Abstract
The SkyMapper photometric surveys provides u$v$griz 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.
| Original language | English |
|---|---|
| Pages (from-to) | 2770-2787 |
| Number of pages | 18 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 482 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1 Jan 2019 |
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