rave.mainivo://org.gavo.dc/rave/q/mainThe GAVO DC teamKordopatis,G.Gilmore, G.Steinmetz, M.Boeche, C.Seabroke, G.M.Siebert, A.Zwitter, T.Binney, J.de Laverny, P.Recio−Blanco, A.Williams, M.E.K.Piffl, T.Enke, H.Roeser, S.Bijaoui, A.Wyse, R.F.G.Freeman, K.Munari, U.Carillo, I.Anguiano, B.Burton, D.Campbell, R.Cass, C.J.P.Fiegert, K.Hartley, M.Parker, Q.A.Reid, W.Ritter, A.Russell, K.S.Stupart, M.Watson, F.G.Bienayme, ́O.Bland−Hawthorn, J.Gerhard, O.Gibson, B.K.Grebel, E.K.Helmi, A.Navarro, J.F.Conrad, C.Famaey, B.Faure, C.Just, A.Kos, J.Matijevic, G.McMillan, P.J.Minchev, I.Scholz, R.Sharma, S.Siviero, A.Wylie de Boer, E.Zerjal, M.2024-04-04T08:11:23ZData Release 5GAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837surveysstarsradial-velocitymilky-way-galaxyThe RAVE object catalog of radial velocities, surface gravities, and chemical parameters for about 500000 stars, data release 5. We have removed almost all fields originating from crossmatches (as this is intended for use within our TAP service, where users can do the crossmatches themselves). Also, some obviously buggy columns (e.g., footprint_flag) were dropped. Note that columns with names ending in _k originate from the stellar parameters pipeline, those with names ending in _c come from the chemical pipeline. Columns ending in _n_k indicate calibrated values.2017AJ....153...75Khttp://dc.g-vo.org/tableinfo/rave.mainUK Schmidt AAO6dF0/8,11 1/16,24,42-43 2/68,72,80,82,88,100,104,113,120,144,146,149,151-152,154,156-157,159-160,162,165 3/7,276-278,280-282,292-294,296,324-326,332,335,340,356,360-362,367,404,406,408,410,420-422,424-426,448,450-451,458,464-465,468-469,484-485,488-490,580-582,588,590,592-593,595,601-603,612,614,620,622,632-633,635,644-645,656-657,659,667,670-671 4/0-1,27,256,265,267-268,270,282,285,292-293,295,514,552,576,776,809,814,1116-1118,1136,1180-1181,1188-1190,1192-1194,1196,1207-1209,1216,1308,1310,1332,1334-1335,1338,1344-1345,1347-1349,1351,1357,1365,1368,1370,1374,1377,1379,1382,1386,1428-1430,1432-1434,1436,1452,1454,1456,1460,1463,1506,1512,1620-1622,1636-1638,1648,1653-1654,1659,1692,1708,1710,1728,1796-1798,1825,1829,1838-1841,1844,1850-1851,1854,1864-1865,1868-1870,1880-1881,1887-1888,1890,1893,1908,1944-1946,1964-1965,1968,1976,1992,2332-2334,2356,2358,2364,2376-2377,2379,2401-2403,2455,2463,2485-2487,2492-2494,2536-2537,2539,2584-2586,2588-2589,2591,2610,2618-2619,2621-2623,2632,2635,2656-2657,2660,2664,2666-266752741 56386Opticalrave The RAdial Velocity Experiment (RAVE) contains stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, chemical abundances and distances. Observations between 2003 and 2013 were used to build the five RAVE data releases.rave.mainThe RAVE object catalog of radial velocities, surface gravities, and chemical parameters for about 500000 stars, data release 5. We have removed almost all fields originating from crossmatches (as this is intended for use within our TAP service, where users can do the crossmatches themselves). Also, some obviously buggy columns (e.g., footprint_flag) were dropped. Note that columns with names ending in _k originate from the stellar parameters pipeline, those with names ending in _c come from the chemical pipeline. Columns ending in _n_k indicate calibrated values.520629rave_obs_idUnique Identifier for RAVE objects: Observation Date, Fieldname, Fibernumbermeta.id;meta.maincharindexedprimaryraveidMain RAVE identifiermeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.main0.0020416711.6986187.976347.739359.9951doubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.main-87.5159-77.45-36.6149-3.1733327.74051doubleindexednullableglonGalactic longitudedegpos.galactic.lon0.000276.99548278.956353.304359.9991doublenullableglatGalactic latitudedegpos.galactic.lat-89.8798-73.9055-19.208346.573773.63471doublenullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-2938.4-70.2027.2697.01132667.081floatindexednullablee_rvError in heliocentric radial