SkyMapper stellar parameters for Galactic Archaeology on a grand-scale
Abstract
The SkyMapper photometric surveys provides uvgriz photometry for several millions sources in the Southern sky. We use DR1.1 to explore the quality of its photometry, and develop a formalism to homogenize zero-points across the sky using stellar effective temperatures. Physical flux transformations, and zero-points appropriate for this release are derived, along with relations linking colour indices to stellar parameters. Reddening-free pseudo-colours and pseudo-magnitudes are also introduced. For late-type stars which are best suited for Galactic Archaeology, we show that SkyMapper + 2MASS are able to deliver a precision better than 100 K in effective temperatures (depending on the filters), ∼0.2 dex for metallicities above -2, and a reliable distinction between M-dwarfs and -giants. Together with astrometric and asteroseismic space mission, SkyMapper promises to be a treasure trove for stellar and Galactic studies.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- January 2019
- DOI:
- 10.1093/mnras/sty2878
- arXiv:
- arXiv:1810.09581
- Bibcode:
- 2019MNRAS.482.2770C
- Keywords:
-
- stars: fundamental parameters;
- stars: late-type;
- Galaxy: stellar content;
- Astrophysics - Solar and Stellar Astrophysics;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- MNRAS, accepted. Metallicities and effective temperatures for 9 million Gaia+SkyMapper stars at https://github.com/casaluca/SkyMapper