arihip.mainivo://org.gavo.dc/arihip/q/mainThe GAVO DC teamWielen, R.Schwan, H.Dettbarn, C.Lenhardt, H.Jahreiß, H.Jährling, RKhalisi, E.2024-05-28T11:23:32ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837starscatalogsastrometryproper-motions The catalogue ARIHIP has been constructed by selecting the 'best data' for a given star from combinations of HIPPARCOS data with Boss' GC and/or the Tycho-2 catalogue as well as the FK6. It provides 'best data' for 90 842 stars with a typical mean error of 0.89 mas/year (about a factor of 1.3 better than Hipparcos for this sample of stars).2001VeARI..40....1Whttps://dc.g-vo.org/tableinfo/arihip.mainCatalog0/0-1147770 492142.721e-19 4.138e-19Opticalarihip The catalogue ARIHIP has been constructed by selecting the 'best data' for a given star from combinations of HIPPARCOS data with Boss' GC and/or the Tycho-2 catalogue as well as the FK6. It provides 'best data' for 90 842 stars with a typical mean error of 0.89 mas/year (about a factor of 1.3 better than Hipparcos for this sample of stars).arihip.main The catalogue ARIHIP has been constructed by selecting the 'best data' for a given star from combinations of HIPPARCOS data with Boss' GC and/or the Tycho-2 catalogue as well as the FK6. It provides 'best data' for 90 842 stars with a typical mean error of 0.89 mas/year (about a factor of 1.3 better than Hipparcos for this sample of stars).90842hipnoNumber of the star in the HIPPARCOS Catalogue (ESA 1997).meta.id;meta.main13488.6958948.5114865.771204041.0intindexedprimarysrcselSource of the astrometric solutionmeta.codecharnullableraj2000Right ascension from a single-star solutiondegpos.eq.ra;meta.main0.00090000811.1353181.28348.946359.9791doubleindexeddej2000Declination from a single-star solutiondegpos.eq.dec;meta.main-89.7824-70.7875-2.111869.099489.56941doubleindexedpmraProper motion in right ascension times cos(delta) for a single-star solution.deg/yrpos.pm;pos.eq.ra-0.000904975-3.31434e-05-4.38889e-073.23571e-050.00187971floatnullablepmdeProper motion in declination for a single-star solution.deg/yrpos.pm;pos.eq.dec-0.0016153-4.22579e-05-1.56389e-061.49154e-050.002868891floatnullablet_raCentral epoch of RA (SI)yrstat.error;time.epoch;pos.eq.ra1989.871990.951991.241991.561992.331floatnullableerr_raError in RA from the single star solution, with cos(delta) already applieddegstat.error;pos.eq.ra7.77778e-081.22222e-072.25e-074.83333e-074.84444e-061floatnullableerr_pmraMean error in PM(RA)*cos(delta) from the single star solutiondeg/yrstat.error;pos.pm;pos.eq.ra5.55556e-081.25e-072.19444e-074.13889e-079.37222e-061floatnullablet_deCentral epoch of Dec (SI)yrstat.error;time.epoch;pos.eq.dec1990.351990.851991.271991.661992.411floatnullableerr_deError in Dec from the single star solutiondegstat.error;pos.eq.dec8.33333e-081.19444e-071.86111e-073.69444e-073.02222e-061floatnullableerr_pmdeMean error in PM(Dec) form the single star solutiondeg/yrstat.error;pos.pm;pos.eq.dec5e-081.22222e-071.97222e-073.63889e-077.35e-061floatnullableparallaxParallax used in deriving the data of the star in the catalogue selected for the ARIHIP. This is either the HIPPARCOS parallax or a photometric/spectroscopic parallax (see