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相关论文: Identification of selected sources from the ROSAT …

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The optical identification of large number of X-ray sources such as those from the ROSAT All-Sky Survey is challenging with conventional spectroscopic follow-up observations. We investigate two ROSAT All-Sky Survey fields of size 10 * 10…

高能天体物理现象 · 物理学 2015-02-25 J. Greiner , G. A. Richter

We present a summary of an identification program of the more than 2000 X-ray sources detected during the ROSAT All-Sky Survey (Voges et al. 1999) at high galactic latitude, |b| > 30 degr, with countrate above 0.2 s-1. This program, termed…

In the construction of an X-ray selected sample of galaxy clusters for cosmological studies, we have assembled a sample of 495 X-ray sources found to show extended X-ray emission in the first processing of the ROSAT All-Sky Survey. The…

We present the statistical evaluation of a count rate and area limited complete sample of the ROSAT All-Sky Survey (RASS) comprising 674 sources. The RASS sources are located in six study areas outside the galactic plane (|b^II| >= 20 deg)…

The ROSAT Bright Survey (RBS) aims to completely optically identify the more than 2000 brightest sources detected in the ROSAT all-sky survey at galactic latitudes |b| > 30 degr (excluding LMC, SMC, Virgo cluster). This paper presents a…

天体物理学 · 物理学 2015-06-24 J. -U. Fischer , G. Hasinger , A. D. Schwope , H. Brunner , Th. Boller , J. Truemper , W. Voges , S. Neizvestny

The ROSAT Deep Survey includes a complete sample of 50 X-ray sources with fluxes in the $0.5 - 2$ keV band larger than 5.5 $10^{-15}$ erg cm$^{-2}$ s$^{-1}$ in the Lockman field (Hasinger et al., Paper I). We have obtained deep broad-band…

We have identified a population of blank field sources (or `blanks') among the ROSAT bright unidentified X-ray sources with faint optical counterparts. The extreme X-ray over optical flux ratio of blanks is not compatible with the main…

天体物理学 · 物理学 2009-11-07 Ilaria Cagnoni , Martin Elvis , Dong-Woo Kim , Fabrizio Nicastro , Annalisa Celotti

We present the ROSAT All-Sky Survey Bright Source Catalogue (RASS-BSC, revision 1RXS) derived from the all-sky survey performed during the first half year (1990/91) of the ROSAT mission. 18,811 sources are catalogued (i) down to a limiting…

The IBIS/ISGRI first year galactic plane survey has produced a catalogue containing 123 hard X-ray sources visible down to a flux limit of a few milliCrabs. The point source location accuracy of typically 1-3 arcminutes has allowed the…

天体物理学 · 物理学 2009-11-10 J. B. Stephen , L. Bassani , M. Molina , A. Malizia , A. Bazzano , P. Ubertini , A. J. Dean , A. J. Bird , R. Much , R. Walter

We present optical candidates for 75 X-ray sources in a $\sim 1$ deg$^2$ overlapping region with the medium deep ROSAT survey. These candidates are selected using the multi-color CCD imaging observations made for the T329 field of the…

天体物理学 · 物理学 2013-04-29 Haotong Zhang , Suijian Xue , David Burstein , Xu Zhou , Zhaoji Jiang , Hong Wu , Jun Ma , Jiansheng Chen , Zhenlong Zou

The ROSAT ALL Sky Survey Bright Source Catalogue (RASS-BSC) has been correlated with the Catalogue of Principal Galaxies (PGC) to identify new extragalactic counterparts. 550 reliable optical counterparts have been detected. We took optical…

天体物理学 · 物理学 2009-11-13 W. Kollatschny , R. Kotulla , W. Pietsch , K. Bischoff , M. Zetzl

We present the X-ray data and the optical identifications for a deep ROSAT PSPC observation in the "Marano field". In the inner region of the ROSAT field (15' radius) we detected 50 X-ray sources with Sx >= 3.7x10^(-15) erg/cm^2/s. When…

天体物理学 · 物理学 2007-05-23 G. Zamorani , M. Mignoli , G. Hasinger , R. Burg , R. Giacconi , M. Schmidt , J. Trumper , P. Ciliegi , C. Gruppioni , B. Marano

A complete sample of bright ROSAT sources with hard XRB-like spectra in the Galactic Plane (|b| < 15 deg.) has been tentatively identified with radio sources in the GB6/PMN/NVSS surveys, and subsequently observed with the Australia…

天体物理学 · 物理学 2007-05-23 G. S. Tsarevsky , E. P. Pavlenko , R. A. Stathakis , N. S. Kardashev , O. B. Slee

We describe further results of a program aimed to yield ~10^4 fully characterized optical identifications of ROSAT X-ray sources. Our program employs X-ray data from the ROSAT All-Sky Survey (RASS), and both optical imaging and…

We present a systematic search for variability among the ROSAT All-Sky Survey (RASS) X-ray sources. We generated lightcurves for about 30000 X-ray point sources detected sufficiently high above background. For our variability study…

天体物理学 · 物理学 2009-11-07 B. Fuhrmeister , J. H. M. M. Schmitt

The second IBIS/ISGRI survey has produced a catalogue containing 209 hard X-ray sources visible down to a flux limit of around 1 milliCrab. The point source location accuracy of typically 1-3 arcminutes has allowed the counterparts for most…

天体物理学 · 物理学 2009-11-11 J. B. Stephen , L. Bassani , A. Malizia , A. Bazzano , P. Ubertini , A. J. Bird , A. J. Dean , F. Lebrun , R. Walter

The North-Ecliptic Pole is an important region for extragalactic surveys. Deep/wide contiguous surveys are being performed by several space observatories. We analyse all ROSAT pointed and survey observations within 40 deg2 around the NEP,…

宇宙学与河外天体物理 · 物理学 2021-01-20 G. Hasinger , M. Freyberg , E. M. Hu , C. Z. Waters , P. Capak , A. Moneti , H. J. McCracken

We report the discovery of several new OB/X-ray accreting binary candidates. These massive systems were found by cross-correlating in position SIMBAD OB star catalogues with the part of the ROSAT all-sky survey located at low galactic…

天体物理学 · 物理学 2016-08-30 C. Motch , F. Haberl , K. Dennerl , M. Pakull , E. Janot-Pacheco

We selected a sample of sources with high X-ray over optical flux ratio from the ROSAT PSPC archives. Out of the 16 sources in our sample, one is a (possibly extreme) BL Lac and two are AGNs. Six more sources are tentatively classified as…

天体物理学 · 物理学 2007-05-23 I. Cagnoni , M. Elvis , D. -W. Kim , J. -S. Huang , A. Celotti , F. Nicastro

We have surveyed 188 ROSAT PSPC fields for X-ray sources with hard spectra (alpha<0.5); such sources must be major contributors to the X-ray background at faint fluxes. In this paper we present optical identifications for 62 of these…

天体物理学 · 物理学 2009-11-06 M. J. Page , J. P. D. Mittaz , F. J. Carrera
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