J/A+A/513/A21ivo://CDS.VizieR/J/A+A/513/A21doi:10.26093/cds/vizier.35130021CDSMassaro E.Ventura G.Massa F.Feroci M.Mineo T.Cusumano G.,Casella P.Belloni T.2017-10-09T13:34:06Z2010-05-10T09:45:23ZCDS support team

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

cds-question@unistra.frquasarsx-ray-sourcesaccretionGRS 1915+105 was observed by BeppoSAX for about 10 days in October 2000. For about 80% of the time, the source was in the variability class rho, characterised by a series of recurrent bursts. We describe the results of the timing analysis performed on the MECS (1.6-10keV) and PDS (15-100keV) data. The X-ray count rate from GRS 1915+105 showed an increasing trend with different characteristics in the various energy bands: in the bands (1.6-3keV) and (15-100keV), it was nearly stable in the first part of the pointing and increased in a rather short time by about 20%, while in the energy range (3-10keV) the increase had a smoother trend.2010A&A...513A..21Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/513/A21CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/397/711 : Comptonization and reflection in GRS 1915+105 (Rau+, 2003)J/ApJ/657/409 : K-band light curve of GRS 1915+105 (Neil+, 2007)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/513/A21https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/513/A21http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/513/A21https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/513/A21https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/513/A21http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/513/A21GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapX-raydefaultJ/A+A/513/A21/tablea2Initial times and multiplicity of burstsNburstsNumber of complete burstsmeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeriesSeries codemeta.id;meta.maincharprimaryn_SeriesSimbad column added by the CDSmeta.ref.urlcharTimeInitial time, origin is 20 October 2000 at UT=21h26m55sstime.epochdoubleDurDuration of burststime.intervalfloatCt(1.6-10)MECS (1.6-10keV) mean count rate [energy channels 36-220]ctphot.count;em.X-rayfloatCt(1.6-3)MECS (1.6-3.0keV) mean count rate [energy channels 36-66]ctphot.count;em.X-rayfloatCt(3-5)MECS (3.0-5.0keV) mean count rate [energy channels 67-110]ctphot.count;em.X-rayfloatCt(5-10)MECS (5.0-10keV) mean count rate [energy channels 110-220]ctphot.count;em.X-rayfloatCt(15-150)? PDS (15-150keV) mean count ratectphot.count;em.X-rayfloatnullableNp1Number of p1 burstsmeta.numberintNp2Number of p2 burstsmeta.numberintNp3Number of p3 burstsmeta.numberintNp4Number of p4 burstsmeta.numberintNp>4Number of p>4 burstsmeta.numberintN<p>Mean burst multiplicitymeta.numberfloatNabNumber of anomalous burstsmeta.numberintJ/A+A/513/A21/tablea3Results of the Fourier and wavelet spectral analysisrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeriesSeries codemeta.id;meta.maincharP1/P2? P1/P2 power ratio of two highest peaksphot.flux;arith.ratiofloatnullableTrec? Recurrence time of the unique (for the S series) or the first (for the T series) dominant peakstime.intervalfloatnullableTrec2? Recurrence time of the second dominant peak (for the T series)stime.intervalfloatnullableTrec3? Recurrence time of the centroid (for the M series)stime.intervalfloatnullableWidth? Interval width (for the M series)stime.intervalfloatnullableDeltatTemporal resolution at the peakstime.resolutionfloat<Tmax>Time scale of the maximum in the wavelet spectrastime.scalefloatRwRatio Rw (=sigma_T_/<Tmax>) of the standard deviation of the T_J,max_ to its mean value across the series (1)%src.var.indexfloatTypeS, T or M series classificationsrc.classchar