skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: THE BERLIN EXOPLANET SEARCH TELESCOPE II CATALOG OF VARIABLE STARS. I. CHARACTERIZATION OF THREE SOUTHERN TARGET FIELDS

Abstract

A photometric survey of three southern target fields with BEST II yielded the detection of 2406 previously unknown variable stars and an additional 617 stars with suspected variability. This study presents a catalog including their coordinates, magnitudes, light curves, ephemerides, amplitudes, and type of variability. In addition, the variability of 17 known objects is confirmed, thus validating the results. The catalog contains a number of known and new variables that are of interest for further astrophysical investigations, in order to, e.g., search for additional bodies in eclipsing binary systems, or to test stellar interior models. Altogether, 209,070 stars were monitored with BEST II during a total of 128 nights in 2009/2010. The overall variability fraction of 1.2%-1.5% in these target fields is well comparable to similar ground-based photometric surveys. Within the main magnitude range of R in [11, 17], we identify 0.67(3)% of all stars to be eclipsing binaries, which indicates a completeness of about one third for this particular type in comparison to space surveys.

Authors:
; ; ; ; ; ; ; ; ; ;  [1]; ;  [2]
  1. Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt, Rutherfordstr. 2, D-12489 Berlin (Germany)
  2. Astronomisches Institut, Ruhr-Universität Bochum, D-44780 Bochum (Germany)
Publication Date:
OSTI Identifier:
22273284
Resource Type:
Journal Article
Journal Name:
Astronomical Journal (New York, N.Y. Online)
Additional Journal Information:
Journal Volume: 146; Journal Issue: 5; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 1538-3881
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ASTRONOMY; ASTROPHYSICS; BINARY STARS; CATALOGS; COMPARATIVE EVALUATIONS; ECLIPSE; PHOTOMETRY; STAR MODELS; TELESCOPES; VARIABLE STARS; VISIBLE RADIATION

Citation Formats

Fruth, T., Cabrera, J., Csizmadia, Sz., Dreyer, C., Eigmüller, P., Erikson, A., Kabath, P., Kirste, S., Pasternacki, T., Rauer, H., Titz-Weider, R., Chini, R., Lemke, R., and Murphy, M., E-mail: thomas.fruth@dlr.de. THE BERLIN EXOPLANET SEARCH TELESCOPE II CATALOG OF VARIABLE STARS. I. CHARACTERIZATION OF THREE SOUTHERN TARGET FIELDS. United States: N. p., 2013. Web. doi:10.1088/0004-6256/146/5/136.
Fruth, T., Cabrera, J., Csizmadia, Sz., Dreyer, C., Eigmüller, P., Erikson, A., Kabath, P., Kirste, S., Pasternacki, T., Rauer, H., Titz-Weider, R., Chini, R., Lemke, R., & Murphy, M., E-mail: thomas.fruth@dlr.de. THE BERLIN EXOPLANET SEARCH TELESCOPE II CATALOG OF VARIABLE STARS. I. CHARACTERIZATION OF THREE SOUTHERN TARGET FIELDS. United States. https://doi.org/10.1088/0004-6256/146/5/136
Fruth, T., Cabrera, J., Csizmadia, Sz., Dreyer, C., Eigmüller, P., Erikson, A., Kabath, P., Kirste, S., Pasternacki, T., Rauer, H., Titz-Weider, R., Chini, R., Lemke, R., and Murphy, M., E-mail: thomas.fruth@dlr.de. 2013. "THE BERLIN EXOPLANET SEARCH TELESCOPE II CATALOG OF VARIABLE STARS. I. CHARACTERIZATION OF THREE SOUTHERN TARGET FIELDS". United States. https://doi.org/10.1088/0004-6256/146/5/136.
@article{osti_22273284,
title = {THE BERLIN EXOPLANET SEARCH TELESCOPE II CATALOG OF VARIABLE STARS. I. CHARACTERIZATION OF THREE SOUTHERN TARGET FIELDS},
author = {Fruth, T. and Cabrera, J. and Csizmadia, Sz. and Dreyer, C. and Eigmüller, P. and Erikson, A. and Kabath, P. and Kirste, S. and Pasternacki, T. and Rauer, H. and Titz-Weider, R. and Chini, R. and Lemke, R. and Murphy, M., E-mail: thomas.fruth@dlr.de},
abstractNote = {A photometric survey of three southern target fields with BEST II yielded the detection of 2406 previously unknown variable stars and an additional 617 stars with suspected variability. This study presents a catalog including their coordinates, magnitudes, light curves, ephemerides, amplitudes, and type of variability. In addition, the variability of 17 known objects is confirmed, thus validating the results. The catalog contains a number of known and new variables that are of interest for further astrophysical investigations, in order to, e.g., search for additional bodies in eclipsing binary systems, or to test stellar interior models. Altogether, 209,070 stars were monitored with BEST II during a total of 128 nights in 2009/2010. The overall variability fraction of 1.2%-1.5% in these target fields is well comparable to similar ground-based photometric surveys. Within the main magnitude range of R in [11, 17], we identify 0.67(3)% of all stars to be eclipsing binaries, which indicates a completeness of about one third for this particular type in comparison to space surveys.},
doi = {10.1088/0004-6256/146/5/136},
url = {https://www.osti.gov/biblio/22273284}, journal = {Astronomical Journal (New York, N.Y. Online)},
issn = {1538-3881},
number = 5,
volume = 146,
place = {United States},
year = {Fri Nov 01 00:00:00 EDT 2013},
month = {Fri Nov 01 00:00:00 EDT 2013}
}