The T16 Project: Image Subtraction Light Curves from TESS Cycle 1 Full-frame Images for Stars with T < 16

Abstract We present 83,717,159 light curves for 56,401,549 stars with T < 16 mag observed in the Full-Frame Images (FFIs) of Cycle 1 of the NASA TESS mission. These light curves were extracted from subtracted images produced by the Cluster Difference Imaging Survey. We make public the raw image subtraction light curves, together with light curves de-trended against instrumental systematics. We compare the light curves to other publicly available light curves from the TESS FFIs, finding that for a substantial fraction of stars with T < 16, the T16 project provides the highest precision FFI light curves available. We demonstrate that the detrended T16 light curves are generally as good as, or better than, than the light curves from other projects for the known TOIs. We also show that the un-detrended light curves can be used to study high amplitude variable stars. The light curves are being made available through the NASA Mikulski Archive for Space Telescopes. Light curve production is underway for additional TESS Cycles.

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Publication Details

Journal
Publications of the Astronomical Society of the Pacific
Published
2025-02-01
DOI
https://doi.org/10.1088/1538-3873/adad42
Citations
5
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
5.77

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article

The T16 Project: Image Subtraction Light Curves from TESS Cycle 1 Full-frame Images for Stars with T < 16

Z. Csubry, J. D. Hartman, G. Á. Bakos, Luke G. Bouma
5 citations
Publications of the Astronomical Society of the Pacific
Stellar, planetary, and galactic studies
5.77
article

The T16 Project: Image Subtraction Light Curves from TESS Cycle 1 Full-frame Images for Stars with T < 16

Z. Csubry, J. D. Hartman, G. Á. Bakos, Luke G. Bouma
article en
5 citations

Abstract

Abstract We present 83,717,159 light curves for 56,401,549 stars with T &lt; 16 mag observed in the Full-Frame Images (FFIs) of Cycle 1 of the NASA TESS mission. These light curves were extracted from subtracted images produced by the Cluster Difference Imaging Survey. We make public the raw image subtraction light curves, together with light curves de-trended against instrumental systematics. We compare the light curves to other publicly available light curves from the TESS FFIs, finding that for a substantial fraction of stars with T &lt; 16, the T16 project provides the highest precision FFI light curves available. We demonstrate that the detrended T16 light curves are generally as good as, or better than, than the light curves from other projects for the known TOIs. We also show that the un-detrended light curves can be used to study high amplitude variable stars. The light curves are being made available through the NASA Mikulski Archive for Space Telescopes. Light curve production is underway for additional TESS Cycles.

Publications of the Astronomical Society of the PacificVol. 137(2)
California Institute of Technology (US), Carnegie Institution for Science (US), Princeton University (US), Konkoly Observatory (HU), Carnegie Observatories (US)
Astrophysics Division
Openalex Percentile: Top 5%
Stellar, planetary, and galactic studies
5.77
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The T16 Project: Image Subtraction Light Curves from TESS Cycle 1 Full-frame Images for Stars with T &lt; 16 — Z. Csubry, J. D. Hartman, et al. · Publications of the Astronomical Society of the Pacific (2025) | TGRS Research Map | TGRS