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Lyman Alpha Signatures from Direct Collapse Black Holes

, , and . (2016)cite arxiv:1602.07695Comment: 16 pages, 7 figures, submitted to ApJ following revision based on referee report.

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The growth of typical star-forming galaxies and their super massive black holes across cosmic time since z~2, , , , , , , and . (2016)cite arxiv:1609.03571Comment: 10 pages, 8 figures, accepted to MNRAS.On the nature of the luminous Lya emitter CR7 and its UV components: physical conditions and JWST predictions, , , , , , , , and . (2017)cite arxiv:1710.08422Comment: Submitted to MNRAS, comments welcomed. 19 pages, 11 figures.The colors and sizes of recently quenched galaxies: a result of compact starburst before quenching, , , , , , , , , and 4 other author(s). (2019)cite arxiv:1912.03683Comment: 16 pages, 8 figures, 1 table, accepted by ApJ.A $1.4$ deg$^2$ blind survey for CII, CIII and CIV at $z\sim0.7-1.5$. I: nature, morphologies and equivalent widths, , , , and . (2017)cite arxiv:1703.10169Comment: Submitted to MNRAS. Comments welcome! 17 pages, 12 figures, 8 tables.A large, multi-epoch H\alpha survey at z=2.23, 1.47, 0.84 & 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS, , , , , , , and . (2012)cite arxiv:1202.3436 Comment: 19 pages, 10 Figures, submitted to MNRAS.Star formation at z=1.47 from HiZELS: An H\alpha+OII double-blind study, , , , , and . (2011)cite arxiv:1109.1830 Comment: 20 pages, 21 figures, submitted to MNRAS.A relationship between specific star formation rate and metallicity gradient within z=1 galaxies from KMOS-HiZELS, , , , , , , , and . (2014)cite arxiv:1407.1047Comment: Accepted for publication in MNRAS.Identification of the brightest Ly\alpha\ emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era, , , , , and . (2015)cite arxiv:1502.07355Comment: 20 pages, main results shown in Fig. 6 and Fig. 7, submitted to MNRAS.A large narrow band H$\alpha$ survey at $z\sim0.2$: the bright end of the luminosity function, cosmic variance and clustering across cosmic time, and . (2015)cite arxiv:1507.02687Comment: Accepted for publication in MNRAS; 18 pages, 19 figures, 6 tables.The KMOS Redshift One Spectroscopic Survey (KROSS): The Tully-Fisher Relation at z ~ 1, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1604.06103Comment: Accepted for publication in MNRAS. 30 pages, 7 figures.