Sie befinden Sich nicht im Netzwerk der Universität Paderborn. Der Zugriff auf elektronische Ressourcen ist gegebenenfalls nur via VPN oder Shibboleth (DFN-AAI) möglich. mehr Informationen...
Ergebnis 1 von 11
Monthly notices of the Royal Astronomical Society. Letters, 2016-02, Vol.457 (1), p.L127-L131
2016
Volltextzugriff (PDF)

Details

Autor(en) / Beteiligte
Titel
The high-redshift star formation history from carbon-monoxide intensity maps
Ist Teil von
  • Monthly notices of the Royal Astronomical Society. Letters, 2016-02, Vol.457 (1), p.L127-L131
Ort / Verlag
Oxford University Press
Erscheinungsjahr
2016
Quelle
Alma/SFX Local Collection
Beschreibungen/Notizen
  • We demonstrate how cosmic star formation history can be measured with one-point statistics of carbon-monoxide intensity maps. Using a P(D) analysis, the luminosity function of CO-emitting sources can be inferred from the measured one-point intensity PDF. The star formation rate density (SFRD) can then be obtained, at several redshifts, from the CO luminosity density. We study the effects of instrumental noise, line foregrounds, and target redshift, and obtain constraints on the CO luminosity density of the order of 10 per cent. We show that the SFRD uncertainty is dominated by that of the model connecting CO luminosity and star formation. For pessimistic estimates of this model uncertainty, we obtain an error of the order of 50 per cent on SFRD for surveys targeting redshifts between two and seven with reasonable noise and foregrounds included. However, comparisons between intensity maps and galaxies could substantially reduce this model uncertainty. In this case, our constraints on SFRD at these redshifts improve to roughly 5 − 10 per cent, which is highly competitive with current measurements.
Sprache
Englisch
Identifikatoren
ISSN: 1745-3925
eISSN: 1745-3933
DOI: 10.1093/mnrasl/slw005
Titel-ID: cdi_crossref_primary_10_1093_mnrasl_slw005
Format

Weiterführende Literatur

Empfehlungen zum selben Thema automatisch vorgeschlagen von bX