arihip coneivo://x-unregistred/arihip/q/coneInstitute for Solar Physics, Stockholm UniversityWielen, R.Schwan, H.Dettbarn, C.Lenhardt, H.Jahreiß, H.Jährling, RKhalisi, E.2026-06-05T10:30:34ZMats Lofdahl

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invalid@example.comDelete this line if you don't want to give itstarscatalogsastrometryproper-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....1Whttp://stw-main.utenforuio.no:8080/arihip/q/cone/infoCatalogARIHIP is licensed under the `Creative Commons Attribution 3.0 License <http://creativecommons.org/licenses/by/3.0/>`_ .. image:: /static/img/ccby.png :alt: [CC-BY] 0/0-1147770 492142.721e-19 4.138e-19http://stw-main.utenforuio.no:8080/arihip/q/cone/coverageOpticalarihip 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).output 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)._rDistance to cone centerdegpos.distancedoublenullablehipnoNumber of the star in the HIPPARCOS Catalogue (ESA 1997).meta.id;meta.mainintraj2000Right ascension from a single-star solutiondegpos.eq.ra;meta.maindoubledej2000Declination from a single-star solutiondegpos.eq.dec;meta.maindoublepmraProper motion in right ascension times cos(delta) for a single-star solution.deg/yrpos.pm;pos.eq.rafloatnullablepmdeProper motion in declination for a single-star solution.deg/yrpos.pm;pos.eq.decfloatnullableerr_raError in RA from the single star solution, with cos(delta) already applieddegstat.error;pos.eq.rafloatnullableerr_pmraMean error in PM(RA)*cos(delta) from the single star solutiondeg/yrstat.error;pos.pm;pos.eq.rafloatnullableerr_deError in Dec from the single star solutiondegstat.error;pos.eq.decfloatnullableerr_pmdeMean error in PM(Dec) form the single star solutiondeg/yrstat.error;pos.pm;pos.eq.decfloatnullableparallaxParallax 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.parallaxfloatnullablevradRadial velocity as used in calculating the foreshortening effect.km/sspect.dopplerVeloc;pos.heliocentricfloatnullablemvVisual magnitude taken from the HIPPARCOS cataloguemagphot.mag;em.opt.VfloatnullablekmVariability flag. See note.meta.code;src.varcharnullablekbinBinarity flag. See note.meta.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.radoublenullabledeltpDeclination in LTP modedegpos.eq.decdoublenullablepmraltpProper motion in RA, cos(delta) applied, in LTP modedeg/yrpos.pm;pos.eq.rafloatnullablepmdeltpProper motion in Dec in LTP modedeg/yrpos.pm;pos.eq.decfloatnullablerastpRight ascension in STP modedegpos.eq.radoublenullabledestpDeclination in STP modedegpos.eq.decdoublenullablepmrastpProper motion in RA, cos(delta) applied, in STP modedeg/yrpos.pm;pos.eq.rafloatnullablepmdestpProper motion in Dec in STP modedeg/yrpos.pm;pos.eq.decfloatnullablerahipRight ascension in HIP modedegpos.eq.radoublenullabledehipDeclination in HIP modedegpos.eq.decdoublenullablepmrahipProper motion in RA, cos(delta) applied, in HIP modedeg/yrpos.pm;pos.eq.rafloatnullablepmdehipProper motion in Dec in HIP modedeg/yrpos.pm;pos.eq.decfloatnullable