activity
20032012
most citedXMM-Newton observations of PSr B1259-63 near the 2004 periastron passage

100 citations · 184 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2012★ 7 cited

Search for variable gamma-ray emission from the Galactic plane in the Fermi data

A. Neronov, D. Malyshev, M. Chernyakova +1

High-energy gamma-ray emission from the Galactic plane above ~100 MeV is composed of three main contributions: diffuse emission from cosmic ray interactions in the interstellar med…

astro-ph.HE2012★ 35 cited

Superorbital modulation of X-ray emission from gamma-ray binary LSI +61 303

M. Chernyakova, A. Neronov, S. Molkov +3

We report the discovery of a systematic constant time lag between the X-ray and radio flares of the gamma-ray binary LSI +61 303, persistent over long, multi-year, time scale. Usin…

astro-ph2006★ 100 cited

XMM-Newton observations of PSr B1259-63 near the 2004 periastron passage

M. Chernyakova, A. Neronov, A. Lutovinov +2

PSR B1259-63 is in a highly eccentric 3.4 year orbit with a Be star and crosses the Be star disc twice per orbit, just prior to and just after periastron. Unpulsed radio, X-ray and…

astro-ph2005★ 35 cited

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…

astro-ph2004

INTEGRAL and RXTE observations of broad-line radio galaxy 3C 111

M. Chernyakova, P. Favre, T. J. -L. Courvoisier +8

3C 111 is an X-ray bright broad-line radio galaxy which is classified as a Fanaroff-Riley type II source with a double-lobe/single jet morphology, and reported superluminal motion.…

astro-ph2003★ 7 cited

First INTEGRAL Observations of Eight Persistent Neutron Star Low Mass X-ray Binaries

A. Paizis, V. Beckmann, T. J. -L. Courvoisier +16

Early results from the INTEGRAL Core Program, for a sample of eight persistently bright neutron star low mass X-ray binaries in the energy range from 5 keV to 200 keV are presented…