J/A+A/625/A66ivo://CDS.VizieR/J/A+A/625/A66doi:10.26093/cds/vizier.36250066CDSDionatos O.Woitke P.Guedel M.Degroote P.Liebhart A.Anthonioz F.,Antonellini S.Baldovin-Saavedra C.Carmona A.Dominik C.Greaves J.,Ilee J.D.Kamp I.Menard F.Min M.Pinte C.Rab C.Rigon L.,Thi W.F.Waters L.B.F.M.2021-05-19T09:40:18Z2019-05-17T11:49:35ZCDS support team

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

cds-question@unistra.frpre-main-sequence-starsaccretionspectroscopyx-ray-sourcesConsistent modeling of protoplanetary disks requires the simultaneous solution of both continuum and line radiative transfer, heating and cooling balance between dust and gas and, of course, chemistry. Such models depend on panchromatic observations that can provide a complete description of the physical and chemical properties and energy balance of protoplanetary systems. Along these lines we present a homogeneous, panchromatic collection of data on a sample of 85 T Tauri and Herbig Ae objects for which data cover a range from X-rays to centimeter wavelengths. Datasets consist of photometric measurements, spectra, along with results from the data analysis such as line fluxes from atomic and molecular transitions. Additional properties resulting from modeling of the sources such as disc mass and shape parameters, dust size and PAH properties are also provided for completeness. The purpose of this data collection is to provide a solid base that can enable consistent modeling of the properties of protoplan- etary disks. To this end, we performed an unbiased collection of publicly available data that were combined to homogeneous datasets adopting consistent criteria. Targets were selected based on both their properties but also on the availability of data. Data from more than 50 different telescopes and facilities were retrieved and combined in homogeneous datasets directly from public data archives or after being extracted from more than 100 published articles. X-ray data for a subset of 56 sources represent an exception as they were reduced from scratch and are presented here for the first time. Compiled datasets along with a subset of continuum and emission-line models are stored in a dedicated database and distributed through a publicly accessible online system. All datasets contain metadata descriptors that allow to backtrack them to their original resources. The graphical user interface of the online system allows the user to visually inspect individual objects but also compare between datasets and models. It also offers to the user the possibility to download any of the stored data and metadata for further processing.2019A&A...625A..66Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/625/A66CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/625/A66https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/625/A66http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/625/A66https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/625/A66https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/625/A66http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/625/A66GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/625/A66/xray_obs (List of X-ray observations)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/625/A66/xray_obs?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/625/A66/xray_obs?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/625/A66/xray_obs?GETtext/xml+votable180.050000true69.61916726.1803890.005555555555555556Cone search capability for table J/A+A/625/A66/table4 (Model results of X-ray spectra (corrected version, 18-May-2021))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/625/A66/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/625/A66/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/625/A66/table4?GETtext/xml+votable180.050000true276.124167-29.7803610.0055555555555555566/342 1029 1031 1039 1048 1050 1052 1054 1073-1075 1082 1111 1113-1114 1136 1169-1171 23548-23549 23551 24201 28762 28921 29519 30733 36948 36956-36957 37012 37128 37186 38382 38687 42595 42605 42610 42704 42736 42970 42972 42981 44049 44362 44379 47828https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/625/A66?format=asciiX-raydefaultJ/A+A/625/A66/xray_obsList of X-ray observationsNameSource namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000.0)pos.eq.ra;meta.mainDEJ2000Declination (J2000.0)pos.eq.dec;meta.mainInstInstrument (XMM-Newton or Chandra)meta.id;instrcharObsIdObservation identificationmeta.id;obs.param;obsIntTimeIntegration time (seconds)sectime.epochdoubleSimbadSimbad column added by the CDSmeta.ref.urlcharJ/A+A/625/A66/table4Model results of X-ray spectra (corrected version, 18-May-2021)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource namemeta.id;meta.maincharRAJ2000Right ascension (J2000.0)pos.eq.ra;meta.mainDEJ2000Declination (J2000.0)pos.eq.dec;meta.mainCDColumn Densitycm**-2phys.columnDensitydoubleFluxFluxmW.m**-2phot.flux;em.X-raydoubleFluxSFlux softmW.m**-2phot.flux;em.X-raydoubleFluxHFlux hardmW.m**-2phot.flux;em.X-raydoubleh1Hardnessphot.fluxfloatFabsFlux absorbedmW.m**-2phot.flux;em.X-raydoubleFabsSFlux absorbed softmW.m**-2phot.flux;em.X-raydoubleFabsHFlux absorbed hardmW.m**-2phot.flux;em.X-raydoubleh2Hardness absorbedphot.fluxfloatT1Temperature component 1Kphys.temperaturedoubleT2Temperature component 2Kphys.temperaturedouble