carmenes SSAPivo://org.gavo.dc/carmenes/q/ssaThe GAVO DC teamRibas, I.Reiners, A.Zechmeister, M.A. Caballero, J.C. Morales, J.Sabotta, S.Baroch, D.J. Amado, P.Quirrenbach, A.Abril, M.Aceituno, J.Anglada-Escudé, G.Azzaro, M.Barrado, D.J. S. Béjar, V.Benítez de Haro, D.Bergond, G.Bluhm, P.Calvo Ortega, R.Cardona Guillén, C.Chaturvedi, P.Cifuentes, C.Colomé, J.Cont, D.Cortés-Contreras, M.Czesla, S.Díez-Alonso, E.Dreizler, S.Duque-Arribas, C.Espinoza, N.Fernández, M.Fuhrmeister, B.Galadí-Enríquez, D.García-López, A.González-Álvarez, E.I. González Hernández, J.W. Guenther, E.de Guindos, E.P. Hatzes, A.Henning, Th.Herrero, E.Hintz, D.L. Huelmo, Á.V. Jeffers, S.N. Johnson, E.de Juan, E.Kaminski, A.Kemmer, J.Khaimova, J.Khalafinejad, S.Kossakowski, D.Kürster, M.Labarga, F.Lafarga, M.Lalitha, S.Lampón, M.Lillo-Box, J.Lodieu, N.J. López González, M.López-Puertas, M.Luque, R.Magán, H.Mancini, L.Marfil, E.L. Martín, E.Martín-Ruiz, S.Molaverdikhani, K.Montes, D.Nagel, E.Nortmann, L.Nowak, G.Pallé, E.M. Passegger, V.Pavlov, A.Pedraz, S.Perdelwitz, V.Perger, M.Ramón-Ballesta, A.Reffert, S.Revilla, D.Rodríguez, E.Rodríguez-López, C.Sadegi, S.Á. Sánchez Carrasco, M.Sánchez-López, A.Sanz-Forcada, J.Schäfer, S.Schlecker, M.H. M. M. Schmitt, J.Schöfer, P.Schweitzer, A.Seifert, W.Shan, Y.L. Skrzypinski, S.Solano, E.Stahl, O.Stangret, M.Stock, S.Stürmer, J.M. Tabernero, H.Tal-Or, L.Trifonov, T.Vanaverbeke, S.Yan, F.Zapatero Osorio, M. R.2026-01-16T10:32:06ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837exoplanetshabitable-planetshigh-resolution-spectroscopyradial-velocity The CARMENES instrument, installed at the 3.5 m telescope of the Calar Alto Observatory in Almería, Spain, was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of nearby cool stars. The service publishes the CARMENES guaranteed time observations (GTO), spanning from 2016 to 2020, during which 19 633 spectra for a sample of 362 targets were collected. DR1 makes public all observations obtained during the GTO of the CARMENES survey.2023A&A...670A.139Rhttp://dc.g-vo.org/carmenes/q/ssa/infoArchiveResearchIsServedByGAVO Data Center ObscoreGAVO Data Center TAP servicehttp://dc.g-vo.org/carmenes/q/ssa/ssap.xml?https://dc.g-vo.org/carmenes/q/ssa/ssap.xml?GETapplication/x-votable+xmlPOSICRS position of target objectdegcharSIZESize of the region of interest around POSdegrealBANDWavelength (range) of interest (or symbolic bandpass names)mcharTIMEMidpoint of exposure (MJD)time.epochcharFORMATMIME type of the file servedmeta.code.mimecharAPERTUREAngular diameter of aperturedegphys.angSize;instr.fovcharSNRSignal-to-noise ratio estimated for this datasetstat.snrcharREDSHIFTRedshift of target objectsrc.redshiftcharTARGETNAMECommon name of object observed.meta.id;srccharTARGETCLASSObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classcharMTIMEDate last published.charFLUXCALIBType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).charSPATRESSpatial resolution of datadegpos.angResolutioncharWAVECALIBType of wavelength calibrationmeta.code.qualcharCOLLECTIONA short handle naming the collection this spectrum belongs to.charSPECRPLower limit to spectral resolution power (λ/Δλ) as a single number.realPUBDIDDataset identifier assigned by the publishermeta.ref.ivoidcharCREATORDIDDataset identifier assigned by the creatormeta.idcharWILDTARGETShell pattern of target observed (case insensitive)charWILDTARGETCASEShell pattern of target observed (case sensitive)charREQUESTThis is queryData for the default operation; some services support getData as wellcharTOPOnly return the TOP "best" records (on this service, this usually is equivalent to MAXREC, so no ranking is implied).integerCOMPRESSReturn compressed results?charRUNIDAn identifier for a certain run. Opaque to the servicecharresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integerfullpointedarchivalICRS9010000001000090MAXREC=1http://dc.g-vo.org/carmenes/q/web/formhttps://dc.g-vo.org/carmenes/q/web/formhttp://dc.g-vo.org/carmenes/q/ssa/capabilitieshttps://dc.g-vo.org/carmenes/q/ssa/capabilitieshttp://dc.g-vo.org/carmenes/q/ssa/availabilityhttps://dc.g-vo.org/carmenes/q/ssa/availabilityhttp://dc.g-vo.org/carmenes/q/ssa/tableMetadatahttps://dc.g-vo.org/carmenes/q/ssa/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/taphttp://dc.g-vo.org/carmenes/q/sdl/dlgethttps://dc.g-vo.org/carmenes/q/sdl/dlgethttp://dc.g-vo.org/carmenes/q/sdl/dlmetahttps://dc.g-vo.org/carmenes/q/sdl/dlmetaGETapplication/x-votable+xml;content=datalinkIDThe publisher DID of the dataset of interestmeta.id;meta.maincharresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integerCalar AltoCARMENESInfraredOpticalivoaDefinition and support code for the ObsCore data model and table.ivoa.obscoreThis data collection is queryable in GAVO Data Center's obscore table.carmenes The CARMENES instrument, installed at the 3.5 m telescope of the Calar Alto Observatory in Almería, Spain, was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of nearby cool stars. The service publishes the CARMENES guaranteed time observations (GTO), spanning from 2016 to 2020, during which 19 633 spectra for a sample of 362 targets were collected. DR1 makes public all observations obtained during the GTO of the CARMENES survey.carmenes.dataThe spectra from which the CARMENES radial velocity curves were made. Note that we only publish spectra that were actually used in time series. Also, note that positions and object names from the headers of the spectra are unreliable.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpass520 .. 1063 nmcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.VersionDR 6charnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wlcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.densitycharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionCARMENES DR1charnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcesurveycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationNORMALIZEDcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablen_ordersNumber of orders in the spectrum.meta.numberintnullableorder_minMinimal Echelle order in the spectrum.instr.order;stat.minintnullableorder_maxMaximal Echelle order in the spectrum.instr.order;stat.maxintnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullabledatalinkA link to a datalink document for this spectrum.meta.ref.urlcharnullablerv_driftEstimated RV drift against the evening referencem/sobs.paramfloatnullablename_hdrTarget name as given in the FITS header (ssa_targname is an attempt to clean these up, but that may occasionally be wrong).meta.idcharnullable