scholarly journals LOFAR/H-ATLAS: the low-frequency radio luminosity–star formation rate relation

2018 ◽  
Vol 475 (3) ◽  
pp. 3010-3028 ◽  
Author(s):  
G Gürkan ◽  
M J Hardcastle ◽  
D J B Smith ◽  
P N Best ◽  
N Bourne ◽  
...  
Keyword(s):  
Star Formation ◽  
Star Formation Rate ◽  
Formation Rate ◽  
Low Frequency ◽  
Radio Luminosity ◽  
Rate Relation

scholarly journals THE RADIO CONTINUUM-STAR FORMATION RATE RELATION IN WSRT SINGS GALAXIES

2014 ◽  
Vol 147 (5) ◽  
pp. 103 ◽  
Author(s):  
Volker Heesen ◽  
Elias Brinks ◽  
Adam K. Leroy ◽  
George Heald ◽  
Robert Braun ◽  
...  
Keyword(s):  
Star Formation ◽  
Star Formation Rate ◽  
Formation Rate ◽  
Radio Continuum ◽  
Rate Relation

scholarly journals The local star formation rate and radio luminosity density

2002 ◽  
Vol 330 (3) ◽  
pp. 621-624 ◽  
Author(s):  
Stephen Serjeant ◽  
Carlotta Gruppioni ◽  
Seb Oliver
Keyword(s):  
Star Formation ◽  
Star Formation Rate ◽  
Formation Rate ◽  
Radio Luminosity

scholarly journals SHAPING THE DUST MASS-STAR-FORMATION RATE RELATION

2014 ◽  
Vol 782 (2) ◽  
pp. L23 ◽  
Author(s):  
Jens Hjorth ◽  
Christa Gall ◽  
Michał J. Michałowski
Keyword(s):  
Star Formation ◽  
Star Formation Rate ◽  
Formation Rate ◽  
Mass Star ◽  
Dust Mass ◽  
Rate Relation

scholarly journals Measuring the cosmic star-formation rate density using deep radio surveys

2007 ◽  
Vol 3 (S245) ◽  
pp. 415-416
Author(s):  
T. Dwelly ◽  
N. Seymour ◽  
I. M. McHardy ◽  
D. Moss ◽  
M. Page ◽  
...  
Keyword(s):  
Star Formation ◽  
Radio Emission ◽  
Star Formation Rate ◽  
Formation Rate ◽  
Starburst Galaxies ◽  
Radio Luminosity ◽  
Blank Field ◽  
Star Forming ◽  
Dust Absorption ◽  
Good Agreement

There is now good agreement between the various methods of estimating the space density of the star-formation rate (SFRD) at low redshifts (z < 1), with uncertainties around 30–50%. However, the situation at higher redshifts remains much less clear, with uncertainties in the SFRD, due to e.g. poorly known dust absorption corrections, of as much as 300–500%. Radio emission from star-forming galaxies is unaffected by absorption and scales linearly with star-formation rate, thus the radio luminosity of star-forming galaxies provides an excellent independent, unbiased measure of their star-formation rate. The current deepest ‘blank field’ radio surveys (reaching <10 μJy rms at 1.4 GHz) are sensitive enough to detect starburst galaxies out to z ~ 3, and so potentially offer an excellent way to measure the SFRD. Indeed, modelling of the sub-mJy source counts requires an additional population of faint steep spectrum objects, that are very likely to be starburst galaxies.

scholarly journals Does the evolution of the radio luminosity function of star-forming galaxies match that of the star formation rate function?

2017 ◽  
Vol 469 (2) ◽  
pp. 1912-1923 ◽  
Author(s):  
Matteo Bonato ◽  
Mattia Negrello ◽  
Claudia Mancuso ◽  
Gianfranco De Zotti ◽  
Paolo Ciliegi ◽  
...  
Keyword(s):  
Star Formation ◽  
Luminosity Function ◽  
Star Formation Rate ◽  
Formation Rate ◽  
Rate Function ◽  
Radio Luminosity ◽  
Star Forming ◽  
Radio Luminosity Function
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