Cosmic Evolution of Gas and Star Formation
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583825" target="_blank" >RIV/67985815:90259/23:00583825 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.3847/1538-4357/aca1bc" target="_blank" >https://doi.org/10.3847/1538-4357/aca1bc</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/1538-4357/aca1bc" target="_blank" >10.3847/1538-4357/aca1bc</a>
Alternative languages
Result language
angličtina
Original language name
Cosmic Evolution of Gas and Star Formation
Original language description
Atacama Large Millimeter/submillimeter Array (ALMA) observations of the long-wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming galaxies at z = 0.3-4.5. We determine the dependence of gas masses and star formation efficiencies (SFEs, SFR per unit gas mass) on redshift (z), M *, and star formation rate (SFR) relative to the main sequence (MS). We find that 70% of the increase in SFRs of the MS is due to the increased gas masses at earlier epochs, while 30% is due to increased efficiency of star formation (SF).
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
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Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysical Journal
ISSN
0004-637X
e-ISSN
1538-4357
Volume of the periodical
943
Issue of the periodical within the volume
2
Country of publishing house
GB - UNITED KINGDOM
Number of pages
18
Pages from-to
82
UT code for WoS article
000922615200001
EID of the result in the Scopus database
2-s2.0-85147215742