Evidence map›Paper›PMID 41079407›Full record

ArticleThe Astrophysical journal2025

The Impact of Extended CO

Wynter Broussard, Edward W Schwieterman, Clara Sousa-Silva, Grace Sanger-Johnson, Sukrit Ranjan, Olivia Venot

Abstract read
In one paragraph

Article in The Astrophysical journal, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
0cells of the map it votes in
0citing 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

0 citing papers in PubMed.

No citing paper in PubMed yet.

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

6 authors.

Wynter BroussardDepartment of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA; abrou009@ucr.edu.ORCID https://orcid.org/0009-0006-2304-3419
Edward W SchwietermanDepartment of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA; abrou009@ucr.edu.ORCID https://orcid.org/0000-0002-2949-2163
Clara Sousa-SilvaBard College, 30 Campus Rd, Annandale-On-Hudson, NY 12504, USA.ORCID https://orcid.org/0000-0002-7853-6871
Grace Sanger-JohnsonDepartment of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA.ORCID https://orcid.org/0000-0002-4463-2902
Sukrit RanjanBlue Marble Space Institute of Science, Seattle, WA 98104, USA.ORCID https://orcid.org/0000-0002-5147-9053
Olivia VenotUniversité Paris Cité and Univ. Paris Est Creteil, CNRS, LISA, F-75013 Paris, France.ORCID https://orcid.org/0000-0003-2854-765X

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Our interpretation of terrestrial exoplanet atmospheric spectra will always be limited by the accuracy of the data we use as input in our forward and retrieval models. Ultraviolet molecular absorption cross sections are one category of these essential model inputs; however, they are often poorly characterized at the longest wavelengths relevant to photodissociation. Photolysis reactions dominate the chemical kinetics of temperate terrestrial planet atmospheres. One molecule of particular importance is CO

Identifiers

PMID41079407
PMCPMC12513620

What OpenQuestion holds

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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.