Systematic Phase Curve Study of Known Transiting Systems from Year One of the TESS Mission

Ian Wong, Avi Shporer, Tansu Daylan, Björn Benneke, Tara Fetherolf, Stephen R. Kane, George R. Ricker, Roland Vanderspek, David W. Latham, Joshua N. Winn, Jon M. Jenkins, Patricia T. Boyd, Ana Glidden, Robert F. Goeke, Lizhou Sha, Eric B. Ting, Daniel Yahalomi

Research output: Contribution to journalArticle

Abstract

We present a systematic phase curve analysis of known transiting systems observed by the Transiting Exoplanet Survey Satellite (TESS) during year one of the primary mission. Using theoretical predictions for the amplitude of the planetary longitudinal atmospheric brightness modulation, stellar ellipsoidal distortion and Doppler boosting, as well as brightness considerations to select targets with likely detectable signals, we applied a uniform data processing and light-curve modeling framework to fit the full-orbit phase curves of 22 transiting systems with planet-mass or brown dwarf companions, including previously published systems. Statistically significant secondary eclipse depths and/or atmospheric brightness modulation amplitudes were measured for HIP 65A, WASP-18, WASP-19, WASP-72, WASP-100, WASP-111, WASP-121, and WASP-122/KELT-14. For WASP-100b, we found marginal evidence that the brightest region of the atmosphere is shifted eastward away from the substellar point. We detected significant ellipsoidal distortion signals in the light curves of HIP 65A, TOI-503, WASP-18, and WASP-30, with HIP 65A, TOI-503 and WASP-18 also exhibiting Doppler boosting. The measured amplitudes of these signals agree with the predictions of theoretical models. Combining the optical secondary eclipse depths with previously published Spitzer 3.6 and 4.5 μm measurements, we derived dayside brightness temperatures and visible-light geometric albedos for a subset of the analyzed systems. We also calculated updated transit ephemerides combining the transit timings from the TESS light curves with previous literature values.

Original languageEnglish (US)
Article number155
JournalAstronomical Journal
Volume160
Issue number4
DOIs
StatePublished - Oct 2020

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Systematic Phase Curve Study of Known Transiting Systems from Year One of the TESS Mission'. Together they form a unique fingerprint.

  • Cite this

    Wong, I., Shporer, A., Daylan, T., Benneke, B., Fetherolf, T., Kane, S. R., Ricker, G. R., Vanderspek, R., Latham, D. W., Winn, J. N., Jenkins, J. M., Boyd, P. T., Glidden, A., Goeke, R. F., Sha, L., Ting, E. B., & Yahalomi, D. (2020). Systematic Phase Curve Study of Known Transiting Systems from Year One of the TESS Mission. Astronomical Journal, 160(4), [155]. https://doi.org/10.3847/1538-3881/ababad