Improved distances and ages for stars common to TGAS and RAVE

Paul J. McMillan, Georges Kordopatis, Andrea Kunder, James Binney, Jennifer Wojno, Tomaž Zwitter, Matthias Steinmetz, Joss Bland-Hawthorn, Brad K. Gibson, Gerard Gilmore, Eva K. Grebel, Amina Helmi, Ulisse Munari, Julio F. Navarro, Quentin A. Parker, George Seabroke, Fred Watson, Rosemary F.G. Wyse

Forskningsoutput: TidskriftsbidragArtikel i vetenskaplig tidskriftPeer review

24 Citeringar (SciVal)

Sammanfattning

We combine parallaxes from the first Gaia data release with the spectrophotometric distance estimation framework for stars in the fifth RAVE survey data release. The combined distance estimates aremore accurate than either determination in isolation - uncertainties are on average two times smaller than for RAVE-only distances (three times smaller for dwarfs), and 1.4 times smaller than TGAS parallax uncertainties (two times smaller for giants). We are also able to compare the estimates from spectrophotometry to those from Gaia, and use this to assess the reliability of both catalogues and improve our distance estimates. We find that the distances to the lowest log g stars are, on average, overestimated and caution that they may not be reliable. We also find that it is likely that the Gaia random uncertainties are smaller than the reported values. As a by-product we derive ages for the RAVE stars, many with relative uncertainties less than 20 per cent. These results for 219 566 RAVE sources have been made publicly available, and we encourage their use for studies that combine the radial velocities provided by RAVE with the proper motions provided by Gaia. A sample that we believe to be reliable can be found by taking only the stars with the flag notification 'flag_any=0'.

Originalspråkengelska
Sidor (från-till)5279-5300
Antal sidor22
TidskriftMonthly Notices of the Royal Astronomical Society
Volym477
Utgåva4
DOI
StatusPublished - 2018 juli 11

Ämnesklassifikation (UKÄ)

  • Astronomi, astrofysik och kosmologi

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