J/A+A/545/A120ivo://CDS.VizieR/J/A+A/545/A120doi:10.26093/cds/vizier.35450120CDSSuleimanov V.Poutanen J.Werner K.2018-01-31T06:09:53Z2012-09-19T09:05:55ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmospheresx-ray-binary-starsTheoretical spectra of X-ray bursting neutron star (NS) model atmospheres are widely used for determination of the NS basic parameters such as their masses and radii. Compton scattering, that plays an important role in spectra formation at high luminosities, is often accounted for using the differential Kompaneets operator, while in other models a more general, integral operator for the Compton scattering kernel is used. We construct here accurate NS atmosphere models using exact treatment of Compton scattering with the integral relativistic kinetic equation and exact relativistic angle-dependent redistribution function.2012A&A...545A.120Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/545/A120CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/527/A139 : X-ray bursting neutron star atmosphere modelshttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/545/A120https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/545/A120http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/545/A120https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/545/A120https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/545/A120http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/545/A120GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/545/A120/setSet parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSet[1/18] Set numbermeta.id;meta.mainintprimaryXX abundance (0, 0.7374, 1)phys.abund.XfloatYY abundance (0, 0.2492, 0.2586, 0.2613, 0.2625, 1)phys.abund.YfloatZZ abundance (0, 1.34E-2, 4.02E-3, 1.34E-3, 1.34E-4)src.redshiftdoubleloggLogarithm of surface gravity (14.0, 14.3, 14.6)log(cm.s**-2)phys.gravityfloatTEddEddington temperature (9 values)keVphys.temperature.effectivefloatRNeutron star radius (8.16, 10.88, 14.80)kmphys.size.radiusfloatzRedshift (0.18, 0.27, 0.42)src.redshiftfloatLumNumber of luminosities for a given setstat.fit.paramintJ/A+A/545/A120/tabled1Color and dilution factorsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSet[1/18] Set numbermeta.id;meta.mainintlRelative luminosity L/L_Edd (1)phys.luminosity;arith.ratiofloatgrad/gRatio of the radiation acceleration to gravitystat.fit.paramfloatTeffEffective temperaturekeVphys.temperature.effectivefloatfc1Color correction factor f_c,1_ (2)arith.factor;phot.fluxfloatfc2Color correction factor f_c,2_ (2)arith.factor;phot.fluxfloatfc3Color correction factor f_c,3_ (2)arith.factor;phot.fluxfloatfc4Color correction factor f_c,4_ (2)arith.factor;phot.fluxfloatfc5Color correction factor f_c,5_ (2)arith.factor;phot.fluxfloatw*fc1+4Product of dilution factor and (fc1)^4^arith.factor;pos.distancefloatw*fc2+4Product of dilution factor and (fc2)^4^arith.factor;pos.distancefloatw*fc3+4Product of dilution factor and (fc3)^4^arith.factor;pos.distancefloatJ/A+A/545/A120/tabled2*Atmosphere model spectra (fluxes)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSetSet numbermeta.id;meta.mainintEPhoton energykeVem.energydoubleF(0001)Flux F_E_ for l=0.001 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0003)Flux F_E_ for l=0.003 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0010)Flux F_E_ for l=0.01 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0030)Flux F_E_ for l=0.03 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0050)Flux F_E_ for l=0.05 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0070)Flux F_E_ for l=0.07 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0100)Flux F_E_ for l=0.1 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0150)Flux F_E_ for l=0.15 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0200)Flux F_E_ for l=0.2 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0300)Flux F_E_ for l=0.3 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0400)Flux F_E_ for l=0.4 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0500)Flux F_E_ for l=0.5 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0550)Flux F_E_ for l=0.55 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0600)Flux F_E_ for l=0.6 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0650)Flux F_E_ for l=0.65 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0700)Flux F_E_ for l=0.7 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0750)Flux F_E_ for l=0.75 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0800)Flux F_E_ for l=0.8 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0850)Flux F_E_ for l=0.85 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0900)Flux F_E_ for l=0.9 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0950)Flux F_E_ for l=0.95 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(0980)Flux F_E_ for l=0.98 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(1000)Flux F_E_ for l=1.0 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(1020)Flux F_E_ for l=1.02 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(1040)Flux F_E_ for l=1.04 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(1060)Flux F_E_ for l=1.06 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoubleF(1080)? Flux F_E_ for l=1.08 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoublenullableF(1100)? Flux F_E_ for l=1.10 (1)mW.m**-2.keV**-1phot.flux;em.X-raydoublenullableJ/A+A/545/A120/tabled3*Atmosphere model spectra (specific intensities)SetSet numbermeta.id;meta.mainintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintEPhoton energykeVem.energydoubleI(0001,0.113)I_E_i at cosi=0.113 for l=0.001 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0001,0.5)I_E_i at cosi=0.5 for l=0.001 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0001,0.887)I_E_i at cosi=0.887 for l=0.001 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0003,0.113)I_E_i at cosi=0.113 for l=0.003 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0003,0.5)I_E_i at cosi=0.5 for l=0.003 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0003,0.887)I_E_i at cosi=0.887 for l=0.003 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0010,0.113)I_E_i at cosi=0.113 for l=0.01 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0010,0.5)I_E_i at cosi=0.5 for l=0.01 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0010,0.887)I_E_i at cosi=0.887 for l=0.01 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0030,0.113)I_E_i at cosi=0.113 for l=0.03 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0030,0.5)I_E_i at cosi=0.5 for l=0.03 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0030,0.887)I_E_i at cosi=0.887 for l=0.03 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0050,0.113)I_E_i at cosi=0.113 