Precision Light Curves from TESS Full-Frame Images: A Difference Imaging Approach

Abstract

The Transiting Exoplanet Survey Satellite (TESS) will observe $\sim$150~million stars brighter than $T_{\mathrm{mag}}\approx 16$, with photometric precision from 60~ppm to 3~percent, enabling an array of exoplanet and stellar astrophysics investigations.While light curves will be provided for $\sim$400,000 targets observed at 2-min cadence, observations of most stars will only be provided as full-frame images (FFIs) at 30~min cadence. The TESS image scale of $\sim 21$''/pix is highly susceptible to crowding, blending, and source confusion, and the highly spatially variable point spread function (PSF) will challenge traditional techniques, such as aperture and Gaussian-kernel PSF photometry. We use official "End-to-End~6" TESS simulated FFIs to demonstrate a difference image analysis pipeline, using a $\delta$-function kernel,that achieves the mission specification noise floor of 60~ppm~hr${}^{-1/2}$. We show that the pipeline performance does not depend on position across the field, and only $\sim$2\% of stars appear to exhibit residual systematics at the level of $\sim$5~ppt. We also demonstrate recoverability of planet transits, eclipsing binaries, and other variables. We provide the pipeline as an open-source tool at https://github.com/ryanoelkers/DIA in both IDL and PYTHON. We intend to extract light curves for all point sources in the \textit{TESS} FFIs as soon as they become publicly available, and will provide the light curves through the Filtergraph data visualization service. An example data portal based on the simulated FFIs is available for inspection at https://filtergraph.com/tess_ffi.

11 pages, 4 figures, submitted to AAS journals, comments and suggestions are welcome! Release version 0 of the pipeline can be found at the URL: https://github.com/ryanoelkers/DIA. All data products from this letter, and future data products produced by the pipeline, can be found at the URL: https://filtergraph.com/tess_ffi

References in corpus (6)

• A Technique for Extracting Highly Precise Photometry for the Two-Wheeled Kepler Mission
• A New Algorithm For Difference Image Analysis
• Variability Properties of 4 Million Sources in the $TESS$ Input Catalog Observed with the Kilodegree Extremely Little Telescope Survey
• Difference Image Analysis of Defocused Observations with CSTAR
• GW150914: First search for the electromagnetic counterpart of a gravitational-wave event by the TOROS collaboration
• Identification of Young Stellar Variables with KELT for K2 II: The Upper Scorpius Association

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