Evidence map›Paper›PMID 39009611›Full record

ArticleNature communications2024

Laboratory infrared spectra and fragmentation chemistry of sulfur allotropes.

Piero Ferrari, Giel Berden, Britta Redlich, Laurens B F M Waters, Joost M Bakker

Abstract read
In one paragraph

Article in Nature communications, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing 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

5 citing papers in PubMed.

  1. Article
  2. Article
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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

5 authors.

Piero FerrariRadboud University, Institute for Molecules and Materials, FELIX Laboratory, Nijmegen, The Netherlands. piero.ferrariramirez@ru.nl.ORCID http://orcid.org/0000-0001-6096-7772
Giel BerdenRadboud University, Institute for Molecules and Materials, FELIX Laboratory, Nijmegen, The Netherlands.ORCID http://orcid.org/0000-0003-1500-922X
Britta RedlichRadboud University, Institute for Molecules and Materials, FELIX Laboratory, Nijmegen, The Netherlands.
Laurens B F M WatersDepartment of Astrophysics, IMAPP, Radboud University, Nijmegen, The Netherlands.
Joost M BakkerRadboud University, Institute for Molecules and Materials, FELIX Laboratory, Nijmegen, The Netherlands.ORCID http://orcid.org/0000-0002-1394-7661

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Sulfur is one of six life-essential elements, but its path from interstellar clouds to planets and their atmospheres is not well known. Astronomical observations in dense clouds have so far been able to trace only 1 percent of cosmic sulfur, in the form of gas phase molecules and volatile ices, with the missing sulfur expected to be locked in a currently unidentified form. The high sulfur abundances inferred in icy and rocky solar system bodies indicate that an efficient pathway must exist from volatile atomic sulfur in the diffuse interstellar medium to some form of refractory sulfur. One hypothesis is the formation of sulfur allotropes, particularly of the stable S

Identifiers

PMID39009611
PMCPMC11251068

What OpenQuestion holds

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Registered trials

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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.