for l=0.05 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0050,0.5)I_E_i at cosi=0.5 for l=0.05 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0050,0.887)I_E_i at cosi=0.887 for l=0.05 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0070,0.113)I_E_i at cosi=0.113 for l=0.07 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0070,0.5)I_E_i at cosi=0.5 for l=0.07 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0070,0.887)I_E_i at cosi=0.887 for l=0.07 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0100,0.113)I_E_i at cosi=0.113 for l=0.1 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0100,0.5)I_E_i at cosi=0.5 for l=0.1 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0100,0.887)I_E_i at cosi=0.887 for l=0.1 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0150,0.113)I_E_i at cosi=0.113 for l=0.15 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0150,0.5)I_E_i at cosi=0.5 for l=0.15 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0150,0.887)I_E_i at cosi=0.887 for l=0.15 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0200,0.113)I_E_i at cosi=0.113 for l=0.2 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0200,0.5)I_E_i at cosi=0.5 for l=0.2 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0200,0.887)I_E_i at cosi=0.887 for l=0.2 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0300,0.113)I_E_i at cosi=0.113 for l=0.3 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0300,0.5)I_E_i at cosi=0.5 for l=0.3 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0300,0.887)I_E_i at cosi=0.887 for l=0.3 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0400,0.113)I_E_i at cosi=0.113 for l=0.4 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0400,0.5)I_E_i at cosi=0.5 for l=0.4 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0400,0.887)I_E_i at cosi=0.887 for l=0.4 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0500,0.113)I_E_i at cosi=0.113 for l=0.5 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0500,0.5)I_E_i at cosi=0.5 for l=0.5 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0500,0.887)I_E_i at cosi=0.887 for l=0.5 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0550,0.113)I_E_i at cosi=0.113 for l=0.55 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0550,0.5)I_E_i at cosi=0.5 for l=0.55 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0550,0.887)I_E_i at cosi=0.887 for l=0.55 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0600,0.113)I_E_i at cosi=0.113 for l=0.6 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0600,0.5)I_E_i at cosi=0.5 for l=0.6 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0600,0.887)I_E_i at cosi=0.887 for l=0.6 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0650,0.113)I_E_i at cosi=0.113 for l=0.65 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0650,0.5)I_E_i at cosi=0.5 for l=0.65 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0650,0.887)I_E_i at cosi=0.887 for l=0.65 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0700,0.113)I_E_i at cosi=0.113 for l=0.7 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0700,0.5)I_E_i at cosi=0.5 for l=0.7 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0700,0.887)I_E_i at cosi=0.887 for l=0.7 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0750,0.113)I_E_i at cosi=0.113 for l=0.75 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0750,0.5)I_E_i at cosi=0.5 for l=0.75 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0750,0.887)I_E_i at cosi=0.887 for l=0.75 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0800,0.113)I_E_i at cosi=0.113 for l=0.8 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0800,0.5)I_E_i at cosi=0.5 for l=0.8 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0800,0.887)I_E_i at cosi=0.887 for l=0.8 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0850,0.113)I_E_i at cosi=0.113 for l=0.85 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0850,0.5)I_E_i at cosi=0.5 for l=0.85 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0850,0.887)I_E_i at cosi=0.887 for l=0.85 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0900,0.113)I_E_i at cosi=0.113 for l=0.9 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0900,0.5)I_E_i at cosi=0.5 for l=0.9 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0900,0.887)I_E_i at cosi=0.887 for l=0.9 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0950,0.113)I_E_i at cosi=0.113 for l=0.95 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0950,0.5)I_E_i at cosi=0.5 for l=0.95 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0950,0.887)I_E_i at cosi=0.887 for l=0.95 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0980,0.113)I_E_i at cosi=0.113 for l=0.98 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0980,0.5)I_E_i at cosi=0.5 for l=0.98 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(0980,0.887)I_E_i at cosi=0.887 for l=0.98 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1000,0.113)I_E_i at cosi=0.113 for l=1.0 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1000,0.5)I_E_i at cosi=0.5 for l=1.0 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1000,0.887)I_E_i at cosi=0.887 for l=1.0 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1020,0.113)I_E_i at cosi=0.113 for l=1.02 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1020,0.5)I_E_i at cosi=0.5 for l=1.02 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1020,0.887)I_E_i at cosi=0.887 for l=1.02 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1040,0.113)I_E_i at cosi=0.113 for l=1.04 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1040,0.5)I_E_i at cosi=0.5 for l=1.04 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1040,0.887)I_E_i at cosi=0.887 for l=1.04 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1060,0.113)I_E_i at cosi=0.113 for l=1.06 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1060,0.5)I_E_i at cosi=0.5 for l=1.06 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1060,0.887)I_E_i at cosi=0.887 for l=1.06 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoubleI(1080,0.113)? I_E_i at cosi=0.113 for l=1.08 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoublenullableI(1080,0.5)? I_E_i at cosi=0.5 for l=1.08 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoublenullableI(1080,0.887)? I_E_i at cosi=0.887 for l=1.08 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoublenullableI(1100,0.113)? I_E_i at cosi=0.113 for l=1.1 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoublenullableI(1100,0.5)? I_E_i at cosi=0.5 for l=1.1 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoublenullableI(1100,0.887)? I_E_i at cosi=0.887 for l=1.1 (1)mW.m**-2.keV**-1.sr**-1phot.fluxdoublenullable