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• W3104582511 abstract "We present a study of the morphological nature of redshift z~0.7 star-forming galaxies using a combination of HST/ACS, GALEX and ground-based images of the COSMOS field. Our sample consists of 8,146 galaxies, 5,777 of which are detected in the GALEX near-ultraviolet band down to a limiting magnitude of 25.5 (AB). We make use of the UV to estimate star formation rates, correcting for the effect of dust using the UV-slope, and compute, from the ACS F814W images, the C,A,S,G,M20 morphological parameters for all objects in our sample. We observe a morphological bimodality in the galaxy population and show that it has a strong correspondence with the FUV - g color bimodality. We conclude that UV-optical color predominantly evolves concurrently with morphology. We observe many of the most star-forming galaxies to have morphologies approaching that of early-type galaxies, and interpret this as evidence that strong starburst events are linked to bulge growth and constitute a process through which galaxies can be brought from the blue to the red sequence while simultaneously modifying their morphology accordingly. We conclude that the red sequence has continued growing at z~<0.7. We also observe z~0.7 galaxies to have physical properties similar to that of local galaxies, except for higher star formation rates. Whence we infer that the dimming of star-forming galaxies is responsible for most of the evolution in the star formation rate density of the Universe since that redshift, although our data are also consistent with a mild number evolution. [abridged]" @default.
• W3104582511 created "2020-11-23" @default.
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• W3104582511 date "2007-09-01" @default.
• W3104582511 modified "2023-10-16" @default.
• W3104582511 title "Deep <i>GALEX</i> Imaging of the COSMOS <i>HST</i> Field: A First Look at the Morphology of <i>z</i> ∼ 0.7 Star‐forming Galaxies" @default.
• W3104582511 cites W1607434071 @default.
• W3104582511 cites W1847269195 @default.
• W3104582511 cites W1969005644 @default.
• W3104582511 cites W1969396761 @default.
• W3104582511 cites W1969628537 @default.
• W3104582511 cites W1970440163 @default.
• W3104582511 cites W1970517322 @default.
• W3104582511 cites W1982104044 @default.
• W3104582511 cites W1982686285 @default.
• W3104582511 cites W1985771209 @default.
• W3104582511 cites W1985789402 @default.
• W3104582511 cites W1987402993 @default.
• W3104582511 cites W1989362633 @default.
• W3104582511 cites W1993839984 @default.
• W3104582511 cites W1994671833 @default.
• W3104582511 cites W1996537612 @default.
• W3104582511 cites W2000470824 @default.
• W3104582511 cites W2007055314 @default.
• W3104582511 cites W2007741717 @default.
• W3104582511 cites W2012543417 @default.
• W3104582511 cites W2013355735 @default.
• W3104582511 cites W2018388366 @default.
• W3104582511 cites W2018828554 @default.
• W3104582511 cites W2019615555 @default.
• W3104582511 cites W2027653586 @default.
• W3104582511 cites W2029965202 @default.
• W3104582511 cites W2032020213 @default.
• W3104582511 cites W2033279414 @default.
• W3104582511 cites W2033731878 @default.
• W3104582511 cites W2035820594 @default.
• W3104582511 cites W2037870704 @default.
• W3104582511 cites W2039833992 @default.
• W3104582511 cites W2048152489 @default.
• W3104582511 cites W2048186190 @default.
• W3104582511 cites W2048265872 @default.
• W3104582511 cites W2049020672 @default.
• W3104582511 cites W2058379217 @default.
• W3104582511 cites W2061140827 @default.
• W3104582511 cites W2062266008 @default.
• W3104582511 cites W2066202006 @default.
• W3104582511 cites W2068340869 @default.
• W3104582511 cites W2070677059 @default.
• W3104582511 cites W2071079352 @default.
• W3104582511 cites W2072404641 @default.
• W3104582511 cites W2072944584 @default.
• W3104582511 cites W2079227246 @default.
• W3104582511 cites W2079597783 @default.
• W3104582511 cites W2080927107 @default.
• W3104582511 cites W2082182881 @default.
• W3104582511 cites W2082266584 @default.
• W3104582511 cites W2088761263 @default.
• W3104582511 cites W2092504858 @default.
• W3104582511 cites W2093124600 @default.
• W3104582511 cites W2093697839 @default.
• W3104582511 cites W2095369941 @default.
• W3104582511 cites W2097351307 @default.

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