2018RAA....18..118B


Query : 2018RAA....18..118B

2018RAA....18..118B - Research in Astron. and astroph., 18, 118-118 (2018/October-0)

Machine learning classification of Gaia Data Release 2.

BAI Y., LIU J.-F. and WANG S.

Abstract (from CDS):

Machine learning has increasingly gained more popularity with its incredibly powerful ability to make predictions or calculate suggestions for large amounts of data. We apply machine learning classification to 85 613 922 objects in the Gaia Data Release 2, based on a combination of Pan-STARRS 1 and AllWISE data. The classification results are cross-matched with the Simbad database, and the total accuracy is 91.9%. Our sample is dominated by stars, ∼98%, and galaxies make up 2%. For the objects with negative parallaxes, about 2.5% are galaxies and QSOs, while about 99.9% are stars if the relative parallax uncertainties are smaller than 0.2. Our result implies that using the threshold of 0 < σπ/π < 0.2 could yield a very clean stellar sample.

Abstract Copyright: ∼

Journal keyword(s): methods: data analysis - stars: general - Gaia catalog

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Psc-Per Supercluster SCG 02 33.2 +41 37           ~ 444 1
2 NAME Gal Anticenter reg 05 46 +28.9           ~ 1024 0
3 ACO 624 ClG 08 17 45 +76 51.8           ~ 4 0
4 NAME Shapley Supercluster SCG 13 06.0 -33 04           ~ 677 0

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