Improved source classification and performance analysis using Gaia DR3
Astronomy & Astrophysics(2024)
摘要
The Discrete Source Classifier (DSC) provides probabilistic classification of
sources in Gaia Data Release 3 using a Bayesian framework and a global prior.
The DSC Combmod classifier in GDR3 achieved for the extragalactic classes
(quasars and galaxies) a high completeness of 92
to contamination from the far larger star class. However, these single metrics
mask significant variation in performance with magnitude and sky position.
Furthermore, a better combination of the individual classifiers is possible.
Here we compute two-dimensional representations of the completeness and the
purity as function of Galactic latitude and source brightness, and exclude also
the Magellanic Clouds where stellar contamination significantly depresses the
purity. Reevaluated on a cleaner validation set and without introducing changes
to the published GDR3 DSC probabilities themselves, we achieve for Combmod
average 2-d completenesses of 92
89
proportions of extragalactic objects to stars in Gaia is expected to vary
significantly with brightness and latitude, we introduce a new prior as a
continuous function of brightness and latitude, and compute new class
probabilities. This variable prior only improves the performance by a few
percentage points, mostly at the faint end. Significant improvement, however,
is obtained by a new additive combination of Specmod and Allosmod. This
classifier, Combmod-α, achieves average 2-d completenesses of 82
93
respectively when using the global prior. Thus we achieve a significant
improvement in purity for a small loss of completeness. The improvement is most
significant for faint quasars where the purity rises from 20
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