J/A+A/511/A90        RAVE DR2 distance catalogue               (Breddels+, 2010)

Distance determination for RAVE stars using stellar models. Breddels M.A., Smith M.C., Helmi A., Bienayme O., Binney J., Bland-Hawthorn J., Boeche C., Burnett B.C.M., Campbell R., Freeman K.C., Gibson B., Gilmore G., Grebel E.K., Munari U., Navarro J.F., Parker Q.A., Seabroke G.M., Siebert A., Siviero A., Steinmetz M., Watson F.G., Williams M., Wyse R.F.G., Zwitter T. <Astron. Astrophys., 511, A90-90 (2010)> =2010A&A...511A..90B 2010A&A...511A..90B
ADC_Keywords: Surveys ; Radial velocities; Milky Way ; Stars, distances Keywords: methods: numerical - methods: statistical - stars: distances - Galaxy: kinematics and dynamics - Galaxy: structure Abstract: We develop a method for deriving distances from spectroscopic data and obtaining full 6D phase-space coordinates for the RAVE survey's second data release. Description: We used stellar models combined with atmospheric properties from RAVE (effective temperature, surface gravity and metallicity) and (J-Ks) photometry from archival sources to derive absolute magnitudes. In combination with apparent magnitudes, sky coordinates, proper motions from a variety of sources and radial velocities from RAVE, we are able to derive the full 6D phase-space coordinates for a large sample of RAVE stars. This method is tested with artificial data, Hipparcos trigonometric parallaxes and observations of the open cluster M 67. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file ravedr2.dat 703 16146 Distance catalogue for the RAVE second data release -------------------------------------------------------------------------------- See also: III/257 : RAVE second data release (Zwitter+, 2008) Byte-by-byte Description of file: ravedr2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name RAVE internal identifier 17- 25 F9.5 deg RAdeg Right ascension in decimal degrees (J2000) 27- 35 F9.5 deg DEdeg Declination in decimal degrees (J2000) 37- 52 F16.11 deg GLON [-180/180] Galactic longitude 54- 67 F14.10 deg GLAT Galactic latitude 69- 87 F19.14 km/s RV Weighted mean of available radial velocities 88-103 F16.12 km/s e_RV Weighted error of available radial velocities 105-110 F6.1 mas/yr pmRA Proper motion along RA 112-117 F6.1 mas/yr pmDE Proper motion along DE 119-123 F5.1 mas/yr e_pmRA rms uncertainty on pmRA 125-129 F5.1 mas/yr e_pmDE rms uncertainty on pmDE 131-137 F7.1 K Teff Effective temperature (arithmetic mean) 139 I1 --- o_Teff [1/2] Number of observations having Teff 141-145 F5.3 [cm/s2] logg Surface gravity (arithmetic mean) 147 I1 --- o_logg [1/2] Number of observations having log(g) 149-154 F6.3 [Sun] [M/H] Uncalibrated metallicity abundance (mean) 156 I1 --- o_[M/H] [1/2] Number of observations having [M/H] 158-163 F6.3 [Sun] [M/H]c Calibrated metallicity abundance (mean) 165 I1 --- o_[M/H]c [1/2] Number of observations having [M/H] 167-171 F5.3 [Sun] [a/f] α-elements enhancement [α/Fe] 173 I1 --- o_[a/f] [1/2] Number of observations having [α/Fe] 175-180 F6.3 mag Jmag 2MASS J magnitude 182-186 F5.3 mag e_Jmag rms uncertainty on Jmag 188-193 F6.3 mag Kmag 2MASS K magnitude 195-199 F5.3 mag e_Kmag rms uncertainty on Kmag 201-218 F18.15 mag JMAG Absolute J-band magnitude (from fitting method) 220-233 F14.12 mag e_JMAG rms uncertainty on JMAG 235-253 F19.16 mag JMAGm Median absolute J magnitude 255-270 F16.13 kpc Dist Heliocentric distance 272-287 F16.14 kpc e_Dist rms uncertainty on Dist 289-305 F17.13 kpc x Galactocentric x coordinate (1) 306-322 E17.15 kpc e_x rms uncertainty on x 324-342 E19.15 kpc y Galactocentric y coordinate (1) 344-360 E17.15 kpc e_y rms uncertainty on y 362-378 F17.13 kpc z Galactocentric z coordinate (1) 380-395 F16.14 kpc e_z rms uncertainty on z 397-416 F20.14 km/s U Galactic velocity relative to Sun along x (1) 418-434 F17.12 km/s e_U rms uncertainty on U 436-455 F20.14 km/s V Galactic velocity relative to Sun along y (1) 457-473 F17.12 km/s e_V rms uncertainty on V 475-495 F21.15 km/s W Galactic velocity relative to Sun along z (1) 497-512 F16.12 km/s e_W rms uncertainty on W 514-534 F21.15 km/s Vx Galactocentric velocity along x (1) 536-552 F17.12 km/s e_Vx rms uncertainty on xGalVel 554-572 F19.13 km/s Vy Galactocentric velocity along y (1) 574-590 F17.12 km/s e_Vy rms uncertainty on yGalVel 592-611 F20.14 km/s Vz Galactocentric velocity along z (1) 613-629 F17.12 km/s e_Vz rms uncertainty on zGalVel 630-649 F20.14 km/s Vrho Galactocentric radial velocity Vρ (1) 651-667 F17.12 km/s e_Vrho rms uncertainty on Vrho 669-685 F17.12 km/s Vphi Galactocentric orthoradial velocity Vφ (1) 687-703 F17.12 km/s e_Vphi rms uncertainty on Vphi -------------------------------------------------------------------------------- Note (1): The coordinate system we use is a right-handed Cartesian coordinate system centred on the Galactic Centre (GC): the x axis is aligned with the GC-Sun axis with the Sun located at x=-8kpc; the y axis pointing in the direction of rotation and the z axis pointing towards the Northern Galactic Pole (NGP). The velocities with respect to the Sun in the directions of (x, y, z) are (U, V, W) respectively, with the rest frame taken at the Sun (such that the Sun is at (U, V, W)=(0, 0, 0)). The catalogue also includes cylindrical polar coordinates (V{rho}, Vφ , Vz), defined in a Galactic rest frame such that the local standard of rest (LSR) moves at vφ=-220km/s. To transform from the rest frame of the Sun to the Galactic rest frame, we use vLSR=220km/s for the LSR and take the velocity of the Sun (10.0, 5.25, 7.17)km/s with respect to the LSR (Dehnen & Binney, 1998MNRAS.298..387D 1998MNRAS.298..387D). -------------------------------------------------------------------------------- History: Copied at http://www.astro.rug.nl/~rave/
(End) Patricia Vannier [CDS] 11-Jun-2010
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line