Data Release 2rave.dr2ivo://org.gavo.dc/rave/q/dr2The 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.2016-09-22T00:00:00ZData Release 5GAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837surveysstarsradial-velocitymilky-way-galaxy
The second data release of RAVE contains spectroscopic radial velocities
for 49327 stars in the Milky-Way southern hemisphere using the 6dF
instrument at the AAO. Stellar parameters are published for a set of 21121
stars belonging to the second year of observation.
This data collection has been superceded by RAVE data release 3
(`table rave.dr </__system__/dc_tables/show/tableinfo/rave.dr3>`_
in the data center).
The data published here comprises all original RAVE data. Columns
in the data release that resulted from crossmatching were left out.
For details, see 2008MNRAS.391..793S.http://dc.zah.uni-heidelberg.de/tableinfo/rave.dr2UK 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 56386OpticalraveRAdial Velocity Experiment: RAVE DR5 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.dr2Data Release 2
The second data release of RAVE contains spectroscopic radial velocities
for 49327 stars in the Milky-Way southern hemisphere using the 6dF
instrument at the AAO. Stellar parameters are published for a set of 21121
stars belonging to the second year of observation.
This data collection has been superceded by RAVE data release 3
(`table rave.dr </__system__/dc_tables/show/tableinfo/rave.dr3>`_
in the data center).
The data published here comprises all original RAVE data. Columns
in the data release that resulted from crossmatching were left out.
For details, see 2008MNRAS.391..793S.51829nameTarget designationmeta.id;meta.maincharnullablealtnameTarget alternative designationmeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.maindoubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.maindoubleindexednullableglonGalactic longitudedegpos.galactic.lonfloatnullableglatGalactic latitudedegpos.galactic.latfloatnullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentricfloatnullablee_rvHRV errorkm/sstat.errorfloatnullablepmraProper motion in RAmas/yrpos.pm;pos.eq.rafloatnullablee_pmraError in proper motion in RAmas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdeProper motion in Declinationmas/yrpos.pm;pos.eq.decfloatnullablee_pmdeError in proper motion in Declinationmas/yrstat.error;pos.pm;pos.eq.decfloatnullablepmsrcSource of proper motion (0 - no PM; 1 - Tycho-2; 2 - Supercosmos; 3 - STARNET 2.0; 4 - GSC1.2x2MASS; 5 - UCAC-2)meta.ref;pos.pm;pos.eq.decshortnullableimagInput catalog I magnitudemagphot.mag;em.opt.IfloatnullableobsdateDate of observationdtime.epoch;obscharnullablefieldName of RAVE fieldmeta.id;obs.fieldcharnullableplatePlate number usedmeta.id;instr.paramshortfiberFiber numbermeta.idshortteffEffective TemperatureKphys.temperature.effectiveintnullableloggGravityphys.gravityfloatnullablem_h_uncalUncalibrated [M/H]phys.abund.Fefloatnullablealfa_fealpha enhancement [{alpha}/Fe]phys.abundfloatnullablem_hCalibrated [M/H], Sun=1phys.abund.Fefloatnullablechi2chi squarestat.fit.chi2doublenullablesnrCorrected signal to noisestat.snrfloatnullabletdccTonry-Davis correlation coefficientstat.fit.paramfloatnullablehcpHeight of correlation peakstat.correlationfloatnullablewcpWidth of correlation peakkm/sstat.correlationfloatnullablezeropointZero point correction appliedkm/sarith.zpfloatnullablehrvskyMeasured heliocentric radial velocity of skykm/sspect.dopplerVeloc;obs.field;pos.heliocentricfloatnullablee_hrvskyError HRV of skykm/sstat.errorfloatnullabletdccskySky Tonry-Davis correlation coefficientstat.fit.paramfloatnullablesnrspecSpectra signal to noise ratiostat.snrfloatnullablezp1Entire plate zero point correction flag [dispersion around correction <1 (A), 1..2 (B), 2..3 (C), >3 km/s (D); E - less than 15 fibers available.]meta.codecharnullablezp250 fibers group to which the fiber belongs zero point correction flagmeta.codecharnullablegapwarningFiber is close to a 15 fibers gapmeta.codebooleanqualSpectra quality flag [a - asymmetric Ca lines; c - cosmic ray pollution; e - emission line spectra; n - noise dominated spectra; l - no lines visible; w - weak lines; g - strong ghost; t - bad template fit; s - strong residual sky emission; cc - bad continuum; r - red part of the spectra shows problem; b - blue part of the spectra shows problem; p - possible binary/doubled lined; x - peculiar object;]meta.code.qualcharnullable