velocitykm/sstat.error;spect.dopplerVeloc;pos.heliocentric00.5751.1898.1281239.511floatnullableobsdateObservation date.dtime.epoch;obs52741529195464656124563861doublenullablefield_nameName of RAVE field (RA/DE)meta.id;obs.fieldcharnullableplate_numberNumber of field plate [1..3]meta.id;obs.field11.02.03.031.0shortfiber_numberNumber of optical fiber used to obtain the spectrum [1,150].meta.number;instr.setup18.077.0127.01271.0shortteff_kEffective temperature from the stellar parameter pipeline.Kphys.temperature.effective300038004849704780000.952949floatnullablee_teff_kError in the effective temperature from the stellar parameter pipeline.Kstat.error;phys.temperature.effective4949742349810.952949floatnullablelogg_kLog gravity as determined by the stellar pipeline.phys.gravity00.493.174.825.50.952949floatnullablee_logg_kError in logg_k.stat.error;phys.gravity0.080.10.160.471.010.952949floatnullablemet_kMetallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-5-1.62-0.470.410.952949floatnullablemet_n_kCalibrated metallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-5.78-1.26-0.20.450.950.952949floatnullablee_met_kError in metallicity [m/H] from the stellar parameter pipeline.stat.error;phys.abund.Z0.070.080.10.211.030.952949floatnullablesnr_kSignal to noise value for the stellar parameter pipeline.stat.snr010499520310.952949floatindexednullablealgo_conv_kQuality flag for stellar parameter pipeline [0..4].meta.code.qual000440.952949floatnullablealAbundance of Al [Al/H]phys.abund-3.06-0.66-0.040.541.10.687691floatnullableal_nNumber of spectral lines used for the computation of Al abundance.phys.abund02.02.02.020.76315intnullablesiAbundance of Si [Si/H]phys.abund-3.09-0.680.010.551.090.729871floatnullablesi_nNumber of spectral lines used for the computation of Si abundance.phys.abund05.013.017.0270.7631538intnullablefeAbundance of Fe [Fe/H]phys.abund.Fe-3.02-0.89-0.160.391.10.722071floatnullablefe_nNumber of spectral lines used for the computation of Fe abundance.phys.abund116.041.056.0810.76315intnullabletiNumber of spectral lines used for the computation of Ti abundance.phys.abund-3.02-0.67-0.030.641.10.622731floatnullableti_nNumber of used spectral lines for calculation of Ti abundance.phys.abund02.013.034.0400.76315intnullableniAbundance of Ni [Ni/H]phys.abund-1.63-0.79-0.060.691.10.332246floatnullableni_nNumber of spectral lines used for the computation of Ni abundance.phys.abund00.02.04.060.76315intnullablemgAbundance of Mg [Mg/H]phys.abund-2.99-0.73-0.140.41.090.708921floatnullablemg_nNumber of spectral lines used for the computation of Mg abundance.phys.abund-22.04.05.060.7631538intnullablejmag2MASS J magnitudemagphot.mag;em.IR.J-2.98911.82815.54816.84322.8431floatindexednullablee_jmag2MASS J total magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0150.0230.0690.1679.9990.953595floatnullablehmag2MASS H magnitudemagphot.mag;em.IR.H-4.00711.06314.90816.27824.2920.999999floatindexednullablee_hmag2MASS H total magnitude uncertaintymagstat.error;phot.mag;em.IR.H0.010.0220.0790.2139.9990.909418floatnullablekmag2MASS K_s magnitudemagphot.mag;em.IR.K-4.37810.73314.66516.20520.5320.999998floatnullablee_kmag2MASS K_s total magnitude uncertaintymagstat.error;phot.mag;em.IR.K0.0110.0210.0860.2439.9990.770189floatnullablechisq_cχ² of the Chemical Pipelinestat.fit.chi20.1824.51156.51880.551e+060.76315floatnullableid_2mass2MASS Target designationmeta.idcharnullableid_denisDENIS Target designationmeta.idcharnullableid_usnob1USNOB1 Target designationmeta.idcharnullableid_tycho2TYCHO2 target designationmeta.idcharnullableid_ucac4UCAC4 target designationmeta.idcharnullableid_ppmxlPPMXL target designation.meta.id11529489412846565331.3112217555738726e+184.840295169519e+186.770253335717306e+1869175240734767787700.9986728longnullableparallaxParallax (from 2014MNRAS.437..351B)maspos.parallax0.0430.2371.5539.1521042.570.904763floatnullablee_parallaxError Parallax (from 2014MNRAS.437..351B)masstat.error;pos.parallax00.0540.5132.908266.0380.904763floatnullabledist_binneyDistance (from 