RAdial Velocity Experiment: RAVE DR5 2009-09-30T14:53:00Z 100 Kordopatis,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. Data Release 5 surveys stars radial-velocity milky-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. http://www.rave-survey.org Optical `_ and many other tables using our \RSTservicelink{/tap}{TAP service}. ]]> 2017AJ....153...75K UK Schmidt AAO 6dF All publications making use of the RAVE data should refer to the paper given in source. Flag of Stellar Parameter Pipeline. === ================================================================== 0 Pipeline converged 1 no convergence. 2 MATISSE oscillates between two values and the mean is given. 3 results of MATISSE at the boundaries or outside the grid and the DEGAS value has been adopted 4 the metal-poor giants with SNR<20 have been re-run by DEGAS with a scale factor (ie, internal parameter of DEGAS) of 0.40 === ================================================================== //scs#pgs-pos-indexThe 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. Position ICRS SPHER3 "raj2000" "dej2000" "dist_binney" 52741 56386 0/8,11 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 4/0-1,27,256,265,267-268,270,282,285,292-293,295,514,552,576,776,809,814,1116-1118,1136,1180-1181,1188-1190,1192-1194,1196,1207-1209,1216,1308,1310,1332,1334-1335,1338,1344-1345,1347-1349,1351,1357,1365,1368,1370,1374,1377,1379,1382,1386,1428-1430,1432-1434,1436,1452,1454,1456,1460,1463,1506,1512,1620-1622,1636-1638,1648,1653-1654,1659,1692,1708,1710,1728,1796-1798,1825,1829,1838-1841,1844,1850-1851,1854,1864-1865,1868-1870,1880-1881,1887-1888,1890,1893,1908,1944-1946,1964-1965,1968,1976,1992,2332-2334,2356,2358,2364,2376-2377,2379,2401-2403,2455,2463,2485-2487,2492-2494,2536-2537,2539,2584-2586,2588-2589,2591,2610,2618-2619,2621-2623,2632,2635,2656-2657,2660,2664,2666-2667 //scs#pgs-pos-indexThe 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. Position ICRS SPHER3 "raj2000" "dej2000" "dist_binney" Flag value of the form FGSH, F being for the entire plate, G for the 50 fibers group to which the fiber belongs. S flags the zero-point correction used: C for cubic and S for a constant shift. If H is set to * the fiber is close to a 15 fiber gap. For F and G the values can be * A, B, C, D, or E, meaning: === ============================================== A dispersion around correction lower than 1 km/s B dispersion between 1 and 2 km/s C dispersion between 2 and 3 km/s D dispersion larger than 3 km/s E less than 15 fibers available for the fit === ============================================== //scs#pgs-pos-index`_ in the data center). Columns in the data release that resulted from crossmatching were left out. For details, see 2011AJ....141..187S. ]]> Position ICRS SPHER3 "raj2000" "dej2000" -1 VelocityInterval Velocity "pmra" "pmde" "rv" Error "e_pmra" "e_pmde" "e_rv" Position GALACTIC "glon" "glat" Source of proper motion === ============== 0 no PM 1 Tycho-2 2 Supercosmos 3 PPMX 4 GSC1.2x2MASS 5 UCAC-2 6 USNO-B" === ============== Flag value of the form FGSH, F being for the entire plate, G for the 50 fibers group to which the fiber belongs. S flags the zero-point correction used: C for cubic and S for a constant shift. If H is set to * the fiber is close to a 15 fiber gap. For F and G the values can be * A, B, C, D, or E, meaning: === ============================================= A dispersion around correction lower than 1km/s B dispersion between 1 and 2km/s C dispersion between 2 and 3km/s D dispersion larger than 3km/s E less than 15 fibers available for the fit === ============================================= qual identifies possible problems in the spectrum (values can be combined) as follows: === ======================================== a asymmetric Ca lines c cosmic ray pollution e emission line spectrum n noise dominated spectrum 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 spectrum shows problem b blue part of the spectrum shows problem p possible binary/doubled lined x peculiar object === ======================================== The maskflag column identifies the fraction of the spectrum unaffected by continuum problems from the MASK program. Spectra with maskflags lower than 0.70 must be used with caution. //scs#pgs-pos-index`_ 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. ]]>Data Release 2 Position ICRS SPHER3 "raj2000" "dej2000" -1 Position GALACTIC "glon" "glat" 1- 16 18- 33 35- 46 48- 59 61- 69 71- 79 81- 87 89- 