JWST-TST DREAMS: A Super-Solar Metallicity in WASP-17 b Dayside Atmosphere from NIRISS SOSS Eclipse Spectroscopy
Am\'elie Gressier, Ryan J. MacDonald, N\'estor Espinoza, Hannah R., Wakeford, Nikole K. Lewis, Jayesh Goyal, Dana R. Louie, Michael Radica,, Natasha E. Batalha, Douglas Long, Erin M. May, Elijah Mullens, Sara Seager,, Kevin B. Stevenson, Jeff A. Valenti, Lili Alderson

TL;DR
This study presents the first emission spectrum of the hot Jupiter WASP-17 b using JWST, revealing super-solar water abundance and a non-inverted temperature profile, with implications for atmospheric composition and observational techniques.
Contribution
First JWST emission spectrum of WASP-17 b showing super-solar water and non-inverted temperature profile, highlighting sensitivity to data analysis choices.
Findings
Detection of H2O at 6.4 sigma significance.
Evidence for a non-inverted temperature-pressure profile.
Potential high internal temperature or reflected light contributions.
Abstract
We present the first emission spectrum of the hot Jupiter WASP-17 b using one eclipse observation from the JWST Near Infrared Imager and Slitless Spectrograph (NIRISS) Single Object Slitless Spectroscopy (SOSS) mode. Covering a wavelength range of 0.6 to 2.8 microns, our retrieval analysis reveals a strong detection of H2O in WASP-17b dayside atmosphere (6.4sigma). Our retrievals consistently favor a super-solar dayside H2O abundance and a non-inverted temperature-pressure profile over a large pressure range. Additionally, our examination of the brightness temperature reveals excess emission below 1 microns, suggesting the possibility of a high internal temperature (600 to 700 K) and/or contributions from reflected light. We highlight that JWST emission spectroscopy retrieval results can be sensitive to whether negative eclipse depths are allowed at optical wavelengths during light…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Atmospheric Ozone and Climate · Calibration and Measurement Techniques
