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TOI-1075 b: A Dense, Massive, Ultra-short-period Hot Super-Earth Straddling the Radius Gap

  • Authors: Zahra Essack, Avi Shporer, Jennifer A. Burt, Sara Seager, Saverio Cambioni, Zifan Lin, Karen A. Collins, Eric E. Mamajek, Keivan G. Stassun, George R. Ricker, Roland Vanderspek, David W. Latham, Joshua N. Winn, Jon M. Jenkins, R. Paul Butler, David Charbonneau, Kevin I. Collins, Jeffrey D. Crane, Tianjun Gan, Coel Hellier, Steve B. Howell, Jonathan Irwin, Andrew W. Mann, Ali Ramadhan, Stephen A. Shectman, Johanna K. Teske, Samuel W. Yee, Ismael Mireles, Elisa V. Quintana, Peter Tenenbaum, Guillermo Torres, Elise Furlan

Zahra Essack et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 4.

TESS light curves of TOI-1075. Top: detrended, normalized, and flattened PDCSAP flux measurements for Sector 13 (left) and Sector 27 (right). Lighter gray points are the TESS 2 minute cadence flux measurements; darker points are the same data binned into 30 minute intervals. The transits of TOI-1075 b are marked by orange triangles. Middle: phase-folded light curve on the planet’s orbital period (0.605 day), along with the best-fit transit model (red). Gray points are 2 minute cadence measurements; white points are the same data binned into 5 minute intervals. Bottom: residuals after the data have been subtracted from the best-fit model.

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