Pipeline Reduction of Binary Light Curves from Large-Scale Surveys
Andrej Prsa, Tomaz Zwitter

TL;DR
This paper reviews recent advancements in automated pipelines for processing large-scale binary star light curve data, addressing challenges of data quality and coverage in modern astronomical surveys.
Contribution
It provides a comprehensive overview of semi-automatic and fully automatic methods developed for analyzing binary star light curves from large surveys.
Findings
Automatic pipelines have been successfully applied to Hipparcos, OGLE, and ASAS data.
Automated methods improve efficiency in processing massive survey datasets.
Challenges remain in data quality and coverage affecting analysis accuracy.
Abstract
One of the most important changes in observational astronomy of the 21st Century is a rapid shift from classical object-by-object observations to extensive automatic surveys. As CCD detectors are getting better and their prices are getting lower, more and more small and medium-size observatories are refocusing their attention to detection of stellar variability through systematic sky-scanning missions. This trend is aditionally powered by the success of pioneering surveys such as ASAS, DENIS, OGLE, TASS, their space counterpart Hipparcos and others. Such surveys produce massive amounts of data and it is not at all clear how these data are to be reduced and analysed. This is especially striking in the eclipsing binary (EB) field, where most frequently used tools are optimized for object-by-object analysis. A clear need for thorough, reliable and fully automated approaches to modeling and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Astronomical Observations and Instrumentation
