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J/A+A/522/A54       Distance determination for RAVE stars. II. (Zwitter+, 2010)

Distance determination for RAVE stars using stellar models. II. Most likely values assuming a standard stellar evolution scenario. Zwitter T., Matijevic G., Breddels M.A., Smith M.C., Helmi A., Munari U., Bienayme O., Binney J., Bland-Hawthorn J., Boeche C., Brown A.G.A., Campbell R., Freeman K. C., Fulbright J., Gibson B., Gilmore G., Grebel E. K., Navarro J.F., Parker Q.A., Seabroke G.M., Siebert A., Siviero A., Steinmetz M., Watson F.G., Williams M., Wyse R.F.G. <Astron. Astrophys. 522, A54 (2010)> =2010A&A...522A..54Z
ADC_Keywords: Surveys ; Stars, nearby ; Proper motions ; Stars, distances Keywords: stars: distances - catalogs - surveys - Galaxy: structure - Galaxy: stellar content - stars: statistics Abstract: The RAdial Velocity Experiment (RAVE) is a spectroscopic survey of the Milky Way which already collected over 400000 spectra of ∼330000 different stars. We use the subsample of spectra with spectroscopically determined values of stellar parameters to determine the distances to these stars. The list currently contains 235064 high quality spectra which show no peculiarities and belong to 210872 different stars. The numbers will grow as the RAVE survey progresses. The distances are determined with a method based on the work by Breddels et al. (2010, Cat. J/A+A/511/A90). Here we assume that the star undergoes a standard stellar evolution and that its spectrum shows no peculiarities. The refinements include: the use of either of the three isochrone sets, a better account of the stellar ages and masses, use of more realistic errors of stellar parameter values, and application to a larger dataset. The derived distances of both dwarfs and giants match within ∼21% to the astrometric distances of Hipparcos stars and to the distances of observed members of open and globular clusters. Multiple observations of a fraction of RAVE stars show that repeatability of the derived distances is even better, with half of the objects showing a distance scatter of ≤11%. RAVE dwarfs are ∼300pc from the Sun, and giants are at distances of 1 to 2kpc, and up to 10kpc. This places the RAVE dataset between the more local Geneva-Copenhagen survey and the more distant and fainter SDSS sample. As such it is ideal to address some of the fundamental questions of Galactic structure and evolution in the pre-Gaia era. Individual applications are left to separate papers, here we show that the full 6-dimensional information on position and velocity is accurate enough to discuss the vertical structure and kinematic properties of the thin and thick disks. Description: Spectrophotometric distance moduli to ∼16000 stars in the Milky Way southern hemisphere calculated from spectroscopic stellar parameters as determined by the RAVE spectroscopic survey using the 6dF instrument at the AAO. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file catalog.dat 230 16052 Catalog of distance moduli calculated with three sets of isochrones and for two sets of stellar parameters and their assumed errors for 15386 stars
See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) III/257 : RAVE second data release (DR2) (Zwitter+, 2008) J/A+A/511/A90 : RAVE DR2 distance catalogue (Breddels+, 2010) Byte-by-byte Description of file: catalog.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Target designation 18- 29 F12.8 deg RAdeg Right ascension in decimal degrees (J2000.0) 31- 42 F12.8 deg DEdeg Declination in decimal degrees (J2000.0) 44- 49 F6.1 km/s HRV Heliocentric radial velocity 51- 56 F6.1 km/s e_HRV Formal HRV error 58- 63 F6.1 mas/yr pmRA ?=9999.9 Proper motion in RA 65- 70 F6.1 mas/yr e_pmRA ?=9999.9 Error proper motion in RA 72- 77 F6.1 mas/yr pmDE ?=9999.9 Proper motion in DE 79- 84 F6.1 mas/yr e_pmDE ?=9999.9 Error proper motion in DE 86- 91 F6.3 mag Jmag 2MASS J apparent magnitude 94- 99 F6.3 mag Kmag 2MASS Ks apparent magnitude 101-108 A8 "YYYYMMDD" ObsDate Date of observation 110-119 A10 --- Field Name of RAVE field 121-123 I3 --- FibNum [1/150] Fiber number 125-130 I6 K Teff Effective temperature 133-136 F4.2 [cm/s2] logg Surface gravity 138-142 F5.2 [Sun] MH Calibrated metallicity [M/H] 144-149 F6.2 --- SN Signal to noise ratio per pixel 152-157 F6.3 mag muYY Distance modulus (using YY isochrones and DR2 values of stellar parameters with their DR2 errors) 160-165 F6.3 mag e_muYY Formal error in muYY 169-174 F6.3 mag muDar Distance modulus (using Dartmouth isochrones and DR2 values of stellar parameters with their DR2 errors) 177-182 F6.3 mag e_muDar Formal error in muDar 185-190 F6.3 mag muPad Distance modulus (using Padova isochrones and DR2 values of stellar parameters with their DR2 errors) 193-198 F6.3 mag e_muPad Formal error in muPad 201-206 F6.3 mag muPN Distance modulus (using Padova isochrones and DR3 values of stellar parameters with their DR2 errors) 209-214 F6.3 mag e_muPN Formal error in muPN 217-222 F6.3 mag muPNR Distance modulus (using Padova isochrones and DR3 values of stellar parameters with errors from repeated observations) 225-230 F6.3 mag e_muPNR Formal error in muPNR
Acknowledgements: Tomaz Zwitter, tomaz.zwitter(at)fmf.uni-lj.si References: Breddels et al., Paper I 2010A&A...511A..90B, Cat. J/A+A/511/A90
(End) Patricia Vannier [CDS] 18-Nov-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

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