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dc.contributor.author | Kuznetsov, S. | |
dc.contributor.author | Falanga, M. | |
dc.contributor.author | Blay Serrano, Pedro Jose | |
dc.contributor.author | Goldwurm, A. | |
dc.contributor.author | Goldoni, P. | |
dc.contributor.author | Reglero Velasco, Victor | |
dc.date.accessioned | 2010-07-13T08:13:09Z | |
dc.date.available | 2010-07-13T08:13:09Z | |
dc.date.issued | 2003 | |
dc.identifier.citation | KUZNETSOV, S. ; Falanga, M. ; Blay Serrano, Pedro Jose, Goldwurm, A. ; Goldoni, P. ; Reglero Velasco, Victor, 2003, First observations of the X-ray transient EXO 2030+375 with IBIS/ISGRI, Astronomy and Astrophysics, vol. 411, no. 1, p. L437–L440 | en |
dc.identifier.uri | http://hdl.handle.net/10550/16000 | |
dc.description.abstract | We present a first INTEGRAL observation of the 42 s transient X-ray pulsar EXO 2030+375 with IBIS/ISGRI. The source was detected during Cyg X-1 observations in December 2002.We analyzed observations during the outburst period from 9 to 21 December 2002 with a total exposure time of 770 kilosec. EXO 2030+375 was almost always detected during single ~30 min exposures in the 18−45 energy bands. The source light curve shows the characteristic outburst shape observed in this source. | en |
dc.language.iso | en | en |
dc.subject | Gamma rays ; Observations ; X-rays ; Individual ; EXO 2030+375 ; Telescopes ; INTEGRAL ; IBIS | en |
dc.title | First observations of the X-ray transient EXO 2030+375 with IBIS/ISGRI | en |
dc.type | journal article | es_ES |
dc.subject.unesco | UNESCO::ASTRONOMÍA Y ASTROFÍSICA | en |
dc.subject.unesco | UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica | en |
dc.identifier.doi | 10.1051/0004-6361:20031354 | en |
dc.identifier.idgrec | 006163 | en |
dc.type.hasVersion | VoR | es_ES |
dc.identifier.url | http://www.aanda.org/articles/aa/pdf/2003/43/aaINTEGRAL66.pdf | en |