Published February 27, 2025
| Version v1
Dataset
Open
JWST COMPASS: NIRSpec/G395H Transmission Observations of TOI-776 c, a 2 R⊕ M Dwarf Planet
Authors/Creators
-
Teske, Johanna
(Contact person)1
-
Batalha, Natasha
(Contact person)2
-
Wallack, Nicole
(Contact person)3
-
Kirk, James
(Contact person)4
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Wogan, Nicholas
(Project member)5
-
Gordon, Tyler
(Project member)5
-
Alam, Munazza
(Project member)6
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Aguichine, Artyom
(Project member)2
-
Wolfgang, Angie
(Project member)7
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Wakeford, Hannah
(Project member)8
-
Scarsdale, Nicholas
(Project member)
-
Adams, Jea
(Project member)9
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Moran, Sarah E.
(Project member)10
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López-Morales, Mercedes
(Project member)6
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Meech, Annabella
(Project member)
-
Gao, Peter
(Project member)
-
Batalha, Natalie
(Project member)2
-
Alderson, Lili
(Project member)
-
Gagnebin, Anna
(Project member)
- 1. Carnegie Institution for Science Earth and Planets Laboratory
-
2.
University of California, Santa Cruz
-
3.
Carnegie Institution for Science
-
4.
Imperial College London
- 5. University of Washington
-
6.
Space Telescope Science Institute
- 7. Wolfgang Independent Contracting in Astronomy and Data Science
-
8.
University of Bristol
-
9.
Amherst College
- 10. The University of Arizona Department of Planetary Sciences and Lunar and Planetary Laboratory
Description
Data and models presented in "JWST COMPASS: NIRSpec/G395H Transmission Observations of TOI-776 c, a 2 R⊕ M Dwarf Planet"
- Transmission spectra from the Tiberius and Eurkea reductions
- Fitted white light curves from both reductions
- Fitted spectroscopic light curves from both reductions
- Models, PICASO models and data for Figures 10, 11, 12, 13, and 15
- MH_Curve_Data_Figure11&15.csv : This is a comma separated file with columns for logMH, MMW, and [POC]_[VISIT]_[PRESS]logBar with POC=[NW or JK], VISIT=[v1, v2, j] and PRESS=[0,-1,-2,-3,-4].
- SpectraFigureData77601_NW_j_Figure12-14.nc : This is an xarray file where the data_vars are spectra (transit depth) for varying metallicities and water content levels, as shown in the paper in units of ppm. The coords are in wavelength micron units.
Manuscript: Teske & Batalha et al. DOI: [https://doi.org/10.3847/1538-3881/adb975]
Files
MH_Curve_Data_Figure11&15.csv
Files
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