J/MNRAS/465/3203      GALAH observational overview              (Martell+, 2017)

The GALAH Survey: Observational overview and Gaia DR1 companion. Martell S.L., Sharma S., Buder S., Duong L., Schlesinger K.J., Simpson J., Lind K., Ness M., Marshall J.P., Asplund M., Bland-Hawthorn J., Casey A.R., De Silva G., Freeman K.C., Kos J., Lin J., Zucker D.B., Zwitter T., Anguiano B., Bacigalupo C., Carollo D., Casagrande L., Da Costa G.S., Horner J., Huber D., Hyde E.A., Kafle P.R., Lewis G.F., Nataf D., Navin C.A., Stello D., Tinney C.G., Watson F.G., Wittenmyer R. <Mon. Not. R. Astron. Soc. 465, 3203 (2017)> =2017MNRAS.465.3203M 2017MNRAS.465.3203M (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Milky Way ; Stars, nearby ; Stars, bright ; Abundances, [Fe/H] ; Effective temperatures ; Radial velocities ; Reddening ; Stars, distances Keywords: stars: abundances - Galaxy: disc - Galaxy: evolution - Galaxy: formation - Galaxy: stellar content Abstract: The Galactic Archaeology with HERMES (GALAH) Survey is a massive observational project to trace the Milky Way's history of star formation, chemical enrichment, stellar migration and minor mergers. Using high-resolution (R∼28,000) spectra taken with the High Efficiency and Resolution Multi-Element Spectrograph (HERMES) instrument at the Anglo-Australian Telescope (AAT), GALAH will determine stellar parameters and abundances of up to 29 elements for up to one million stars. Selecting targets from a colour-unbiased catalogue built from 2MASS, APASS and UCAC4 data, we expect to observe dwarfs at 0.3 to 3kpc and giants at 1 to 10kpc. This enables a thorough local chemical inventory of the Galactic thin and thick disks, and also captures smaller samples of the bulge and halo. In this paper we present the plan, process and progress as of early 2016 for GALAH survey observations. In our first two years of survey observing we have accumulated the largest high-quality spectroscopic data set at this resolution, over 200,000 stars. We also present the first public GALAH data catalogue: stellar parameters (Teff, log(g), [Fe/H], [alpha/Fe]), radial velocity, distance modulus and reddening for 10680 observations of 9860 Tycho-2 stars that may be included in the first Gaia data release. Description: Identifiers, positions, derived stellar parameters, radial velocities, distance moduli and reddenings for stars from the Tycho-2 catalogue observed by the GALAH Survey. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 131 10680 Identifiers and quantities derived from GALAH Survey data for stars from Tycho-2 -------------------------------------------------------------------------------- See also: I/337 : Gaia DR1 (Gaia Collaboration, 2016) I/259 : The Tycho-2 Catalogue (Hog+ 2000) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 9 I7 --- GALAH GALAH Survey ID number 13- 24 A12 --- TYC2 Tycho-2 ID number (NNNN-NNNNN-N) 28- 44 A17 --- 2MASS 2MASS ID number (JHHMMSSss+DDMMSSs) 48- 58 F11.7 deg RAdeg Right ascension (J2000.0) 62- 72 F11.7 deg DEdeg Declination (J2000.0) 76- 79 I4 K Teff Effective temperature 83- 86 F4.2 cm/s2 logg Surface gravity 90- 94 F5.2 Sun [Fe/H] Metallicity 98-102 F5.2 Sun [alpha/Fe] alpha enhancement 106-113 F8.3 km/s RV Radial velocity 117-122 F6.3 mag (m-M)V ?=99.999 V-band distance modulus 126-131 F6.3 mag E(B-V) ?=99.999 Reddening -------------------------------------------------------------------------------- Acknowledgements: Sarah Martell, s.martell(at)unsw.edu.au
(End) Sarah Martell [UNSW, Australia], Patricia Vannier [CDS] 08-Sep-2016
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