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20032008
most citedINTEGRAL observations of the cosmic X-ray background in the 5-100 keV range via occultation by the Earth

196 citations · 324 across the 5 of their papers we have counts for

collaborators

16 papers

astro-ph200825 cited

X-ray observations of the Coma Cluster in a broad energy band with INTEGRAL, RXTE, and ROSAT observatories

A. A. Lutovinov, A. Vikhlinin, E. M. Churazov +2

We present results of X-ray observations of the Coma cluster with multiple instruments over a broad energy band. Using the data from INTEGRAL, RXTE and ROSAT observatories, we find…

astro-ph200750 cited

X-ray emission from the stellar population in M32

M. Revnivtsev, E. Churazov, S. Sazonov +2

Using Chandra observations, we study the X-ray emission of the stellar population in the compact dwarf elliptical galaxy M32. The proximity of M32 allows one to resolve all bright…

astro-ph200629 cited

Diagnostics of the black hole candidate SS433 with the RXTE

E. Filippova, M. Revnivtsev, S. Fabrika +2

We present our analysis of the extensive monitoring of SS433 by the RXTE observatory collected over the period 1996-2005. The difference between energy spectra taken at different p…

astro-ph2006196 cited

INTEGRAL observations of the cosmic X-ray background in the 5-100 keV range via occultation by the Earth

E. Churazov, R. Sunyaev, M. Revnivtsev +32

We study the spectrum of the cosmic X-ray background (CXB) in energy range 5-100 keV. Early in 2006 the INTEGRAL observatory performed a series of four 30ksec observations wi…

astro-ph200624 cited

XSS J00564+4548 and IGR J00234+6141 -- new cataclysmic variables from RXTE and INTEGRAL all sky surveys

I. F. Bikmaev, M. G. Revnivtsev, R. A. Burenin +1

We present the results of optical identification of two X-ray sources from RXTE and INTEGRAL all sky surveys: XSS J00564+4548 and IGR J00234+6141. Using the optical data from Russi…

astro-ph2005

Discovery and study of the accreting pulsar 2RXP J130159.6-635806

M. Chernyakova, A. Lutovinov, J. Rodriguez +1

We report on analysis of the poorly studied source 2RXP J130159.6-635806 at different epochs with ASCA, Beppo-SAX, XMM-Newton, and INTEGRAL. The source shows coherent X-ray pulsati…