Roberts , M. J. Middleton , D. J. Walton , S. Mateos

We present an overview of our Supergiant Fast X-ray Transients (SFXT) project, that started in 2007, by highlighting the unique observational contribution Swift is giving to this exciting new field. By means of outburst detection with…

High Energy Astrophysical Phenomena · Physics 2011-04-01 P. Romano , S. Vercellone , V. La Parola , G. Cusumano , V. Mangano , P. Esposito , J. A. Kennea , D. N. Burrows , H. A. Krimm , C. Pagani , N. Gehrels

We consider the prospects for a complete survey of the 18,811 sources of the ROSAT All-Sky Survey Bright Source Catalog (BSC) with NASA's Swift gamma-ray burst (GRB) mission. By observing each BSC source for 500 s with the satellite's…

Astrophysics · Physics 2007-05-23 Derek B. Fox

We present the second ROSAT all-sky survey source catalogue, hereafter referred to as the 2RXS catalogue. This is the second publicly released ROSAT catalogue of point-like sources obtained from the ROSAT all-sky survey (RASS) observations…

High Energy Astrophysical Phenomena · Physics 2016-09-30 Th. Boller , M. J. Freyberg , J. Truemper , F. Haberl , W. Voges , K. Nandra

In recent years, thanks to the continuous surveys performed by INTEGRAL and Swift satellites, our knowledge of the hard X-ray/soft gamma-ray sky has greatly improved. As a result it is now populated with about 2000 sources, both Galactic…

High Energy Astrophysical Phenomena · Physics 2021-02-17 F. Onori , M. Fiocchi , N. Masetti , A. F. Rojas , A. Bazzano , L. Bassani , A. J. Bird

Four hard X-ray sources from the INTEGRAL and Swift catalogs have been identified. X-ray and optical spectra have been obtained for each of the objects being studied by using data from the INTEGRAL, Swift, ROSAT, and Chandra X-ray…

High Energy Astrophysical Phenomena · Physics 2013-07-11 A. A. Lutovinov , A. I. Mironov , R. A. Burenin , M. G. Revnivtsev , S. S. Tsygankov , M. N. Pavlinsky , I. V. Korobtsev , M. V. Eselevich

Supergiant Fast X-ray Transients (SFXTs) are a new class of HMXBs discovered thanks to the monitoring of the Galactic plane performed with the INTEGRAL satellite in the last 5 years. These sources display short outbursts (significantly…

After the first nine years of INTEGRAL operational life, the discovery of new sources and source types, a large fraction of which are highly transient or highly absorbed, is certainly one of the most compelling results and legacies of…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Mariateresa Fiocchi , Lorenzo Natalucci

We present the results of our optical identifications of several hard X-ray sources from the INTEGRAL all-sky survey obtained over 14 years of observations. Having improved the positions of these objects in the sky with the X-ray telescope…

We carried out new observations of two fields in the northern ring of M31 with XMM-Newton with two exposures of 100 ks each and obtained a complete list of X-ray sources down to a sensitivity limit of ~7 x 10^34 erg s^-1 (0.5 - 2.0 keV).…

During the last ~50 years, the population of black hole candidates in X-ray binaries has increased considerably with 59 Galactic objects detected in transient low-mass X-ray binaries, plus a few in persistent systems (including ~5…

High Energy Astrophysical Phenomena · Physics 2016-02-17 Jesus M. Corral-Santana , Jorge Casares , Teo Munoz-Darias , Franz E. Bauer , Ignacio G. Martinez-Pais , David M. Russell

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

High Energy Astrophysical Phenomena · Physics 2015-06-19 A. Paggi , F. Massaro , R. D'Abrusco , H. A. Smith , N. Masetti , M. Giroletti , G. Tosti , S. Funk

We have obtained a deep 8-field XMM-Newton mosaic of M33 covering the galaxy out to the D$_{25}$ isophote and beyond to a limiting 0.2--4.5 keV unabsorbed flux of 5$\times$10$^{-16}$ erg cm$^{-2}$ s$^{-1}$ (L${>}$4$\times$10$^{34}$ erg…