J/MNRAS/422/679ivo://CDS.VizieR/J/MNRAS/422/679doi:10.26093/cds/vizier.74220679CDSStiele H.Munoz-Darias T.Motta S.Belloni T.M.2024-07-17T20:15:53Z2013-01-18T13:52:42ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frx-ray-sourcesx-ray-binary-starsastronomical-modelsWe report on a spectral-timing analysis of the black hole X-ray binary candidate MAXI J1543-564 during its 2011 outburst. All 99 pointed observations of this outburst obtained with the Rossi X-ray Timing Explorer (RXTE) were included in our study. We computed the fundamental diagrams commonly used to study black hole transients, and fitted power density and energy spectra to study the spectral and timing parameters along the outburst. The determination of timing parameters and hence of exact transitions between different states was hampered by the rather low count rate at which this outburst was observed. We detected two periods of exponential decay, one after the source was brightest, which was interrupted by several flares, and another one during the high soft state. The detection of these decays allowed us to obtain an estimate for the source distance of at least 8.5kpc. This leaves two possible explanations for the observed low count rate; either the source has a distance similar to that of other black hole X-ray binary candidates and it is intrinsically faint, or it has a similar luminosity, but is located more than 12 kpc away from us. Furthermore, in the high/soft state the source spectrum appears to be completely disc dominated.2012MNRAS.422..679Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/422/679CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/422/679https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/422/679http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/422/679https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/422/679https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/422/679http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/422/679GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapX-raydefaultJ/MNRAS/422/679/table2*Spectral parameters derived from the best fit for each observation.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential number of observationmeta.recordintObsIDRXTE Observation IDmeta.id;obscharDayTime since the first observation (MJD-55691.1)dobs.param;obsfloatMJDModified Julian date of observationdtime.epochfloatchi2Reduced {chi}^2^stat.fit.chi2floatdiskbbNormalised disc blackbody model parameter (Mitsuda et al. 1984PASJ...36..741M)stat.param;meta.modelledfloatE_diskbbError on diskbb (upper value)stat.error;stat.maxfloate_diskbbError on diskbb (lower value)stat.errorfloatTinInner disc temperaturelog(keV)phys.temperaturefloatE_TinError on Tin (upper value)log(keV)stat.error;stat.maxfloate_TinError on Tin (lower value)log(keV)stat.errorfloatGammaPhoton index {Gamma}meta.code;spect.indexfloatE_Gamma? Error on Gamma (upper value)stat.error;stat.maxfloatnullablee_Gamma? Error on Gamma (lower value)stat.errorfloatnullablefSctr[0/1] Fraction of up-scattered radiationstat.fit.paramfloatE_fSctrError on fSctr (upper value)stat.error;stat.maxfloate_fSctrError on fSctr (lower value)stat.errorfloat