rave.dr4ivo://org.gavo.dc/rave/q/dr4The 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, data release 4. 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, those with name ending in _sparv come from the radial velocity pipeline. Names ending in _n_k indicate calibrated values.2017AJ....153...75Khttp://dc.g-vo.org/tableinfo/rave.dr4UK 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.dr4The RAVE object catalog, data release 4. 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, those with name ending in _sparv come from the radial velocity pipeline. Names ending in _n_k indicate calibrated values.482194nameTarget designationmeta.id;meta.maincharindexedprimaryaltnameRAVE target designationmeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.main0.0020416710.8708185.699348.023359.9951doubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.main-87.5159-77.5138-36.1694-3.0444127.74051doubleindexednullableglonGalactic longitudedegpos.galactic.lon0.000277.05174277.426353.107359.9991doublenullableglatGalactic latitudedegpos.galactic.lat-89.8798-74.4171-21.109346.624873.63471doublenullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-1000.54-68.17287.49195.12481001.311floatindexednullablee_rvError in heliocentric radial velocitykm/sstat.error;spect.dopplerVeloc;pos.heliocentric0.2730.5741.187.273448.7441floatnullableobsdateObservation date.dtime.epoch;obs52740528955461756101562811doublenullablefield_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.setup18.076.0146.01501.0shortteff_kEffective temperature from the stellar parameter pipeline.Kphys.temperature.effective3000380048587049.2780000.932867floatnullablee_teff_kError in the effective temperature from the stellar parameter pipeline.Kstat.error;phys.temperature.effective62629527711660.932867floatnullablelogg_kLog gravity as determined by the stellar pipeline.phys.gravity00.493.184.85.50.932867floatnullablee_logg_kError in logg_k.stat.error;phys.gravity0.090.120.20.521.260.932867floatnullablemet_kMetallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-5-1.57-0.470.3510.932867floatnullablemet_n_kCalibrated metallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-7.709-1.18775-0.197750.2055390.349750.932867floatnullablee_met_kError in metallicity [m/H] from the stellar parameter pipeline.stat.error;phys.abund.Z0.060.080.10.261.140.932867floatnullablesnr_kSignal to noise value for the stellar parameter pipeline.stat.snr011509620310.932867floatindexednullablealgo_conv_kQuality flag for stellar parameter pipeline [0..4].meta.code.qual000440.932867floatnullablealAbundance of Al [Al/H]phys.abund-1.84-0.67-0.070.471.10.585961floatnullableal_nNumber of spectral lines used for the computation of Al abundance.phys.abund02.02.02.020.6493859intnullablesiAbundance of Si [Si/H]phys.abund-2.34-0.73-0.040.511.10.631192floatnullablesi_nNumber of spectral lines used for the computation of Si abundance.phys.abund04.013.016.0330.6493859intnullablefeAbundance of Fe [Fe/H]phys.abund.Fe-2.71-0.94-0.230.321.040.616267floatnullablefe_nNumber of spectral lines used for the computation of Fe abundance.phys.abund116.036.054.0890.6493859intnullabletiNumber of spectral lines used for the computation of Ti abundance.phys.abund-2.67-0.71-0.10.521.10.516039floatnullableti_nNumber of used spectral lines for calculation of Ti abundance.phys.abund01.010.025.0390.6493859intnullableniAbundance of Ni [Ni/H]phys.abund-1.67-0.85-0.160.591.10.236625floatnullableni_nNumber of spectral lines used for the computation of Ni abundance.phys.abund00.00.04.060.6493859intnullablemgAbundance of Mg [Mg/H]phys.abund-2.04-0.76-0.160.381.10.621534floatnullablemg_nNumber of spectral lines used for the