We report results of a serendipitous hard X-ray (3-20 keV), nearly all-sky ($|b|>10^\circ$) survey based on RXTE/PCA observations performed during satellite reorientations in 1996-2002. The survey is 80% (90%) complete to a 4σ limiting flux of $\approx $1.8 (2.5) $\times$ 10-11 erg s-1 cm-2 in the 3-20 keV band. The achieved sensitivity in the 3-8 keV and 8-20 keV subbands is similar to and an order of magnitude higher than that of the previously record HEAO-1 A1 and HEAO-1 A4 all-sky surveys, respectively. A combined $7\times 10^3$ sq deg area of the sky is sampled to flux levels below 10-11 erg s-1 cm-2 (3-20 keV). In total 294 sources are detected and localized to better than 1 deg. 236 (80%) of these can be confidently associated with a...
We present the first results from the XMM–Newton Galactic Plane Survey (XGPS). In the first phase of...
Context. The INTEGRAL observatory operating in a hard X-ray/gamma domain has gathered a large observ...
Aims.X-ray sources at intermediate fluxes (a few $\times$ 10-14 erg cm-2 s-1) with a sky density o...
We report results of a serendipitous hard X-ray (3-20 keV), nearly all-sky (absolute value of b grea...
We present results of an all-sky hard X-ray survey based on almost four years of observations with t...
We present a summary of an identification program of the more than 2000 X-ray sources detected durin...
The First Einstein IPC Slew Survey produced a list of 819 x-ray sources, with f(sub x) approximately...
The beginning of X-ray astronomy is based on two accidental discoveries made in 1962. A single point...
Context. The on-going XMM-Newton Slew Survey (XSS) provides coverage of a significant fraction of th...
We present a summary of an identification program of the more than 2000 X-raysources detected during...
This paper is the second in a series devoted to the hard X-ray (17 − 60 keV) whole sky sur...
Abstract. We present a catalog of X-ray sources observed during slew maneuvers by the Medium Energy ...
We have performed a moderately deep soft X-ray ð0:1–2 keVÞ survey of the Galactic plane using pointe...
Hard X-ray selection is the most efficient way to discriminate between accretion-powered sources, su...
Based on RXTE scans and observations with the SWIFT/XRT telescope and INTEGRAL observatory, we repor...
We present the first results from the XMM–Newton Galactic Plane Survey (XGPS). In the first phase of...
Context. The INTEGRAL observatory operating in a hard X-ray/gamma domain has gathered a large observ...
Aims.X-ray sources at intermediate fluxes (a few $\times$ 10-14 erg cm-2 s-1) with a sky density o...
We report results of a serendipitous hard X-ray (3-20 keV), nearly all-sky (absolute value of b grea...
We present results of an all-sky hard X-ray survey based on almost four years of observations with t...
We present a summary of an identification program of the more than 2000 X-ray sources detected durin...
The First Einstein IPC Slew Survey produced a list of 819 x-ray sources, with f(sub x) approximately...
The beginning of X-ray astronomy is based on two accidental discoveries made in 1962. A single point...
Context. The on-going XMM-Newton Slew Survey (XSS) provides coverage of a significant fraction of th...
We present a summary of an identification program of the more than 2000 X-raysources detected during...
This paper is the second in a series devoted to the hard X-ray (17 − 60 keV) whole sky sur...
Abstract. We present a catalog of X-ray sources observed during slew maneuvers by the Medium Energy ...
We have performed a moderately deep soft X-ray ð0:1–2 keVÞ survey of the Galactic plane using pointe...
Hard X-ray selection is the most efficient way to discriminate between accretion-powered sources, su...
Based on RXTE scans and observations with the SWIFT/XRT telescope and INTEGRAL observatory, we repor...
We present the first results from the XMM–Newton Galactic Plane Survey (XGPS). In the first phase of...
Context. The INTEGRAL observatory operating in a hard X-ray/gamma domain has gathered a large observ...
Aims.X-ray sources at intermediate fluxes (a few $\times$ 10-14 erg cm-2 s-1) with a sky density o...