INTEGRAL-RXTE observations of Cygnus X-1
dc.contributor.author | Pottschmidt, Katja | |
dc.contributor.author | Wilms, J. | |
dc.contributor.author | Chernyakova, M. | |
dc.contributor.author | Nowak, M. A. | |
dc.contributor.author | Rodriguez, J. | |
dc.contributor.author | Zdziarski, A. A. | |
dc.contributor.author | Beckmann, V. | |
dc.contributor.author | Kretschmar, P. | |
dc.contributor.author | Gleissner, T. | |
dc.contributor.author | Pooley, G. G. | |
dc.contributor.author | Martínez-Núñez, S. | |
dc.contributor.author | Courvoisier, T. J.-L. | |
dc.contributor.author | Schönfelder, V. | |
dc.contributor.author | Staubert, R. | |
dc.date.accessioned | 2023-10-12T21:50:43Z | |
dc.date.available | 2023-10-12T21:50:43Z | |
dc.date.issued | 2003-11-17 | |
dc.description.abstract | We present first results from contemporaneous observations of Cygnus X-1 with INTEGRAL and RXTE, made during INTEGRAL’s performance verification phase in 2002 November and December. Consistent with earlier results, the 3−250 keV data are well described by Comptonization spectra from a Compton corona with a temperature of kT ∼ 50−90 keV and an optical depth of τ ∼ 1.0−1.3 plus reflection from a cold or mildly ionized slab with a covering factor of Ω/2π ∼ 0.2−0.3. A soft excess below 10 keV, interpreted as emission from the accretion disk, is seen to decrease during the 1.5 months spanned by our observations. Our results indicate a remarkable consistency among the independently calibrated detectors, with the remaining issues being mainly related to the flux calibration of INTEGRAL. | en_US |
dc.description.sponsorship | This work has been financed by Deutsches Zentrum f¨ur Luft- und Raumfahrt grants 50 OG 95030 and 50 OG 9601, Deutsche Forschungsgemeinschaft grant Sta 173/25-3, National Science Foundation grant INT-0233441, National Aeronautics and Space Administration grant NAS8-01129, Deutscher Akademischer Austauschdienst grant D/0247203, KBN grants 5P03D00821, 2P03C00619p1,2, and PBZ-054/P03/2001, as well as the French Space Agency (CNES) and the Foundation for Polish Science. We thank all people involved in building and calibrating INTEGRAL for their efforts, and E. Smith and J. Swank for the very smooth scheduling of the RXTE observations. We would also like to thank Paolo Coppi, the referee, for helpful suggestions. | en_US |
dc.description.uri | https://www.aanda.org/articles/aa/abs/2003/43/aaINTEGRAL26/aaINTEGRAL26.html | en_US |
dc.format.extent | 6 pages | en_US |
dc.genre | journal articles | en_US |
dc.identifier | doi:10.13016/m2e3kk-8ory | |
dc.identifier.citation | Pottschmidt, K., J. Wilms, M. Chernyakova, M. A. Nowak, J. Rodriguez, A. A. Zdziarski, V. Beckmann, et al. “INTEGRAL-RXTE Observations of Cygnus X-1.” Astronomy & Astrophysics 411, no. 1 (November 1, 2003): L383–88. https://doi.org/10.1051/0004-6361:20031258. | en_US |
dc.identifier.uri | https://doi.org/10.1051/0004-6361:20031258 | |
dc.identifier.uri | http://hdl.handle.net/11603/30127 | |
dc.language.iso | en_US | en_US |
dc.publisher | EDP Sciences | en_US |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Center for Space Sciences and Technology | |
dc.relation.ispartof | UMBC Physics Department | |
dc.rights | This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author. | en_US |
dc.rights | Attribution 4.0 International (CC BY 4.0) | * |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | * |
dc.title | INTEGRAL-RXTE observations of Cygnus X-1 | en_US |
dc.type | Text | en_US |
dcterms.creator | https://orcid.org/0000-0002-4656-6881 | en_US |