Evidence map›Paper›PMID 40903599›Full record

ArticleNature2025

Silicate precursor silane detected in cold low-metallicity brown dwarf.

Jacqueline K Faherty, Aaron M Meisner, Ben Burningham, Channon Visscher, Michael Line, Genaro Suárez, Jonathan Gagné, Sherelyn Alejandro Merchan, Austin James Rothermich, Adam J Burgasser and 21 more

Abstract read
PubMed Publisher
In one paragraph

Article in Nature, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing 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

1 citing paper in PubMed.

  1. 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

31 authors.

Jacqueline K FahertyDepartment of Astrophysics, American Museum of Natural History, New York, NY, USA. jfaherty@amnh.org.ORCID http://orcid.org/0000-0001-6251-0573
Aaron M MeisnerNSF National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-1125-7384
Ben BurninghamDepartment of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield, UK.ORCID http://orcid.org/0000-0003-4600-5627
Channon VisscherChemistry and Planetary Sciences, Dordt University, Sioux Center, IA, USA.
Michael LineSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA.ORCID http://orcid.org/0000-0001-6247-8323
Genaro SuárezDepartment of Astrophysics, American Museum of Natural History, New York, NY, USA.ORCID http://orcid.org/0000-0002-2011-4924
Jonathan GagnéPlanétarium de Montreal, Montreal, Quebec, Canada.
Sherelyn Alejandro MerchanDepartment of Astrophysics, American Museum of Natural History, New York, NY, USA.ORCID http://orcid.org/0000-0003-0548-0093
Austin James RothermichDepartment of Astrophysics, American Museum of Natural History, New York, NY, USA.
Adam J BurgasserDepartment of Astronomy and Astrophysics, University of California, San Diego, La Jolla, CA, USA.
Adam C SchneiderFlagstaff Station, United States Naval Observatory, Flagstaff, AZ, USA.ORCID http://orcid.org/0000-0002-6294-5937
Dan CaseldenDepartment of Astrophysics, American Museum of Natural History, New York, NY, USA.ORCID http://orcid.org/0000-0001-7896-5791
J Davy KirkpatrickIPAC, Caltech, Pasadena, CA, USA.
Marc Jason KuchnerScience Mission Directorate, NASA, Washington DC, USA.
Daniella Carolina Bardalez GagliuffiDepartment of Physics and Astronomy, Amherst College, Amherst, MA, USA.
Peter EisenhardtJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
Christopher R GelinoIPAC, Caltech, Pasadena, CA, USA.
Eileen C GonzalesDepartment of Physics and Astronomy, San Francisco State University, San Francisco, CA, USA.ORCID http://orcid.org/0000-0003-4636-6676
Federico MaroccoIPAC, Caltech, Pasadena, CA, USA.ORCID http://orcid.org/0000-0001-7519-1700
Sandy LeggettNSF NOIRLab, Gemini Observatory, Hilo, HI, USA.
Nicolas LodieuInstituto de Astrofísica de Canarias, San Cristobal de La Laguna, Spain.ORCID http://orcid.org/0000-0002-3612-8968
Sarah L CasewellSchool of Physics and Astronomy, University of Leicester, Leicester, UK.ORCID http://orcid.org/0000-0003-2478-0120
Pascal TremblinMaison de la Simulation, Université Paris-Saclay, UVSQ, CNRS, CEA, Gif-sur-Yvette, France.
Michael CushingRitter Astrophysical Research Center, Department of Physics and Astronomy, University of Toledo, Toledo, OH, USA.
Maria Rosa Zapatero OsorioCentro de Astrobiología, CSIC-INTA, Madrid, Spain.ORCID http://orcid.org/0000-0001-5664-2852
Víctor J S BéjarInstituto de Astrofísica de Canarias, San Cristobal de La Laguna, Spain.ORCID http://orcid.org/0000-0002-5086-4232
Bartosz GauzaJanusz Gil Institute of Astronomy, University of Zielona Góra, Zielona Góra, Poland.ORCID http://orcid.org/0000-0001-5452-2056
Edward WrightDepartment of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA, USA.
Mark W PhillipsInstitute for Astronomy, University of Edinburgh, Edinburgh, UK.
Jun-Yan ZhangInstituto de Astrofísica de Canarias, San Cristobal de La Laguna, Spain.ORCID http://orcid.org/0000-0001-5392-2701
Eduardo L MartinInstituto de Astrofísica de Canarias, San Cristobal de La Laguna, Spain.ORCID http://orcid.org/0000-0002-1208-4833

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Within 20 pc of the Sun, there are currently 29 known cold brown dwarfs-sources with measured distances and an estimated effective temperature between that of Jupiter (170 K) and approximately 500 K (ref.

Identifiers

What OpenQuestion holds

Textmetadata
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.