• Corpus ID: 119239815

Eclipsing Binary Stars in the OGLE-III Fields of the Small Magellanic Cloud

@article{Pawlak2013EclipsingBS,
  title={Eclipsing Binary Stars in the OGLE-III Fields of the Small Magellanic Cloud},
  author={Michał Pawlak and Dariusz Graczyk and Igor Soszyński and Paweł Pietrukowicz and Radosław Poleski and Andrzej Udalski and Michał K. Szymański and Marcin Kubiak and Grzegorz Pietrzyński and Lukasz Wyrzykowski and Krzysztof Ulaczyk and Szymon Kozłowski and Jan Skowron},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2013}
}
We present a large sample of eclipsing binary stars detected in the Small Magellanic Cloud fields covering about 14 square degrees that have been monitored for eight years during the third phase of the OGLE survey. This is the largest set of such variables containing 6138 objects, of which 777 are contact and 5361 non-contact binaries. The estimated completeness of this sample is around 82%. We analyze the statistical properties of the sample and present selected interesting objects: 32 systems… 
A Distance Determination to the Small Magellanic Cloud with an Accuracy of Better than Two Percent Based on Late-type Eclipsing Binary Stars
We present a new study of late-type eclipsing binary stars in the Small Magellanic Cloud (SMC) undertaken with the aim of improving the distance determination to this important galaxy. A sample of 10
APSIDAL MOTIONS OF 27 BINARY SYSTEMS IN THE SMALL MAGELLANIC CLOUD
We present the periods of apsidal motion for 27 early-type eclipsing binaries with high eccentricity located in the Small Magellanic Cloud. New times of minima were derived from the light curves
Eclipsing Binary Populations across the Northern Galactic Plane from the KISOGP Survey
We present a catalog of eclipsing binaries in the northern Galactic plane from the Kiso Wide-Field Camera Intensive Survey of the Galactic Plane (KISOGP). We visually identified 7055 eclipsing
Apsidal Motion and Absolute Parameters of 21 Early-type Small Magellanic Cloud Eccentric Eclipsing Binaries
We present the apsidal motion and light-curve analyses of 21 eccentric eclipsing binaries located in the Small Magellanic Cloud. Most of these systems have never been studied before, hence their
A Comprehensive Catalog of Galactic Eclipsing Binary Stars with Eccentric Orbits Based on Eclipse Timing Diagrams
A comprehensive catalog of 623 galactic eclipsing binary (EB) systems with eccentric orbits is presented with more than 2830 times of minima determined from the archived photometric data by various
Eclipsing Binaries in the MOA-II Database
TLDR
The results suggest that contact binaries with periods close to the 0.22-day contact binary limit are commonly accompanied by relatively close tertiary companions.
Apsidal motion and a light curve solution for eighteen SMC eccentric eclipsing binaries
Aims. The Danish 1.54-meter telescope at the La Silla observatory was used for photometric monitoring of selected eccentric eclipsing binaries located in the Small Magellanic Cloud. The new times of
KMTNet Time-series Photometry of the Doubly Eclipsing Binary Stars Located in the Large Magellanic Cloud
We report the results of photometric observations for doubly eclipsing binaries OGLE-LMC-ECL-15674 and OGLE-LMC-ECL-22159, both of which are composed of two pairs (designated A&B) of a detached
Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems
Close, compact, hierarchical, multiple stellar systems, i.e., multiples having an outer orbital period from months to a few years, comprise a small, but continuously growing group of the triple and
The quadruple-lined, doubly-eclipsing system V482 Persei
We report spectroscopic and differential photometric observations of the A-type system V482 Per that reveal it to be a rare hierarchical quadruple system containing two eclipsing binaries. One has
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References

SHOWING 1-2 OF 2 REFERENCES
C4.5: Programs for Machine Learning
TLDR
A complete guide to the C4.5 system as implemented in C for the UNIX environment, which starts from simple core learning methods and shows how they can be elaborated and extended to deal with typical problems such as missing data and over hitting.
General Catalog of Variable Stars ” ( Version 2011 Jan )
  • 2011