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Related papers: Identifying New X-ray Binary Candidates in M31 usi…

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We introduce the New-ANGELS program, an XMM-Newton survey of $\sim7.2\rm~deg^2$ area around M 31, which aims to study the X-ray populations in M 31 disk and the X-ray emitting hot gas in the inner halo of M 31 up to 30 kpc. In this first…

High Energy Astrophysical Phenomena · Physics 2023-06-21 Rui Huang , Jiang-Tao Li , Wei Cui , Joel N. Bregman , Xiang-Dong Li , Gabriele Ponti , Zhijie Qu , Q. Daniel Wang , Yi Zhang

Context. Serendipitous X-ray surveys have proven to be an efficient way to find rare objects, for example tidal disruption events, changing-look active galactic nuclei (AGN), binary quasars, ultraluminous X-ray sources (ULXs), and…

High Energy Astrophysical Phenomena · Physics 2022-01-26 Hugo Tranin , Olivier Godet , Natalie Webb , Daria Primorac

Aims. M 31 has been completely imaged for the first time obtaining a luminosity lower limit ~10^35 erg s-1 in the 0.2-4.5 keV band. Our XMM-Newton EPIC survey combines archival observations with observations taken between June 2006 and…

High Energy Astrophysical Phenomena · Physics 2015-05-28 H. Stiele , W. Pietsch , F. Haberl , D. Hatzidimitriou , R. Barnard , B. F. Williams , A. K. H. Kong , U. Kolb

We have detected 523 sources in a survey of the Small Magellanic Cloud (SMC) Wing with Chandra. By cross-correlating the X-ray data with optical and near-infrared catalogues we have found 300 matches. Using a technique that combines X-ray…

We have previously identified 10 M31 black hole candidates (BHCs) in M31, from their X-ray properties alone. They exhibit "hard state" emission spectra that are seen at luminosities < ~10% Eddington in X-ray binaries (XBs) containing a…

High Energy Astrophysical Phenomena · Physics 2015-06-15 R. Barnard , M. R. Garcia , S. S. Murray

We present Chandra studies of the X-ray binary (XRB) populations in the bulge and ring regions of the ring galaxy NGC 1291. We detect 169 X-ray point sources in the galaxy, 75 in the bulge and 71 in the ring, utilizing the four available…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 B. Luo , G. Fabbiano , T. Fragos , D. -W. Kim , K. Belczynski , N. J. Brassington , S. Pellegrini , P. Tzanavaris , Junfeng Wang , A. Zezas

We present our analysis of high quality high mass X-ray binary (HMXB) candidates in M31 selected from point-source optical-counterpart candidates from the Chandra-PHAT survey catalog. We fit the spectral energy distributions (SEDs) of…

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).…

We present 15 high mass X-ray binary (HMXB) candidates in the disk of M31 for which we are able to infer compact object type, spectral type of the donor star, and age using multiwavelength observations from NuSTAR, Chandra, and the Hubble…

Building on recent work by Chandar et al. (2020), we construct X-ray luminosity functions (XLFs) for different classes of X-ray binary (XRB) donors in the nearby star-forming galaxy M83 through a novel methodology: rather than classifying…

High Energy Astrophysical Phenomena · Physics 2021-05-12 Qiana Hunt , Elena Gallo , Rupali Chandar , Paula Johns Mulia , Angus Mok , Andrea Prestwich , Shengchen Liu

Based on the archival data from the Chandra observations of nearby galaxies, we study different sub populations of low-mass X-ray binaries (LMXBs) - dynamically formed systems in globular clusters (GCs) and in the nucleus of M31 and…

Using hard (E>10 keV) X-ray observations with NuSTAR, we are able to differentiate between accretion states, and thus compact object types, of neutron stars and black holes in X-ray binaries (XRBs) in M31, our nearest Milky Way-type…

We carry out classification of 4330 X-ray sources in the 2XMMi-DR3 catalog. They are selected under the requirement of being a point source with multiple XMM-Newton observations and at least one detection with the signal-to-noise ratio…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Dacheng Lin , Natalie A. Webb , Didier Barret

This paper includes two parts. The first is to present the spectral energy distributions (SEDs) of 49 globular cluster (GC) X-ray sources in the BATC 13 intermediate-band filters from 3800 to 10000 A, and identify 8 unidentified X-ray…

Astrophysics · Physics 2009-11-11 Zhou Fan , Jun Ma , Xu Zhou , Jiansheng Chen , Zhaoji Jiang , Zhenyu Wu

We present a new technique for identifying stellar mass black holes in low mass X-ray binaries (LMXBs), and apply it to XMM-Newton observations of M31. We examine X-ray time series variability seeking power density spectra (PDS) typical of…

Astrophysics · Physics 2009-11-10 R. Barnard , J. P. Osborne , U. C. Kolb , C. A. Haswell

To maximize the discovery potential of future synoptic surveys, especially in the field of transient science, it will be necessary to use automatic classification to identify some of the astronomical sources. The data mining technique of…

Instrumentation and Methods for Astrophysics · Physics 2015-06-18 Kitty K. Lo , Sean Farrell , Tara Murphy , B. M. Gaensler

We investigated for a possible connection between the types of X-ray binaries (XRBs) and the properties of compact star clusters in the nearby galaxy NGC 628. Using {\it Chandra} archival data covering the years 2001-2018, 75 X-ray sources…

High Energy Astrophysical Phenomena · Physics 2023-01-25 Senay Avdan , Aysun Akyuz , Seda Acar , Inci Akkaya Oralhan , Sinan Allak , Nazim Aksaker

We report on optical searches in the error circles of 93 ROSAT survey sources located at low galactic latitudes (|b| < 20 deg). These sources were extracted from the ROSAT Galactic Plane Survey using various selection criteria on hardness…

We present a sample of hard X-ray selected candidate black holes (BHs) in 19 dwarf galaxies. BH candidates are identified by cross-matching a parent sample of ~44,000 local dwarf galaxies (M_stellar < 3 x 10^9 Msun, z<0.055) with the…

Astrophysics of Galaxies · Physics 2015-05-27 Sean Lemons , Amy Reines , Richard Plotkin , Elena Gallo , Jenny Greene

We present the global X-ray properties of the point source population in the grand-design spiral galaxy M101, as seen with XMM-Newton. 108 X-ray sources are detected within the D25 ellipse of M101, of which ~24 are estimated to be…

Astrophysics · Physics 2009-11-10 L. P. Jenkins , T. P. Roberts , R. S. Warwick , R. E. Kilgard , M. J. Ward