The INTEGRAL Galactic Bulge monitoring program

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dc.creatorKuulkers, E.
dc.creatorShaw, S.
dc.creatorBrandt, S.
dc.creatorChenevez, J.
dc.creatorCourvoisier, T. J. -L.
dc.creatorEbisawa, K.
dc.creatorKretschmar, P.
dc.creatorMarkwardt, C.
dc.creatorMowlavi, N.
dc.creatorOosterbroek, T.
dc.creatorOrr, A.
dc.creatorPaizis, A.
dc.creatorSanchez-Fernandez, C.
dc.creatorWijnands, R.
dc.date2006-03-06
dc.date.accessioned2026-07-07T10:27:57Z
dc.date.available2026-07-07T10:27:57Z
dc.descriptionThe Galactic Bulge region is a rich host of variable high-energy point sources. These sources include bright and relatively faint X-ray transients, X-ray bursters, persistent neutron star and black-hole candidate binaries, X-ray pulsars, etc.. We have a program to monitor the Galactic Bulge region regularly and frequently with the gamma-ray observatory INTEGRAL. As a service to the scientific community the high-energy light curves of all the active sources as well as images of the region are made available through the WWW. We show the first results of this exciting new program.
dc.description5 pages, 2 figures, to be published in: "The Transient Milky Way: a perspective for MIRAX", eds. F. D'Amico, J. Braga & R. Rothschild, AIP Conf. Proc
dc.identifierhttps://arxiv.org/abs/astro-ph/0603130
dc.identifierhttp://arxiv.org/abs/astro-ph/0603130
dc.identifierAIPConf.Proc.840:30-34,2006
dc.identifierdoi:10.1063/1.2216598
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177289
dc.subjectAstrophysics
dc.titleThe INTEGRAL Galactic Bulge monitoring program
dc.typetext

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