Evidence map›Paper›PMID 40982673›Full record

ArticleProceedings of the National Academy of Sciences of the United States of America2025

A precise metallicity and carbon-to-oxygen ratio for a warm giant exoplanet from its panchromatic JWST emission spectrum.

Lindsey S Wiser, Taylor J Bell, Michael R Line, Everett Schlawin, Thomas G Beatty, Luis Welbanks, Thomas P Greene, Vivien Parmentier, Matthew M Murphy, Jonathan J Fortney and 4 more

Abstract read
In one paragraph

Article in Proceedings of the National Academy of Sciences of the United States of America, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

2 citing papers in PubMed.

  1. A precise metallicity and carbon-to-oxygen ratio for a warm giant exoplanet from its panchromatic JWST emission spectrum.Proceedings of the National Academy of Sciences of the United States of America · 2025
    Article
  2. Characterization of exoplanets in the James Webb Space Telescope era.Proceedings of the National Academy of Sciences of the United States of America · 2025
    Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

14 authors.

Lindsey S WiserSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287.ORCID 0000-0002-3295-1279
Taylor J BellBay Area Environmental Research Institute, NASA Ames Research Center, Moffett Field, CA 94035.
Michael R LineSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287.
Everett SchlawinDepartment of Astronomy, Steward Observatory, University of Arizona, Tucson, AZ 85721.
Thomas G BeattyDepartment of Astronomy, University of Wisconsin-Madison, Madison, WI 53706.
Luis WelbanksSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287.
Thomas P GreeneSpace Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, CA 94035.
Vivien ParmentierLaboratoire Lagrange, Observatoire de la Côte d'Azur, Université Côte d'Azur, Nice 06300, France.
Matthew M MurphyDepartment of Astronomy, Steward Observatory, University of Arizona, Tucson, AZ 85721.
Jonathan J FortneyDepartment of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA 95064.ORCID 0000-0002-9843-4354
Kenny ArnoldDepartment of Astronomy, University of Wisconsin-Madison, Madison, WI 53706.
Nishil MehtaLaboratoire Lagrange, Observatoire de la Côte d'Azur, Université Côte d'Azur, Nice 06300, France.ORCID 0000-0001-6086-4175
Kazumasa OhnoDivision of Science, National Astronomical Observatory of Japan, Tokyo 181-8588, Japan.
Sagnick MukherjeeDepartment of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA 95064.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

WASP-80 b, a warm sub-Jovian (equilibrium temperature [Formula: see text]820 K, 0.5 Jupiter masses), presents an opportunity to characterize a rare gas giant exoplanet around a low-mass star. In addition, its moderate temperature enables its atmosphere to host a range of carbon and oxygen species (H

Indexed as

atmospheresexoplanetsJWSTplanet formationWASP-80 b

Identifiers

PMID40982673
PMCPMC12501160

What OpenQuestion holds

Textmetadata
LicenceCC BY-NC-ND
Read underepoch 390

Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.