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Disambiguation of "Bowler, R. A. A."

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Changing physical conditions in star-forming galaxies between redshifts 0 < z < 4: OIII/Hb evolution

, , , , , and . (2016)cite arxiv:1605.04228Comment: 13 pages, 5 figures, accepted for publication in MNRAS.

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R. A. A. Bowler

Federico B A A R Matousek

M A R Meier

Felix A R Müller

Volker A R Huss

 

Other publications of authors with the same name

Changing physical conditions in star-forming galaxies between redshifts 0 < z < 4: OIII/Hb evolution, , , , , and . (2016)cite arxiv:1605.04228Comment: 13 pages, 5 figures, accepted for publication in MNRAS.The environment and host haloes of the brightest z~6 Lyman-break galaxies, , , and . (2017)cite arxiv:1702.03309Comment: MNRAS submitted, 18 pages, 8 figures.Normal, Dust-Obscured Galaxies in the Epoch of Reionization, , , , , , , , , and 19 other author(s). (2021)cite arxiv:2109.10378Comment: 16 pages, 7 figures, 4 tables, published in Nature.The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1312.5643Comment: 35 pages, 13 figures, submitted to MNRAS.The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging, , , , , , , , , and 3 other author(s). (2022)cite arxiv:2207.12356Comment: 28 pages, 4 figures in main manuscript, submitted to MNRAS.The rapid transition from star-formation to AGN dominated rest-frame UV light at z ~ 4, , , and . (2021)cite arxiv:2101.01195Comment: 17 pages, 11 figures, 2 tables. Accepted to MNRAS.The total rest-frame UV luminosity function from $3 < z < 5$: A simultaneous study of AGN and galaxies from $-28<M_UV<-16$, , , , and . (2022)cite arxiv:2207.09342Comment: 20 pages, 5 Tables, 12 Figures, Submitted to MNRAS.Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1709.06102Comment: 17 pages, 7 figures, submitted to MNRAS.