Kp).degpos.parallax-8.21667e-06-1.66667e-081.21944e-066.84444e-060.0001525031floatnullablee_parallaxMean error of the parallaxdegstat.error;pos.parallax1.11111e-081.61111e-072.94444e-075.97222e-075.77778e-061floatnullablekpSource of the parallax: H Hipparcos, P photometric parallaxmeta.ref;pos.parallaxcharnullablevradRadial velocity as used in calculating the foreshortening effect.km/sspect.dopplerVeloc;pos.heliocentric-409-61-2594710.17504floatnullablemvVisual magnitude taken from the HIPPARCOS cataloguemagphot.mag;em.opt.V-0.625.978.4710.7414.081floatindexednullablekmVariability flag. See note.meta.code;src.varcharnullablekbinBinarity flag. See note.meta.code.multipcharnullablekdmuBased on Delta mu, 1 is a single-star candidate, 2 is a Delta mu binary, and empty values mean uncertain casesmeta.code.multipcharnullablekaeMeasure of astrometric quality between 1 and 3, higher is better. Empty values mean the star is not 'astrometrically excellent'.meta.code.qualcharnullableraltpRight ascension in LTP modedegpos.eq.ra0.000900311.1353181.28348.946359.9791doublenullabledeltpDeclination in LTP modedegpos.eq.dec-89.7824-70.7875-2.111869.099489.56941doublenullablepmraltpProper motion in RA, cos(delta) applied, in LTP modedeg/yrpos.pm;pos.eq.ra-0.000904736-3.30739e-05-4.41667e-073.23442e-050.001879961floatnullablepmdeltpProper motion in Dec in LTP modedeg/yrpos.pm;pos.eq.dec-0.00161528-4.225e-05-1.55972e-061.48494e-050.002869331floatnullablet_raltpCentral epoch of RA (LTP)yrstat.error;time.epoch;pos.eq.ra1957.051989.491991.241991.41992.271floatnullableerr_raltpError in RA (LTP) with cos(delta) already applieddegstat.error;pos.eq.ra9.16667e-084.22222e-072.22778e-064.30278e-065.15833e-061floatnullableerr_pmraltpMean error in PM(RA)*cos(delta) in LTP modedeg/yrstat.error;pos.pm;pos.eq.ra6.66667e-081.91667e-072.83333e-074.80556e-079.37222e-061floatnullablet_deltpCentral epoch of Dec (LTP)yrstat.error;time.epoch;pos.eq.dec1954.471989.631991.251991.431992.411floatnullableerr_deltpError in Dec (LTP)degstat.error;pos.eq.dec1e-073.52778e-072.225e-064.3e-065.12222e-061floatnullableerr_pmdeltpMean error in PM(Dec) in LTP modedeg/yrstat.error;pos.pm;pos.eq.dec5.83333e-081.86111e-072.77778e-074.52778e-077.36667e-061floatnullablerastpRight ascension in STP modedegpos.eq.ra0.00089966711.1353181.28348.946359.9791doublenullabledestpDeclination in STP modedegpos.eq.dec-89.7824-70.7875-2.111869.099489.56941doublenullablepmrastpProper motion in RA, cos(delta) applied, in STP modedeg/yrpos.pm;pos.eq.ra-0.000905139-3.31299e-05-4.41667e-073.23487e-050.001879631floatnullablepmdestpProper motion in Dec in STP modedeg/yrpos.pm;pos.eq.dec-0.00161518-4.22632e-05-1.56389e-061.49139e-050.002868661floatnullablet_rastpCentral epoch of RA (STP)yrstat.error;time.epoch;pos.eq.ra1989.871990.931991.241991.581992.331floatnullableerr_rastpError in RA (STP) with cos(delta) already applieddegstat.error;pos.eq.ra7.77778e-081.22222e-072.27778e-074.83333e-074.84444e-061floatnullableerr_pmrastpMean error in PM(RA)*cos(delta) in STP modedeg/yrstat.error;pos.pm;pos.eq.ra8.33333e-081.33333e-072.47222e-074.75e-079.37222e-061floatnullablet_destpCentral epoch of Dec (STP)yrstat.error;time.epoch;pos.eq.dec1990.351990.831991.271991.681992.411floatnullableerr_destpError