Evidence map›Paper›PMID 32565548›Full record

ArticleAstronomy and astrophysics2020

Gas phase Elemental abundances in Molecular cloudS (GEMS) II. On the quest for the sulphur reservoir in molecular clouds: the H

D Navarro-Almaida, R Le Gal, A Fuente, P Rivière-Marichalar, V Wakelam, S Cazaux, P Caselli, Jacob C Laas, T Alonso-Albi, J C Loison and 23 more

Open access · bronzeAbstract read
In one paragraph

Article in Astronomy and astrophysics, 2020. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 7 papers.

0numbers the graph read from it
0cells of the map it votes in
7citing papers in PubMed
6.6field-weighted citation impact, top 3% of its field
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

7 citing papers in PubMed, 79 citations in OpenAlex.

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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

33 authors at 13 institutions in 9 countries.

D Navarro-AlmaidaObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
R Le GalHarvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA.
A FuenteObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
P Rivière-MarichalarObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
V WakelamLaboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France.
S CazauxFaculty of Aerospace Engineering, Delft University of Technology, Delft, The Netherlands; University of Leiden, P.O. Box 9513, NL, 2300 RA, Leiden, The Netherlands.
P CaselliCentre for Astrochemical Studies, Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, 85748, Garching, Germany.
Jacob C LaasCentre for Astrochemical Studies, Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, 85748, Garching, Germany.
T Alonso-AlbiObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
J C LoisonInstitut des Sciences Moléculaires (ISM), CNRS, Univ. Bordeaux, 351 cours de la Libération, F-33400, Talence, France.
M GerinObservatoire de Paris, PSL Research University, CNRS, École Normale Supérieure, Sorbonne Universités, UPMC Univ. Paris 06, 75005, Paris, France.
C KramerInstituto Radioastronomía Milimétrica (IRAM), Av. Divina Pastora 7, Nucleo Central, 18012, Granada, Spain.
E RoueffSorbonne Université, Observatoire de Paris, Université PSL, CNRS, LERMA, F-92190, Meudon, France.
R BachillerObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
B CommerçonÉcole Normale Supérieure de Lyon, CRAL, UMR CNRS 5574, Université Lyon I, 46 Allée d'Italie, 69364, Lyon Cedex 07, France.
R FriesenNational Radio Astronomy Observatory, 520 Edgemont Rd., Charlottesville VA USA 22901.
S García-BurilloObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
J R GoicoecheaInstituto de Física Fundamental (CSIC), Calle Serrano 123, 28006, Madrid, Spain.
B M GiulianoCentre for Astrochemical Studies, Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, 85748, Garching, Germany.
I Jiménez-SerraCentro de Astrobiología (CSIC-INTA), Ctra. de Ajalvir, km 4, Torrejón de Ardoz, 28850, Madrid, Spain.
J M KirkJeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK.
V LattanziCentre for Astrochemical Studies, Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, 85748, Garching, Germany.
J MalinenDepartment of Physics, University of Helsinki, PO Box 64, 00014, Helsinki, Finland.
N MarcelinoInstituto de Física Fundamental (CSIC), Calle Serrano 123, 28006, Madrid, Spain.
R Martín-DomènechHarvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA.
G M Muñoz CaroCentro de Astrobiología (CSIC-INTA), Ctra. de Ajalvir, km 4, Torrejón de Ardoz, 28850, Madrid, Spain.
J PinedaCentre for Astrochemical Studies, Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, 85748, Garching, Germany.
B TerceroObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
S P Treviño-MoralesChalmers University of Technology, Department of Space, Earth and Environment, SE-412 93 Gothenburg, Sweden.
O RonceroInstituto de Física Fundamental (CSIC), Calle Serrano 123, 28006, Madrid, Spain.
A HacarLeiden Observatory, Leiden University, PO Box 9513, 2300-RA, Leiden, The Netherlands.
M TafallaObservatorio Astronómico Nacional (OAN), Alfonso XII, 3, 28014, Madrid, Spain.
D Ward-ThompsonJeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK.
Spanish National Observatory · ESMax Planck Institute for Extraterrestrial Physics · DECentre National de la Recherche Scientifique · FRInstituto de Física Fundamental · ESCenter for Astrophysics Harvard & Smithsonian · USCentro de Astrobiología · ESLeiden University · NLUniversity of Lancashire · GBChalmers University of Technology · SEInstituto de Radioastronomía Milimétrica · ESNational Radio Astronomy Observatory · USUniversité Claude Bernard Lyon 1 · FRUniversity of Helsinki · FI

Funding

European Research Council 610256
6 · The paper itself

Abstract

contextSulphur is one of the most abundant elements in the Universe. Surprisingly, sulphuretted molecules are not as abundant as expected in the interstellar medium and the identity of the main sulphur reservoir is still an open question.

aimsOur goal is to investigate the H

methodsUsing millimeter observations of CS, SO, H

resultsOur modeling shows that chemical desorption is the main source of gas-phase H

conclusionsThe gaseous H

Indexed as

astrochemistry – ISMclouds – submillimeterISMmolecules – ISM

Identifiers

PMID32565548
PMCPMC7305024
OpenAlexW3015467411

What OpenQuestion holds

Textmetadata
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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.