Emission line star catalogues post-Gaia DR3

A validation of Gaia DR3 data using the LAMOST OBA emission catalogue

¹ Department of Physics and Electronics, CHRIST (Deemed to be University), Hosur Main Road, Bangalore, India
e-mail: shridharan.b@res.christuniversity.in
² Indian Institute of Astrophysics, Koramangala, Bangalore, India
³ Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai, India

Received: 26 June 2022
Accepted: 22 September 2022

Abstract

Aims.Gaia Data Release 3 (DR3) and further releases have the potential to identify and categorise new emission-line stars in the Galaxy. We perform a comprehensive validation of astrophysical parameters from Gaia DR3 with the spectroscopically estimated emission-line star parameters from the LAMOST OBA emission catalogue.

Method. We compare different astrophysical parameters provided by Gaia DR3 with those estimated using LAMOST spectra. By using a larger sample of emission-line stars, we performed a global polynomial and piece-wise linear fit to update the empirical relation to convert the Gaia DR3 pseudo-equivalent width to the observed equivalent width, after removing the weak emitters from the analysis.

Results. We find that the emission-line source classifications given by DR3 is in reasonable agreement with the classification from the LAMOST OBA emission catalogue. The astrophysical parameters estimated by the esphs module from Gaia DR3 provides a better estimate when compared to gspphot and gspspec. A second degree polynomial relation is provided along with piece-wise linear fit parameters for the equivalent width conversion. We notice that the LAMOST stars with weak Hα emission are not identified to be in emission from BP/RP spectra. This suggests that emission-line sources identified by Gaia DR3 are incomplete. In addition, Gaia DR3 provides valuable information about the binary and variable nature of a sample of emission-line stars.