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dc.contributor.authorMcGruder, C.D.
dc.contributor.authorLópez-Morales, M.
dc.contributor.authorKirk, J.
dc.contributor.authorEspinoza, N.
dc.contributor.authorRackham, B.V.
dc.contributor.authorAlam, M.K.
dc.contributor.authorAllen, N.
dc.contributor.authorNikolov, N.
dc.contributor.authorWeaver, I.C.
dc.contributor.authorOrtiz Ceballos, K.
dc.contributor.authorOsip, D.J.
dc.contributor.authorApai, D.
dc.contributor.authorJordán, A.
dc.contributor.authorFortney, J.J.
dc.date.accessioned2022-11-18T22:09:45Z
dc.date.available2022-11-18T22:09:45Z
dc.date.issued2022
dc.identifier.citationMcGruder, C. D., López-Morales, M., Kirk, J., Espinoza, N., Rackham, B. V., Alam, M. K., Allen, N., Nikolov, N., Weaver, I. C., Ortiz Ceballos, K., Osip, D. J., Apai, D., Jordán, A., & Fortney, J. J. (2022). ACCESS: Confirmation of a Clear Atmosphere for WASP-96b and a Comparison of Light Curve Detrending Techniques. Astronomical Journal, 164(4).
dc.identifier.issn0004-6256
dc.identifier.doi10.3847/1538-3881/ac7f2e
dc.identifier.urihttp://hdl.handle.net/10150/666835
dc.description.abstractOne of the strongest Na i features was observed in WASP-96b. To confirm this novel detection, we provide a new 475-825 nm transmission spectrum obtained with Magellan/IMACS, which indeed confirms the presence of a broad sodium absorption feature. We find the same result when reanalyzing the 400-825 nm VLT/FORS2 data. We also utilize synthetic data to test the effectiveness of two common detrending techniques: (1) a Gaussian processes (GP) routine, and (2) common-mode correction followed by polynomial correction (CMC+Poly). We find that both methods poorly reproduce the absolute transit depths but maintain their true spectral shape. This emphasizes the importance of fitting for offsets when combining spectra from different sources or epochs. Additionally, we find that, for our data sets, both methods give consistent results, but CMC+Poly is more accurate and precise. We combine the Magellan/IMACS and VLT/FORS2 spectra with literature 800-1644 nm HST/WFC3 spectra, yielding a global spectrum from 400 to 1644 nm. We used the PLATON and Exoretrievals retrieval codes to interpret this spectrum, and find that both yield relatively deeper pressures where the atmosphere is optically thick at log-pressures between 1.3 − 1.1 + 1.0 and 0.29 − 2.02 + 1.86 bars, respectively. Exoretrievals finds solar to supersolar Na i and H2O log-mixing ratios of − 5.4 − 1.9 + 2.0 and − 4.5 − 2.0 + 2.0 , respectively, while PLATON finds an overall metallicity of log 10 ( Z / Z ⊙ ) = − 0.49 − 0.37 + 1.0 dex. Therefore, our findings are in agreement with the literature and support the inference that the terminator of WASP-96b has few aerosols obscuring prominent features in the optical to near-infrared (near-IR) spectrum. © 2022. The Author(s). Published by the American Astronomical Society.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.rightsCopyright © 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.
dc.rights.urihttps://creativecommons.org/licenses/by/4.0
dc.titleACCESS: Confirmation of a Clear Atmosphere for WASP-96b and a Comparison of Light Curve Detrending Techniques
dc.typeArticle
dc.typetext
dc.contributor.departmentSteward Observatory, University of Arizona
dc.contributor.departmentLunar and Planetary Laboratory, University of Arizona
dc.identifier.journalAstronomical Journal
dc.description.noteOpen access journal
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal published version
dc.source.journaltitleAstronomical Journal
refterms.dateFOA2022-11-18T22:09:45Z


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Copyright © 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.
Except where otherwise noted, this item's license is described as Copyright © 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.