computation of Mg abundance.phys.abund01.03.05.070.6493859intnullablejmag2MASS 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-4.00711.06314.90816.27824.2920.999999floatnullablee_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.chi2382.6542.1723.91718.21e+060.649386floatnullableid_2mass2MASS Target designationmeta.idcharnullableid_denisDENIS Target designationmeta.idcharnullableid_usnob1USNOB1 Target designationmeta.idcharnullableid_tycho2TYCHO2 target designationmeta.idcharnullableid_ucac4UCAC4 target designationmeta.idcharnullableid_ppmxlPPMXL target designation.meta.id11529489412846565331.3073282239178688e+184.819919694503959e+186.775420030134535e+1869175240734767787700.99372864longnullableparallaxParallax (from 2014MNRAS.437..351B)maspos.parallax0.069520.2489971.546899.73911540.30.80451floatnullablee_parallaxError Parallax (from 2014MNRAS.437..351B)masstat.error;pos.parallax0.002028760.05666440.5582122.97427688.0430.80451floatnullabledist_binneyDistance (from 2014MNRAS.437..351B)kpcpos.distance0.0007883120.1154620.7820914.2611714.4870.80451floatnullablee_distError in Distance (from 2014MNRAS.437..351B)kpcstat.error;pos.distance0.0003843470.03653540.2753821.054085.415810.80451floatnullabledistance_modulusDistance modulus (from 2014MNRAS.437..351B)phot.mag.distMod-5.740335.165069.2763413.086615.79770.80451floatnullablee_distance_modulusDistance modulus (from 2014MNRAS.437..351B)stat.error;phot.mag.distMod0.02265240.3581630.6153731.405245.641650.80451floatnullablelog_avExtinction (from 2014MNRAS.437..351B)phys.absorption-3.32378-1.5398-0.7748930.02653070.807970.80451floatnullablee_log_avError in extinction (from 2014MNRAS.437..351B)stat.error;phys.absorption1.06153e-050.1276110.3426950.4401491.009130.80451floatnullablemin_dists20 minimum distances to the base spectrum given by alphabetic codes from 2012ApJS..200...14M.charnullablecorrelation_coeffTonry & Davis R correlation coefficientstat.fit.param0.048.8251.55103.46201.871floatnullablepeak_heightHeight of the correlation peak.stat.correlation0.0010.4810.9510.9830.991floatnullablepeak_widthWidth of the correlation peak.stat.correlation8.52251.315863.753103.3011434.41floatnullableskyhrvMeasured heliocentry radial velocity of the sky.km/sspect.dopplerVeloc;obs.field;pos.heliocentric-297.286-9.744-0.20711.451254.7950.995029floatnullablee_skyhrvError in the measured heliocentric velocity of the sky.km/sstat.error;spect.dopplerVeloc;obs.field;pos.heliocentric00.9715.2517.259995.5430.995037floatnullabletdccskyTonry & Davis R Sky correlation coefficient.stat.fit.param00.23.7425.299.660.995027floatnullablecorrection_rvZero point correction applied to the radial velocity solutions (see 2011AJ....141..187S).km/sarith.zp-36.953-3.533-0.5192.30543.7511floatnullablezeropoint_flagQuality flag for Zero point correctionmeta.codecharnullableteff_sparvEffective temperature as determined by the radial velocity pipeline.Kphys.temperature.effective2580358749347154508240.945928floatnullablelogg_sparvLog gravity as determined by the radial velocity pipeline.phys.gravity00.73.184.865.50.945928floatnullablealpha_sparvMetallicity as determined by the radial velocity pipeline.phys.abund.Z000.070.310.450.945928floatnullableageLogarithm of age (from 2014MNRAS.437..351B)log(a)time.age7.178949.035659.7410810.003810.080.80451floatnullablee_ageError in Age (from 2014MNRAS.437..351B)log(a)stat.error;time.age0.003448430.06653730.2718180.4821661.138460.80451floatnullablemassMass (from 2014MNRAS.437..351B)solMassphys.mass0.163050.7686651.179511.9294714.40940.80451floatnullablee_massError Mass (from 2014MNRAS.437..351B)solMassstat.error;phys.mass0.001984930.05007570.2106540.8409945.440660.80451floatnullable