Identifying objects with starspot crossing characteristics from Kepler K2 data

by


Misty Chien

Hobart and William Smith Colleges
Geneva, New York
April 2023

ABSTRACT

Sunspots are observable manifestations of the Sun's magnetic field. The Sun is close to us compared to other stars in the Universe. This means that with a telescope, we can see the dark sunspot features in much more detail than a star that is both fainter and much farther away. What if we want to learn about the magnetic field of other stars? A lot less is known about these stars, and the tools with which to learn about them are more limited. A technique that is used by astronomers to circumvent this problem is using transiting planets as a probe. The Kepler spacecraft monitors the brightness of stars and detects orbiting planets through an apparent dip in the brightness when a planet crosses in front of the star. Planets sometimes cross in front of starspots on the star; this has a unique effect on the dip in brightness. The planet is now blocking less light, so there are bumps in the dip of the brightness. Therefore, analyzing in-transit variation of brightness of stars can help identify objects with starspot crossing events. The goal of this project is to identify objects with starspot crossing features from a list of K2 candidates. The planet samples are obtained from Campaigns 1-8 and 10-18 of the K2 mission (Zink et al., 2021). Given an object, the program extracts its long cadence lightcurve data from the Kepler/K2 catalogs of the Mikulski Archive for Space Telescopes (MAST), normalizes individual transits, and computes a model based on its stellar parameters using BAsic Transit Model cAlculatioN in Python (batman). The program then calculates the difference between the data and the model and performs the Kolmogorov-Smirnov (K-S) test on the residuals to determine whether they are statistically from different distributions. Out of 196 objects, 10 objects are identified by visual inspection of their lightcurves to have starspot crossing features. These objects have K-S statistics ranging from 0.15 to 0.39. By compiling a short list of objects with starspot crossing features, this allows for further study on these stars.

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