0000000000609596

AUTHOR

Juan J. Rodriguez

showing 2 related works from this author

X-RAY AND OPTICAL OBSERVATIONS OF A 0535+26

2011

We present recent contemporaneous X-ray and optical observations of the Be/X-ray binary system A\,0535+26 with the \textit{Fermi}/Gamma-ray Burst Monitor (GBM) and several ground-based observatories. These new observations are put into the context of the rich historical data (since $\sim$1978) and discussed in terms of the neutron star Be-disk interaction. The Be circumstellar disk was exceptionally large just before the 2009 December giant outburst, which may explain the origin of the unusual recent X-ray activity of this source. We found a peculiar evolution of the pulse profile during this giant outburst, with the two main components evolving in opposite ways with energy. A hard 30-70 mH…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsBrightnessOscillationAstrophysics::High Energy Astrophysical PhenomenaX-rayFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)AstrophysicsNeutron starSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsGeneral patternAstrophysics - High Energy Astrophysical PhenomenaLine (formation)Fermi Gamma-ray Space TelescopeThe Astrophysical Journal
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The INTEGRAL IBIS/ISGRI System Point Spread Function and Source Location Accuracy

2003

The imager on board INTEGRAL (IBIS) presently provides the most detailed sky images ever obtained at energies above 30 keV. The telescope is based on a coded aperture imaging system which allows to obtain sky images in a large field of view 29deg x 29deg with an angular resolution of 12'. The System Point Spread Function of the telescope and its detailed characteristics are here described along with the specific analysis algorithms used to derive the accurate point-like source locations. The derived location accuracy is studied using the first in-flight calibration data on strong sources for the IBIS/ISGRI system. The dependence of the calibrated location accuracy with the signal to noise r…

Point spread functionAstrophysics::High Energy Astrophysical PhenomenaData analysisFOS: Physical sciencesImage processingField of viewAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAlaw.inventionTelescopeHigh angular resolutionSignal-to-noise ratioImage processinglawData analysis ; Image processing ; High angular resolutionAngular resolutionCoded aperture:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]Remote sensingIbisPhysicsbiologyUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsbiology.organism_classificationSpace and Planetary Science:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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