期刊
ASTRONOMY & ASTROPHYSICS
卷 669, 期 -, 页码 -出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/202244784
关键词
astrometry; catalogs; methods: data analysis; methods: statistical
This study aims to empirically quantify the completeness of Gaia's third data release (DR3) catalogue and develops a simple completeness model that takes into account specific factors of the optical survey. By testing the model's predictions against observational data, it is found that the model can accurately predict Gaia's completeness across the entire sky.
Interpreting and modelling astronomical catalogues requires an understanding of the catalogues' completeness or selection function: what properties determine an object's probability of being including in the catalogue? Here we set out to empirically quantify the completeness of the overall catalogue of Gaia's third data release (DR3). This task is not straightforward because Gaia is the all-sky optical survey with the highest angular resolution to date and no consistent ground truth exists to allow direct comparisons. However, well-characterised deeper imaging enables an empirical assessment of Gaia's G-band completeness across parts of the sky. On this basis, we devised a simple analytical completeness model of Gaia as a function of the observed G magnitude and position over the sky, which accounts for both the effects of crowding and the complex Gaia scanning law. Our model only depends on a single quantity: the median magnitude M-10 in a patch of the sky of catalogued sources with astrometric_matched_transits <= 10. We note that M-10 reflects elementary completeness decisions in the Gaia pipeline and is computable from the Gaia DR3 catalogue itself and therefore applicable across the whole sky. We calibrated our model using the Dark Energy Camera Plane Survey (DECaPS) and tested its predictions against Hubble Space Telescope observations of globular clusters. We found that our model predicts Gaia's completeness values to a few per cent (RMS) across the sky. We make the model available as a part of the gaiaunlimited Python package built and maintained by the GaiaUnlimited project(star).
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据