Trends in Spitzer Secondary Eclipses
Nicole L. Wallack, Heather A. Knutson, and Drake Deming

TL;DR
This study presents new Spitzer secondary eclipse measurements for five gas giant exoplanets, confirming the dominant role of incident stellar flux in shaping their atmospheric properties and finding no significant influence from surface gravity or host star metallicity.
Contribution
It provides new observational data for five exoplanets and analyzes their atmospheric characteristics in the context of existing samples, emphasizing incident flux as the key factor.
Findings
Incident flux is the primary determinant of atmospheric chemistry.
All planets except WASP-7b have circular orbits.
No significant correlation with surface gravity or host star metallicity.
Abstract
It is well-established that the magnitude of the incident stellar flux is the single most important factor in determining the day-night temperature gradients and atmospheric chemistries of short-period gas giant planets. However it is likely that other factors, such as planet-to-planet variations in atmospheric metallicity, C/O ratio, and cloud properties, also contribute to the observed diversity of infrared spectra for this population of planets. In this study we present new 3.6 and 4.5 micron secondary eclipse measurements for five transiting gas giant planets: HAT-P-5b, HAT-P-38b, WASP-7b, WASP-72b, and WASP-127b. We detect eclipses in at least one bandpass for all five planets and confirm circular orbits for all planets except for WASP-7b, which shows evidence for a non-zero eccentricity. Building on the work of Garhart et al. (2020), we place these new planets into a broader…
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