The University of New South Wales Extrasolar Planet Search: a catalogue of variable stars from fields observed 2004--2007

TL;DR

This paper presents a comprehensive catalogue of 850 variable stars identified from data collected during the UNSW Extrasolar Planet Search, providing valuable data for astrophysical research and stellar evolution studies.

Contribution

The study introduces a new catalogue of variable stars from planet search data, including many previously uncatalogued variables, with detailed classifications and potential applications in astrophysics.

Findings

Identified 850 variable stars, 659 of which are new discoveries.

Catalog includes various types of variable stars such as eclipsing binaries, RR Lyrae, Cepheids, and pulsating stars.

Discussed applications in binary star evolution, stellar calibration, and pulsation mysteries.

Abstract

We present a new catalogue of variable stars compiled from data taken for the University of New South Wales Extrasolar Planet Search. From 2004 October to 2007 May, 25 target fields were each observed for 1-4 months, resulting in ~87000 high precision light curves with 1600-4400 data points. We have extracted a total of 850 variable light curves, 659 of which do not have a counterpart in either the General Catalog of Variable Stars, the New Suspected Variables catalogue or the All Sky Automated Survey southern variable star catalogue. The catalogue is detailed here, and includes 142 Algol-type eclipsing binaries, 23 beta Lyrae-type eclipsing binaries, 218 contact eclipsing binaries, 53 RR Lyrae stars, 26 Cepheid stars, 13 rotationally variable active stars, 153 uncategorised pulsating stars with periods <10 d, including delta Scuti stars, and 222 long period variableswith variability on timescales of >10 d. As a general application of variable stars discovered by extrasolar planet transit search projects, we discuss several astrophysical problems which could benefit from carefully selected samples of bright variables. These include: (i) the quest for contact binaries with the smallest mass ratio, which could be used to test theories of binary mergers; (ii) detached eclipsing binaries with pre-main-sequence components, which are important test objects for calibrating stellar evolutionary models; and (iii) RR Lyrae-type pulsating stars exhibiting the Blazhko-effect, which is one of the last great mysteries of pulsating star research.