carmenes.raw_dativo://org.gavo.dc/carmenes/q/raw_dataThe 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

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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/tableinfo/carmenes.raw_dataArchiveResearchCalar AltoCARMENESInfraredOpticalcarmenes 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.raw_data 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.ssa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoubleindexednullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_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_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablen_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.maxintnullableaccrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Sizelongnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_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