in Dec (STP)degstat.error;pos.eq.dec8.33333e-081.22222e-071.86111e-073.69444e-073.02222e-061floatnullableerr_pmdestpMean error in PM(Dec) in STP modedeg/yrstat.error;pos.pm;pos.eq.dec8.61111e-081.30556e-072.11111e-074e-077.35e-061floatnullablerahipRight ascension in HIP modedegpos.eq.ra0.00089920811.1353181.28348.946359.9791doublenullabledehipDeclination in HIP modedegpos.eq.dec-89.7824-70.7875-2.111869.099489.56941doublenullablepmrahipProper motion in RA, cos(delta) applied, in HIP modedeg/yrpos.pm;pos.eq.ra-0.000905211-3.31047e-05-4.38889e-073.23509e-050.001879621floatnullablepmdehipProper motion in Dec in HIP modedeg/yrpos.pm;pos.eq.dec-0.00161518-4.22333e-05-1.56667e-061.49336e-050.002868591floatnullablet_rahipCentral epoch of RA (HIP)yrstat.error;time.epoch;pos.eq.ra1989.871990.921991.231991.61992.381floatnullableerr_rahipError in RA (HIP) with cos(delta) already applieddegstat.error;pos.eq.ra7.77778e-081.22222e-072.27778e-074.86111e-074.84444e-061floatnullableerr_pmrahipMean error in PM(RA)*cos(delta) in HIP modedeg/yrstat.error;pos.pm;pos.eq.ra8.61111e-081.36111e-072.72222e-076.41028e-079.37222e-061floatnullablet_dehipCentral epoch of Dec (HIP)yrstat.error;time.epoch;pos.eq.dec1990.321990.811991.271991.71992.51floatnullableerr_dehipError in Dec (HIP)degstat.error;pos.eq.dec8.33333e-081.22222e-071.86111e-073.69444e-073.02222e-061floatnullableerr_pmdehipMean error in PM(Dec) in HIP modedeg/yrstat.error;pos.pm;pos.eq.dec8.88889e-081.36111e-072.27778e-074.91667e-077.35e-061floatnullableparallaxsiParallax obtained in solution SIdegpos.parallax-8.21667e-06-1.66667e-081.21944e-066.85e-060.0001523251floatnullableerr_parallaxsiError in parallax obtained in solution SIdegstat.error;pos.parallax1.16667e-071.63889e-072.91667e-075.86111e-075.77778e-061floatnullableparallaxstpParallax obtained in solution STPdegpos.parallax-8.21667e-06-1.66667e-081.21944e-066.84444e-060.000152451floatnullableerr_parallaxstpError in parallax obtained in solution STPdegstat.error;pos.parallax1.16667e-071.63889e-072.94444e-075.88889e-075.77778e-061floatnullableparallaxhipParallax obtained in solution HIPdegpos.parallax-8.21667e-06-1.94444e-081.21944e-066.84444e-060.0001525031floatnullableerr_parallaxhipError in parallax obtained in solution HIPdegstat.error;pos.parallax1.16667e-071.63889e-072.97222e-075.97222e-075.77778e-061floatnullableffhF-Measure for proper motions FK5 proper motions vs. Hipparcosstat.fit.goodness;pos.pm;arith.diff0.030.311.484.357528.320.0454195floatnullableff0hF-Measure for proper motions original catalogue positions vs. Hipparcosstat.fit.goodness;pos.pm;arith.diff0.040.341.534.633.050.0454195floatnullableff0gchF-Measure for proper motions GC positions vs. Hipparcosstat.fit.goodness;pos.pm;arith.diff0.010.271.373.96137.260.220922floatnullablef0fF-Measure for proper motions FK5 and Hipparcos positions vs. FK5 proper motionsstat.fit.goodness;pos.pm;arith.diff0.030.281.383.6117.290.0454195floatnullableft2hF-Measure for proper motions Tycho2 and Hipparcos proper motionsstat.fit.goodness;pos.pm;arith.diff00.231.173.1735.220.989718floatnullableflagsBinarity evidence and variability flags (see note)meta.codecharnullable