The Bochum Survey of the Southern Galactic Disk: IV . Multi‐Band Photometry

ABSTRACT The Southern Galactic Disk Survey (GDS) monitored a mosaic of 268 fields along a 6°‐wide stripe in the southern galactic disk from September 2010 to September 2019. These fields were observed between 21 and 407 times sim ultaneously in () and (), supplemented by between 2 and 147 observations in each of the bands , , , and . Here we present the matched multi‐band catalogue, which integrates photometry and light curve data from all bands, containing photometry for almost 21.7 million Gaia DR3 sources, of which 113,449 are identified as variables. We give an overview of the survey's variable content with respect to its main characteristics and known variability type classifications. The comparison with the cross‐match catalogue of Gaia DR3 sources with variables from the literature compiled by Gavras et al. and the International Variable Star Index (VSX) indicates that approximately of the variable sources remain unclassified in terms of variability type. Light curves for all of these sources are contained in the GDS data catalogues, available via the German Astrophysical Virtual Observatory (GAVO), and can contribute to their classification.

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Journal
Astronomische Nachrichten
Published
2026-10-29
DOI
https://doi.org/10.1002/asna.70154
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

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article

The Bochum Survey of the Southern Galactic Disk: IV . Multi‐Band Photometry

D. J. Bomans, C. Westhues, M. Ramolla, Julia Blex et al.
2 links
Astronomische Nachrichten
Stellar, planetary, and galactic studies
article

The Bochum Survey of the Southern Galactic Disk: IV . Multi‐Band Photometry

D. J. Bomans, C. Westhues, M. Ramolla, Julia Blex, Christofer Fein, A. Franckowiak, M. Hackstein, R. Chini, K. Weis, Markus Demleitner
article en

Abstract

ABSTRACT The Southern Galactic Disk Survey (GDS) monitored a mosaic of 268 fields along a 6°‐wide stripe in the southern galactic disk from September 2010 to September 2019. These fields were observed between 21 and 407 times sim ultaneously in () and (), supplemented by between 2 and 147 observations in each of the bands , , , and . Here we present the matched multi‐band catalogue, which integrates photometry and light curve data from all bands, containing photometry for almost 21.7 million Gaia DR3 sources, of which 113,449 are identified as variables. We give an overview of the survey's variable content with respect to its main characteristics and known variability type classifications. The comparison with the cross‐match catalogue of Gaia DR3 sources with variables from the literature compiled by Gavras et al. and the International Variable Star Index (VSX) indicates that approximately of the variable sources remain unclassified in terms of variability type. Light curves for all of these sources are contained in the GDS data catalogues, available via the German Astrophysical Virtual Observatory (GAVO), and can contribute to their classification.

Astronomische Nachrichten
Heidelberg University (DE), Hochschule Niederrhein (DE), Nicolaus Copernicus Astronomical Center (PL), Ruhr University Bochum (DE), Polish Academy of Sciences (PL)
National Science Foundation, National Aeronautics and Space Administration, California Institute of Technology, European Space Agency, Deutsche Forschungsgemeinschaft, Bundesministerium für Bildung und Forschung
Openalex Percentile: Top 15%
Stellar, planetary, and galactic studies
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