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

F. Cullen, M. Cirasuolo, L. Kewley, R. McLure, J. Dunlop, и R. Bowler. (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

R F A Moritz

Другие публикации лиц с тем же именем

The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?R. Bowler, J. Dunlop, R. McLure, A. Rogers, H. McCracken, B. Milvang-Jensen, H. Furusawa, J. Fynbo, Y. Taniguchi, J. Afonso и 2 other автор(ы). (2013)cite arxiv:1312.5643Comment: 35 pages, 13 figures, submitted to MNRAS.Changing physical conditions in star-forming galaxies between redshifts 0 < z < 4: OIII/Hb evolutionF. Cullen, M. Cirasuolo, L. Kewley, R. McLure, J. Dunlop, и R. Bowler. (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 galaxiesP. Hatfield, R. Bowler, M. Jarvis, и C. Hale. (2017)cite arxiv:1702.03309Comment: MNRAS submitted, 18 pages, 8 figures.Normal, Dust-Obscured Galaxies in the Epoch of ReionizationY. Fudamoto, P. Oesch, S. Schouws, M. Stefanon, R. Smit, R. Bouwens, R. Bowler, R. Endsley, V. Gonzalez, H. Inami и 19 other автор(ы). (2021)cite arxiv:2109.10378Comment: 16 pages, 7 figures, 4 tables, published in Nature.The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imagingC. Donnan, D. McLeod, J. Dunlop, R. McLure, A. Carnall, R. Begley, F. Cullen, M. Hamadouche, R. Bowler, H. McCracken и 3 other автор(ы). (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 ~ 4R. Bowler, N. Adams, M. Jarvis, и B. Häußler. (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 $-28<M_UV<-16$N. Adams, R. Bowler, M. Jarvis, R. Varadaraj, и B. Häußler. (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 FieldR. McLure, J. Dunlop, F. Cullen, N. Bourne, P. Best, S. Khochfar, R. Bowler, A. Biggs, J. Geach, D. Scott и 5 other автор(ы). (2017)cite arxiv:1709.06102Comment: 17 pages, 7 figures, submitted to MNRAS.

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