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| Main Authors: | , , , , , , , , , , , , , |
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| Format: | Preprint |
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2026
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2601.01628 |
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| _version_ | 1866917183427182592 |
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| author | Wilson, David J. Youngblood, Allison Duvvuri, Girish M. France, Kevin Schneider, P. Christian Brown, Alexander Longo, Isabella Froning, Cynthia S. Bean, Jacob L. Pineda, J. Sebastian Kempton, Eliza M. -R. Miguel, Yamila Evans-Soma, Thomas M. Berta-Thompson, Zachory |
| author_facet | Wilson, David J. Youngblood, Allison Duvvuri, Girish M. France, Kevin Schneider, P. Christian Brown, Alexander Longo, Isabella Froning, Cynthia S. Bean, Jacob L. Pineda, J. Sebastian Kempton, Eliza M. -R. Miguel, Yamila Evans-Soma, Thomas M. Berta-Thompson, Zachory |
| contents | Correctly interpreting JWST spectra of close-in exoplanets requires a measurement of the X-ray and ultraviolet light that the planets receive from their host stars. Here we provide spectral energy distributions (SEDs) covering the range $\approx5-1\times10^7$A for 20 transiting exoplanet host stars observed in JWST Cycle 1. The SEDs are constructed out of new and archival Hubble Space Telescope, Chandra X-ray Observatory and/or XMM-Newton data combined with spectra from models or stars with similar properties (proxies) filling in unobserved gaps. We have also constructed SEDs of likely Habitable Worlds Observatory targets $κ^1$ Ceti, $τ$ Ceti, $ε$ Indi and 70 Oph B for use as proxies. We find that the JWST target planets almost all experience much stronger ultraviolet fluxes than the Earth, especially in the extreme ultraviolet, even for planets with similar overall instellation. Strong ongoing or past atmospheric escape is possible for a majority of these planets. We also assess the now considerable sample of panchromatic stellar SEDs and its applicability for current JWST observations and beyond. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2601_01628 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | The MUSCLES Extension for Atmospheric Transmission Spectroscopy: Spectral energy distributions for 20 exoplanet host stars that JWST observed in Cycle 1 Wilson, David J. Youngblood, Allison Duvvuri, Girish M. France, Kevin Schneider, P. Christian Brown, Alexander Longo, Isabella Froning, Cynthia S. Bean, Jacob L. Pineda, J. Sebastian Kempton, Eliza M. -R. Miguel, Yamila Evans-Soma, Thomas M. Berta-Thompson, Zachory Earth and Planetary Astrophysics Solar and Stellar Astrophysics Correctly interpreting JWST spectra of close-in exoplanets requires a measurement of the X-ray and ultraviolet light that the planets receive from their host stars. Here we provide spectral energy distributions (SEDs) covering the range $\approx5-1\times10^7$A for 20 transiting exoplanet host stars observed in JWST Cycle 1. The SEDs are constructed out of new and archival Hubble Space Telescope, Chandra X-ray Observatory and/or XMM-Newton data combined with spectra from models or stars with similar properties (proxies) filling in unobserved gaps. We have also constructed SEDs of likely Habitable Worlds Observatory targets $κ^1$ Ceti, $τ$ Ceti, $ε$ Indi and 70 Oph B for use as proxies. We find that the JWST target planets almost all experience much stronger ultraviolet fluxes than the Earth, especially in the extreme ultraviolet, even for planets with similar overall instellation. Strong ongoing or past atmospheric escape is possible for a majority of these planets. We also assess the now considerable sample of panchromatic stellar SEDs and its applicability for current JWST observations and beyond. |
| title | The MUSCLES Extension for Atmospheric Transmission Spectroscopy: Spectral energy distributions for 20 exoplanet host stars that JWST observed in Cycle 1 |
| topic | Earth and Planetary Astrophysics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2601.01628 |