The K2 and TESS Synergy. III. Search and Rescue of the Lost Ephemeris for K2's First Planet

• Published in: The Astronomical journal Vol. 168; no. 4; pp. 161 - 172
• Main Authors: Thygesen, Erica, Rodriguez, Joseph E., de Beurs, Zoë L., Vanderburg, Andrew, Livingston, John H., Irwin, Jonathon, Venner, Alexander, Cretignier, Michael, Collins, Karen A., Bieryla, Allyson, Charbonneau, David, Crossfield, Ian J. M., Dumusque, Xavier, Kielkopf, John, Latham, David W., Werner, Michael
• Format: Journal Article
• Language: English
• Published: Madison The American Astronomical Society 01.10.2024; IOP Publishing
• Subjects: Atmospheric correction; Concept engineering; Dwarf stars; Ephemerides; Exoplanet astronomy; Exoplanet catalogs; Exoplanet systems; Exoplanets; Extrasolar planets; Photometric observations; Photometry; Planet detection; Planetary atmospheres; Planets; Satellite observation; Search and rescue; Spectroscopy; Stellar activity; Transit; Transits
• ISSN: 0004-6256; 1538-3881
• DOI: 10.3847/1538-3881/ad60bf

Abstract K2-2 b/HIP 116454 b, the first exoplanet discovery by K2 during its Two-Wheeled Concept Engineering Test, is a sub-Neptune (2.5 ± 0.1 R ⊕ , 9.7 ± 1.2 M ⊕ ) orbiting a relatively bright ( K S = 8.03) K-dwarf star on a 9.1 day period. Unfortunately, due to a spurious follow-up transit detection and ephemeris degradation, the transit ephemeris for this planet was lost. In this work, we recover and refine the transit ephemeris for K2-2 b, showing a ∼40 σ discrepancy from the discovery results. To accurately measure the transit ephemeris and update the parameters of the system, we jointly fit space-based photometric observations from NASA’s K2, Transiting Exoplanet Survey Satellite, and Spitzer missions with new photometric observations from the ground, as well as radial velocities from HARPS-N that are corrected for stellar activity using a new modeling technique. Ephemerides becoming lost or significantly degraded, as is the case for most transiting planets, highlights the importance of systematically updating transit ephemerides with upcoming large efforts expected to characterize hundreds of exoplanet atmospheres. K2-2 b sits at the high-mass peak of the known radius valley for sub-Neptunes, and is now well-suited for transmission spectroscopy with current and future facilities. Our updated transit ephemeris will ensure no more than a 13 minute uncertainty through 2030.