Untangling Variables in Gaia DR3 Open Access
Schapera, Eden (Spring 2024)
Abstract
Although the GAIA database is an incredibly useful tool to assess baseline variability, the low and uneven cadence across different Gaia sectors makes it very difficult to distinguish between objects with similar lightcurve features. Using previously verified W. Ursa Majoris and RRc Lyra stars, we develop a classification pipeline using minima depth variation in the lightcurve to distinguish between genuine RR Lyrae and eclipsing binaries. We assess a set of 72 variables with poor or incomplete lightcurves in Gaia using TESS archival data, and identify 12 objects as genuine RR Lyrae based on their minima variation and secondary lightcurve features. We further verify the lightcurves of three variables using observational data from the Emory observatory, reinforcing the efficacy of our classification pipeline.
Table of Contents
Chapter 1: Background ------------1
I: RRc Lyrae ------------2
II: W. Ursa Majoris Eclipsing Binaries ------------3
III: Astronomical Databases and Previous Research ------------5
Gaia
TESS
Combining Gaia and TESS for Time Domain Photometry
Chapter 2: Initial Classification and TESS Analysis ------------8
I: Identification of Candidates ------------8
II: The Lightkurve Pipeline ------------8
Data Reduction and Cleaning
Minima Classification
Chapter 3: Observational Studies ------------24
I: Identification of Candidates ------------24
II: Data Collection ------------25
III: Calibration ------------26
IV: Processing ------------28
VI: Visualization and Analysis ------------29
LAMOST J073756.25+311646.5
ASAS J074316+1705
LAMOST/ATO J106.1517+08.6631
Chapter 4: Discussion and Future Research ------------38
References ------------41
Tables ------------43
Figures ------------50
Appendix 1: Smoothing Lightcurve Data ------------52
Appendix 2: The Lightkurve RRc Pipeline ------------56
Appendix 3: PLD Correction ------------58
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