2014MNRAS.437..351B)kpcpos.distance11257614512231060.904763floatnullablee_distError in Distance (from 2014MNRAS.437..351B)kpcstat.error;pos.distance041269116483700.904763floatnullabledistance_modulusDistance modulus (from 2014MNRAS.437..351B)phot.mag.distMod-5.0065.3239.23213.20216.8190.904763floatnullablee_distance_modulusDistance modulus (from 2014MNRAS.437..351B)stat.error;phot.mag.distMod0.0030.3530.6051.4036.7240.904763floatnullablelog_avExtinction (from 2014MNRAS.437..351B)phys.absorption-2.981-1.536-0.7990.0731.0610.904763floatnullablee_log_avError in extinction (from 2014MNRAS.437..351B)stat.error;phys.absorption00.1250.3460.4580.9180.904763floatnullablemin_dists20 minimum distances to the base spectrum given by alphabetic codes from 2012ApJS..200...14M.charnullablestddev_rvStandard deviation in HRV from 10 resampled spectrakm/sstat.stdev;spect.dopplerVeloc;pos.heliocentric00.1930.5954.771917.960.948952floatnullablemad_rvMedian absolute deviation in HRV from 10 resampled spectrakm/sstat.fit.residual;spect.dopplerVeloc;pos.heliocentric;stat.median00.1510.4623.6821451.920.940474floatnullablestddev_teff_kStandard deviation in Teff_K from 10 resampled spectraKstat.stdev;phys.temperature.effective08.6353395.7115452.971653.870.836511floatnullablemad_teff_kMedian absolute deviation in Teff_K from 10 resampled spectraKstat.fit.residual;phys.temperature.effective;stat.median00.980680.97394.3841977.10.754896floatnullablestddev_logg_kStandard deviation in Teff_K from 10 resampled spectrastat.stdev;phys.gravity00.030.240.943.170.836511floatnullablemad_logg_kMedian absolute deviation in metallicity from 10 resampled spectrastat.fit.residual;phys.abund.Z;stat.median00.010.20.854.510.754896floatnullablestddev_met_kStandard deviation in metallicity from 10 resampled spectrastat.stdev;phys.abund.Z00.020.130.483.290.836511floatnullablechisq_kχ² of the Stellar Parameter Pipelinestat.fit.chi24.18.816.175.21.88259e+070.952949floatnullableteff_irEffective temperature from infrared flux methodKphys.temperature.effective340037434936675196980.960811floatnullablee_teff_irError in the effective temperature from infrared flux methodKstat.error;phys.temperature.effective30491183536000.960811floatnullableir_directInfrared temperature method: IRFM -- Temperature derived from infrared flux method; CTRL -- Temperature computed via color-Teff relations; NO -- No temperature derivation possiblemeta.codecharnullablealpha_cAlpha-enhancement from chemical pipeline (log solar ratio; 'dex')phys.abund-9.99-9.990.090.451.170.763008floatnullablefrac_cFraction of spectrum used for calculation of abundancesstat.value00.921110.78943floatnullableav_schlegelTotal Extinction in V-band from 1998ApJ...500..525Smagphys.absorption0.0060.0380.2191.41303349.1740.844171floatnullablen_gauss_fitNumber of components required for multi-Gaussian distance modulus fit.meta.number11.02.03.030.9596238shortnullablegauss_mean_1Gaussian number 1 in the estimated PDF of the object distance, width.stat.fit.param-4.8294.8529.09813.198817.1450.959624floatnullablegauss_frac_1Gaussian number 1 in the estimated PDF of the object distance, weight.stat.fit.param0.3380.5110.859110.959624floatnullablegauss_mean_2Gaussian number 2 in the estimated PDF of the object distance, width.stat.fit.param-4.8206.0711.64216.9260.959624floatnullablegauss_frac_2Gaussian number 2 in the estimated PDF of the object distance, weight.stat.fit.param000.1350.4840.50.959624floatnullablegauss_mean_3Gaussian number 3 in the estimated PDF of the object distance, width.stat.fit.param-4.732005.12718.5880.959624floatnullablegauss_frac_3Gaussian number 3 in the estimated PDF of the object distance, weight.stat.fit.param0000.0340.330.959624floatnullablerep_flagTrue if the object was observed multiple timesmeta.code.qualbooleancluster_flagTrue if this was a targeted cluster observationmeta.code.qualbooleanid_tgasTGAS target designationmeta.id.cross168706316942082.4299709766774426e+185.433330854338756e+186.818433543826135e+1869174937058300416000.47942585longnullable