prikaz prve stranice dokumenta Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?
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Scientific paper - Original scientific paper
Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?
Monthly Notices of the Royal Astronomical Society, 469 (2017), 2; 1912-1923. https://doi.org/10.1093/mnras/stx974
Bonato, Matteo; Negrello, Mattia; Mancuso, Claudia; De Zotti, Gianfranco; Ciliegi, Paolo; Cai, Zhen-Yi; Lapi, Andrea; Massardi, Marcella; Bonaldi, Anna; Sajina, Anna; Smolčić, Vernesa; Schinnerer, Eva

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Bonato, M., Negrello, M., Mancuso, C., De Zotti, G., Ciliegi, P., Cai, Z. Y. ... Schinnerer, E. (2017). Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?. Monthly Notices of the Royal Astronomical Society, 469. (2), 1912-1923. doi: 10.1093/mnras/stx974

Bonato, Matteo, et al. "Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?." Monthly Notices of the Royal Astronomical Society, vol. 469, no. 2, 2017, pp. 1912-1923. https://doi.org/10.1093/mnras/stx974

Bonato, Matteo, Mattia Negrello, Claudia Mancuso, Gianfranco De Zotti, Paolo Ciliegi, Zhen Yi Cai, Andrea Lapi, et al. "Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?." Monthly Notices of the Royal Astronomical Society 469, no. 2 (2017): 1912-1923. https://doi.org/10.1093/mnras/stx974

Bonato, M., et al. (2017) 'Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?', Monthly Notices of the Royal Astronomical Society, 469(2), pp. 1912-1923. doi: 10.1093/mnras/stx974

Bonato M, Negrello M, Mancuso C, De Zotti G, Ciliegi P, Cai ZY, and sur.. Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?. Monthly Notices of the Royal Astronomical Society [Internet]. 2017 [cited 2024 April 18];469(2):1912-1923. doi: 10.1093/mnras/stx974

M. Bonato, et al., "Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?", Monthly Notices of the Royal Astronomical Society, vol. 469, no. 2, pp. 1912-1923, 2017. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:777970. [Accessed: 18 April 2024]

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Metadata
Title (english)Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?
AuthorMatteo Bonato
AuthorMattia Negrello
AuthorClaudia Mancuso
AuthorGianfranco De Zotti
AuthorPaolo Ciliegi
AuthorZhen-Yi Cai
AuthorAndrea Lapi
AuthorMarcella Massardi
AuthorAnna Bonaldi
AuthorAnna Sajina
AuthorVernesa Smolčić
MBZ: 336180
AuthorEva Schinnerer
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Astronomy and Astrophysics
Abstract (english)
The assessment of the relationship between radio continuum luminosity and star formation rate (SFR) is of crucial importance to make reliable predictions for the forthcoming ultra- deep radio surveys and to allow a full exploitation of their results to measure the cosmic star formation history. We have addressed this issue by matching recent accurate determinations of the SFR function up to high redshifts with literature estimates of the 1.4 GHz luminosity functions of star- forming galaxies (SFGs). This was done considering two options, proposed in the literature, for the relationship between the synchrotron emission (Lsynch), that dominates at 1.4 GHz, and the SFR: a linear relation with a decline of the Lsynch/SFR ratio at low luminosities or a mildly non-linear relation at all luminosities. In both cases, we get good agreement with the observed radio luminosity functions but, in the non-linear case, the deviation from linearity must be small. The luminosity function data are consistent with a moderate increase of the Lsynch/SFR ratio with increasing redshift, indicated by other data sets, although a constant ratio cannot be ruled out. A stronger indication of such increase is provided by recent deep 1.4-GHz counts, down to μJy levels. This is in contradiction with models predicting a decrease of that ratio due to inverse Compton cooling of relativistic electrons at high redshifts. Synchrotron losses appear to dominate up to z ≃ 5. We have also updated the Massardi et al. evolutionary model for radio loud AGNs.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleMonthly Notices of the Royal Astronomical Society
Numberingvol. 469, no. 2, pp. 1912-1923
p-ISSN0035-8711
e-ISSN1365-2966
DOIhttps://doi.org/10.1093/mnras/stx974
URN:NBNurn:nbn:hr:217:777970
Publication2017
Document URLhttps://academic.oup.com/mnras/article/469/2/1912/3778005
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
Created on2020-02-27 19:59:36