rave_scsivo://org.gavo.dc/rave/q/coneThe 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-galaxy 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.2017AJ....153...75Khttps://dc.g-vo.org/rave/q/cone/infoIsServedByGAVO Data Center TAP service All publications making use of the RAVE data should refer to the paper given in source.http://dc.g-vo.org/rave/q/cone/formhttps://dc.g-vo.org/rave/q/cone/formhttp://dc.g-vo.org/rave/q/cone/scs.xml?https://dc.g-vo.org/rave/q/cone/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealrvHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentricrealJmag2MASS J magnitudemagphot.mag;em.IR.Jrealsnr_kSignal to noise value for the stellar parameter pipeline.stat.snrrealresponseformatFile 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.integer180100000true324.94-35.760.5http://dc.g-vo.org/rave/q/cone/capabilitieshttps://dc.g-vo.org/rave/q/cone/capabilitieshttp://dc.g-vo.org/rave/q/cone/availabilityhttps://dc.g-vo.org/rave/q/cone/availabilityhttp://dc.g-vo.org/rave/q/cone/tableMetadatahttps://dc.g-vo.org/rave/q/cone/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tapUK 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 56386https://dc.g-vo.org/rave/q/cone/coverageOpticalrave 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.output 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._rDistance to cone centerdegpos.angDistancedoublenullablerave_obs_idUnique Identifier for RAVE objects: Observation Date, Fieldname, Fibernumbermeta.id;meta.maincharnullableraveidMain RAVE identifiermeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.main0.0020416711.6986187.976347.739359.9951doublenullabledej2000Declination (J2000.0)degpos.eq.dec;meta.main-87.5159-77.45-36.6149-3.1733327.74051doublenullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-2938.4-70.2027.2697.01132667.081floatnullablee_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.fieldcharnullableteff_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.snr010499520310.952949floatnullablealgo_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-2.98911.82815.54816.84322.8431floatnullablee_jmag2MASS J total magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0150.0230.0690.1679.9990.953595floatnullablehmag2MASS H magnitudemagphot.mag;em.IR.H-4.00711.06314.90816.27824.2920.999999floatnullablekmag2MASS K_s magnitudemagphot.mag;em.IR.K-4.37810.73314.66516.20520.5320.999998floatnullablechisq_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.absorption00.1250.3460.4580.9180.904763floatnullablechisq_kχ² of the Stellar Parameter Pipelinestat.fit.chi24.18.816.175.21.88259e+070.952949floatnullablealpha_cAlpha-enhancement from chemical pipeline (log solar ratio; 'dex')phys.abund-9.99-9.990.090.451.170.763008floatnullableav_schlegelTotal Extinction in V-band from 1998ApJ...500..525Smagphys.absorption0.0060.0380.2191.41303349.1740.844171floatnullableid_tgasTGAS target designationmeta.id.cross168706316942082.4299709766774426e+185.433330854338756e+186.818433543826135e+1869174937058300416000.47942585longnullable