TL;DR
This paper assesses the completeness of Gaia DR2 by modeling detection probabilities based on observations and magnitude, providing a sky- and magnitude-dependent completeness map crucial for galactic studies.
Contribution
It introduces a novel method to predict Gaia DR2's completeness across the sky, accounting for crowding effects and providing accessible selection functions.
Findings
Gaia DR2 is 99% complete up to G=18.9 to 21.3 depending on the sky region.
Completeness varies significantly in dense regions like the Galactic bulge and Magellanic Clouds.
A new Python package for Gaia DR2 selection functions is provided.
Abstract
The second data release of the Gaia mission contained astrometry and photometry for an incredible 1,692,919,135 sources, but how many sources did Gaia miss and where do they lie on the sky? The answer to this question will be crucial for any astronomer attempting to map the Milky Way with Gaia DR2. We infer the completeness of Gaia DR2 by exploiting the fact that it only contains sources with at least five astrometric detections. The odds that a source achieves those five detections depends on both the number of observations and the probability that an observation of that source results in a detection. We predict the number of times that each source was observed by Gaia and assume that the probability of detection is either a function of magnitude or a distribution as a function of magnitude. We fit both these models to the 1.7 billion stars of Gaia DR2, and thus are able to robustly…
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