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The Canada-France Redshift Survey XIII: The luminosity density and star-formation history of the Universe to z 1,” Astrophys - Lilly, Fevre, et al. - 1996 () Citation Context ...arge range of wavelengths have improved our understanding of the galaxy luminosity function. This has allowed ...
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upper left), stellar metallicity (Z★/Z⊙, upper middle),t★(Myr, upper right), star-formation rate averaged over the previous 10 million years (SFR10(M⊙ yr−1), lower left), diffuse dust attenuation as measured in the V band (AV(mag), lower...
ABSTRACT. Given the sensitivity of the resonant Lyman $\alpha$ (Ly $\alpha $) transition to absorption by neutral hydrogen, observations of Ly $\alpha$ emi
which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through ADAP grant 80NSSC18K0945, NSF grant AST 1815458 and through an award issued by JPL/Caltech. I thank B. Lemaux and V. Strait...
consistent with expectations based on the empirical star-forming main sequence derived at lower redshifts (z ≈ 8; for example, ref.22). Taken together with the measured half-light radius, the star-formation rates imply star-formation rate surface densitiesΣSFR ≈ 64 M⊙ yr...
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Over the wide-area covered by this survey, we find no strong evidence for large scale clustering of LAEs. We estimate a star formation rate (SFR) density of ∼ 7 × 10 −4 M ⊙ yr −1 Mpc −3 for LAEs at z≈ 5.7, and compare it with previous measurements. ...
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