Spectroscopic Time-series Performance of JWST/NIRSpec from Commissioning Observations
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Author
Espinoza, N.Úbeda, L.
Birkmann, S.M.
Ferruit, P.
Valenti, J.A.
Sing, D.K.
Rustamkulov, Z.
Regan, M.
Kendrew, S.
Sabbi, E.
Schlawin, E.
Beatty, T.
Albert, L.
Greene, T.P.
Nikolov, N.
Karakla, D.
Keyes, C.
Alves de Oliveira, C.
Böker, T.
Pena-Guerrero, M.
Giardino, G.
Kumari, N.
Manjavacas, E.
Proffitt, C.
Rawle, T.
Affiliation
Steward Observatory, University of ArizonaIssue Date
2023-01-30
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Institute of PhysicsCitation
Néstor Espinoza et al 2023 PASP 135 018002Rights
© 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence.Collection Information
This 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.Abstract
We report on James Webb Space Telescope (JWST) commissioning observations of the transiting exoplanet HAT-P-14 b, obtained using the Bright Object Time Series (BOTS) mode of the NIRSpec instrument with the G395H/F290LP grating/filter combination (3-5 μm). While the data were used primarily to verify that the NIRSpec BOTS mode is working as expected, and to enable it for general scientific use, they yield a precise transmission spectrum which we find is featureless down to the precision level of the instrument, consistent with expectations given HAT-P-14 b’s small scale-height and hence expected atmospheric features. The exquisite quality and stability of the JWST/NIRSpec transit spectrum—almost devoid of any systematic effects—allowed us to obtain median uncertainties of 50-60 ppm in this wavelength range at a resolution of R = 100 in a single exposure, which is in excellent agreement with pre-flight expectations and close to the (or at the) photon-noise limit for a J = 9.094, F-type star like HAT-P-14. These observations showcase the ability of NIRSpec/BOTS to perform cutting-edge transiting exoplanet atmospheric science, setting the stage for observations and discoveries to be made in Cycle 1 and beyond. © 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved.Note
Open access articleISSN
0004-6280Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1088/1538-3873/aca3d3
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Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence.

