J/ApJ/932/38ivo://CDS.VizieR/J/ApJ/932/38doi:10.26093/cds/vizier.19320038CDSSaikia P.Russell D.M.Baglio M.C.Bramich D.M.Casella P.,Trigo M.D.Gandhi P.Jiang J.Maccarone T.Soria R.Al Noori H.,Al Yazeedi A.Alabarta K.Belloni T.Bel M.C.Ceccobello C.,Corbel S.Fender R.Gallo E.Homan J.Koljonen K.Lewis F.,Markoff S.B.Miller-Jones J.C.A.Rodriguez J.Russell T.D.Shahbaz T.,Sivakoff G.R.Testa V.Tetarenko A.J.2025-09-22T20:10:37Z2025-05-15T12:28:21ZCDS support team

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

cds-question@unistra.frx-ray-binary-starsblack-holestransient-sourcesphotometryvisible-astronomyinfrared-photometryradio-sourcesx-ray-sourcesultraviolet-astronomyWe present a detailed study of the evolution of the Galactic black hole transient GRS 1716-249 during its 2016-2017 outburst at optical (Las Cumbres Observatory), mid-infrared (Very Large Telescope), near-infrared (Rapid Eye Mount telescope), and ultraviolet (the Neil Gehrels Swift Observatory Ultraviolet/Optical Telescope) wavelengths, along with archival radio and X-ray data. We show that the optical/near-infrared and UV emission of the source mainly originates from a multi-temperature accretion disk, while the mid-infrared and radio emission are dominated by synchrotron emission from a compact jet. The optical/UV flux density is correlated with the X-ray emission when the source is in the hard state, consistent with an X-ray irradiated accretion disk with an additional contribution from the viscous disk during the outburst fade. We find evidence for a weak, but highly variable jet component at mid-infrared wavelengths. We also report the long-term optical light curve of the source and find that the quiescent i'-band magnitude is 21.39 +or- 0.15 mag. Furthermore, we discuss how previous estimates of the system parameters of the source are based on various incorrect assumptions, and so are likely to be inaccurate. By comparing our GRS 1716-249 data set to those of other outbursting black hole X-ray binaries, we find that while GRS 1716-249 shows similar X-ray behavior, it is noticeably optically fainter, if the literature distance of 2.4kpc is adopted. Using several lines of reasoning, we argue that the source distance is further than previously assumed in the literature, likely within 4-17kpc, with a most likely range of ~4-8kpc.2022ApJ...932...38Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/932/38CatalogResearchIsServedByTAP VizieR generic servicerelated-toB/eso : ESO Science Archive Catalog (ESO, 1991-2025)B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)V/106 : Catalogue of X-ray binaries (Liu+ 2001)I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)I/358 : Gaia DR3 Part 4. Variability (Gaia Collaboration, 2022)J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009)J/MNRAS/428/2500 : GX 339-4 radio/X-ray flux correlation (Corbel+, 2013)J/ApJS/209/14 : The Swift/BAT hard X-ray transient monitor (Krimm+, 2013)J/A+A/587/A61 : BlackCAT BH in Xray transient (Corral-Santana+, 2016)J/ApJS/222/15 : WATCHDOG: all-sky database of Gal. BHXBs (Tetarenko+, 2016)J/MNRAS/471/1468 : Transient BH X-ray binaries XMM obs. (Eckersall+, 2017)J/ApJ/867/105 : ATLAS all-sky stellar ref. cat. ATLAS-REFCAT2 (Tonry+, 2018)J/A+A/645/A18 : SVOM-ECLAIRs known X-ray sources cat. (Dagoneau+, 2021)J/ApJ/930/20 : Monitoring of neutron star XRB Centaurus X-4 (Baglio+, 2022)J/MNRAS/510/4796 : INTEGRAL/IBIS 17-yr X-ray all-sky survey (Krivonos+, 2022)http://www.sdss.org/ : SDSS home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/932/38https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/932/38http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/932/38https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/932/38https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/932/38http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/932/38GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tap2.381800341673347e-19 4.653515163505597e-19X-rayUVOpticalInfraredRadiodefaultJ/ApJ/932/38/tablea1Faulkes/LCO optical detections of GRS 1716-249recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintiMJD[57781.7/58045.8]? Modified Julian Date of i'-band observationdtime.epoch;obs;em.opt.Idoublenullableimag[15.86/18.11]? Apparent i'-band AB magnitudemagphot.mag;em.opt.Ifloatnullablee_imag[0.003/0.1]? Uncertainty in imagmagstat.error;phot.mag;em.opt.IfloatnullablegMJD[57807.3/58045.8]? Modified Julian Date of g'-band observationdtime.epoch;obs;em.opt.Bdoublenullablegmag[16.9/19.5]? Apparent g'-band AB magnitudemagphot.mag;em.opt.Bfloatnullablee_gmag[0.007/0.1]? Uncertainty in gmagmagstat.error;phot.mag;em.opt.BfloatnullablerMJD[57790.3/57956.7]? Modified Julian Date of r'-band observationdtime.epoch;obs;em.opt.Rdoublenullablermag[16.36/17.64]? Apparent r'-band AB magnitudemagphot.mag;em.opt.Rfloatnullablee_rmag[0.005/0.04]? Uncertainty in rmagmagstat.error;phot.mag;em.opt.RfloatnullableJ/ApJ/932/38/tablea2The Rapid Eye Mount (REM) telescope near-IR detections of GRS 1716-249recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJMJD[57792.3/58025.1]? Modified Julian Date of J-band observationdtime.epoch;obs;em.IR.Jdoublenullablel_Jmag3{sigma} upper limit flag on Jmag when the source was not detectedmeta.code.error;phot.mag;em.IR.JcharJmag[13.16/15.3]? Apparent J-band Vega magnitude (1)magphot.mag;em.IR.Jfloatnullablee_Jmag[0.05/0.3]? Uncertainty in Jmagmagstat.error;phot.mag;em.IR.JfloatnullableHMJD[57792.3/58025.1]? Modified Julian Date of H-band observationdtime.epoch;obs;em.IR.Hdoublenullablel_Hmag3{sigma} upper limit flag on Hmag when the source was not detectedmeta.code.error;phot.mag;em.IR.HcharHmag[13/15.8]? Apparent H-band Vega magnitude (1)magphot.mag;em.IR.Hfloatnullablee_Hmag[0.06/0.3]? Uncertainty in Hmagmagstat.error;phot.mag;em.IR.HfloatnullableKMJD[57792.3/58024.1]? Modified Julian Date of K-band observationdtime.epoch;obs;em.IR.Kdoublenullablel_Kmag3{sigma} upper limit flag on Kmag when the source was not detectedmeta.code.error;phot.mag;em.IR.KcharKmag[12.6/14.33]? Apparent K-band Vega magnitude (1)magphot.mag;em.IR.Kfloatnullablee_Kmag[0.09/0.4]? Uncertainty in Kmagmagstat.error;phot.mag;em.IR.Kfloatnullable