94 96-101 103-108 110-115 117-122 124 126-130 132-139 141-150 152 154-156 158-162 164-167 169-173 175-178 180-184 186-193 195-199 201-205 207-210 212-217 219-224 226-231 233-238 240-244 246-250 465 466 467 469-472 name:Name, altname:RAVEID, raj2000:RAdeg, dej2000:DEdeg, glon:Glon, glat:Glat, rv:HRV, e_rv:eHRV, pmsrc:Spm, imag:Imag, field:FieldName, plate:PlateNumber, fiber:FiberNumber, teff:Teff, logg:logg, met:Met, alpha:alpha, chi2:CHISQ, snr2:S2N, snr:STN, tdcc:CorrelationCoeff, hcp:PeakHeight, wcp:PeakWidth, zeropoint:CorrectionRV, hrvsky:SkyRV, e_hrvsky:SkyeRV, tdccsky:SkyCorrelation, snrspec:SNRatio, zp1:ZeroPointFLAG, qual:SpectraFLAG, maskflag:MaskFLAG data/dr4/RAVE_DR4.csv.gz name, altname, raj2000, dej2000, glon, glat, rv, e_rv, correlation_coeff, peak_height, peak_width, correction_rv, skyhrv, e_skyhrv, tdccsky, zeropoint_flag, stn_sparv, id_tycho2, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, id_ucac4, ignore, ignore, ignore, ignore, ignore, ignore, id_ppmxl, ignore, ignore, ignore, ignore, ignore, ignore, obsdate, field_name, plate_number, fiber_number, teff_k, e_teff_k, logg_k, e_logg_k, met_k, met_n_k, e_met_k, snr_k, algo_conv_k, al, al_n, si, si_n, fe, fe_n, ti, ti_n, ni, ni_n, mg, mg_n, chisq_c, teff_sparv, logg_sparv, alpha_sparv, id_2mass, ignore, ignore, Jmag, e_Jmag, Hmag, e_Hmag, Kmag, e_Kmag, id_denis, ignore, ignore, ignore, ignore, ignore, ignore, ignore, ignore, id_usnob1, ignore, ignore, ignore, ignore, ignore, ignore, ignore, parallax, e_parallax, dist_binney, e_dist, distance_modulus, e_distance_modulus, log_av, e_log_av, age, e_age, mass, e_mass, c1,c2,c3,c4,c5,c6,c7,c8,c9,c10,c11,c12,c13,c14,c15,c16,c17,c18,c19,c20 parseWithNull(@\item, int, r"\\\N") parseWithNull(@\item, float, r"\\\N") parseWithNull(@\item.strip(), str, r"\\\N") rave_obs_id, healpix, raveid, raj2000, dej2000, glon,glat,rv,e_rv, stddev_rv,mad_rv,stn_sparv,snr_k, teff_k,teff_n_k,e_teff_k,mad_teff_k,stddev_teff_k, logg_k,logg_n_k,e_logg_k,mad_logg_k,stddev_logg_k, met_k,met_n_k,e_met_k,mad_met_k,stddev_met_k,chisq_k, algo_conv_k, teff_ir,e_teff_ir,ir_direct, mg,mg_n,al,al_n,si,si_n,ti,ti_n,fe,fe_n,ni,ni_n, alpha_c,chisq_c,frac_c,av_schlegel, dist_binney,e_dist,log_av,e_log_av, parallax,e_parallax, distance_modulus,e_distance_modulus, fit_flag_binney,fitquality_binney, n_gauss_fit,gauss_mean_1,gauss_sigma_1,gauss_frac_1, gauss_mean_2,gauss_sigma_2,gauss_frac_2, gauss_mean_3,gauss_sigma_3,gauss_frac_3, c1,c2,c3,c4,c5,c6,c7,c8,c9,c10,c11,c12,c13,c14,c15,c16,c17,c18,c19,c20, rep_flag,cluster_flag,footprint_flag,id_tgas,matchflag_tgas, ra_tgas,de_tgas,pmra_tgas,pmra_error_tgas,pmde_tgas,pmde_error_tgas, parallax_tgas,parallax_error_tgas, phot_g_mean_mag_tgas,phot_g_mean_flux_tgas, phot_g_mean_flux_error_tgas, id_hipparcos,id_tycho2,dist_tycho2,matchflag_tycho2, btmag_tycho2,ebtmag_tycho2,vtmag_tycho2,evtmag_tycho2, pmra_tycho2,epmra_tycho2,pmde_tycho2,epmde_tycho2, id_ucac4,dist_ucac4,matchflag_ucac4, pmra_ucac4,epmra_ucac4,pmde_ucac4,epmde_ucac4, id_ppmxl,dist_ppmxl,matchflag_ppmxl, pmra_ppmxl,epmra_ppmxl,pmde_ppmxl,epmde_ppmxl, id_2mass,dist_2mass,matchflag_2mass, Jmag,e_Jmag,Hmag,e_Hmag, Kmag,e_Kmag, id_allwise,dist_allwise,matchflag_allwise,w1mag_allwise, ew1mag_allwise,w2mag_allwise,ew2mag_allwise, w3mag_allwise,ew3mag_allwise,w4mag_allwise,ew4mag_allwise, cc_flags_allwise,ext_flg_allwise, var_flg_allwise,ph_qual_allwise, dist_apassdr9,matchflag_apassdr9,bmag_apassdr9,ebmag_apassdr9, vmag_apassdr9,evmag_apassdr9,gpmag_apassdr9,egpmag_apassdr9, rpmag_apassdr9,erpmag_apassdr9,ipmag_apassdr9,eipmag_apassdr9, id_denis,dist_denis,matchflag_denis,imag_denis,eimag_denis, jmag_denis,ejmag_denis,kmag_denis,ekmag_denis, id_usnob1,dist_usnob1,matchflag_usnob1,b1mag_usnob1, r1mag_usnob1,b2mag_usnob1,r2mag_usnob1,imag_usnob1, pmra_usnob1,epmra_usnob1,pmde_usnob1,epmde_usnob1, obsdate,field_name,fiber_number,plate_number,mjd_obs, lst_start,lst_end,utc_start,utc_end parseWithNull(@\item, float, r"NULL") parseWithNull(@\item, float, r"-9") parseWithNull(@\item, int, r"NULL") parseWithNull(@\item, str, r"NULL") rave_scs RAVE DR5 Cone Search 324.94 -35.76 0.5 cone/scs.xml row = self.getFirstVOTableRow(rejectExtras=False) self.assertEqual(row["id_denis"], 'J003641.3-404441') self.assertAlmostEqual(row["rv"], 16.364999771118164) self.assertEqual(row["obsdate"], 52887.0) self.assertEqual(row["id_ppmxl"], 1454951088173346604) self.assertEqual(row["min_dists"], 'nnnnnnnnnnnnnnnnnnnn') self.assertEqual(row["ti"], None)