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Disambiguierung von "Best, Philip N."

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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

, , , , , , , und . (2012)cite arxiv:1202.3436 Comment: 19 pages, 10 Figures, submitted to MNRAS.

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Weitere Publikationen von Autoren mit dem selben Namen

The stellar mass function of star-forming galaxies and the mass-dependent SFR function since z=2.23 from HiZELS, , , , , und . (2013)cite arxiv:1311.1503Comment: Accepted for publication in MNRAS, 14 pages, 9 figures.A fundamental metallicity relation for galaxies at z = 0.84 - 1.47 from HiZELS, , , , , , , , und . (2013)cite arxiv:1309.0506Comment: Accepted for publication in MNRAS.A relationship between specific star formation rate and metallicity gradient within z=1 galaxies from KMOS-HiZELS, , , , , , , , und . (2014)cite arxiv:1407.1047Comment: Accepted for publication in MNRAS.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, , , , , , , und . (2012)cite arxiv:1202.3436 Comment: 19 pages, 10 Figures, submitted to MNRAS.Radio source-component association for the LOFAR Two-metre Sky Survey with region-based convolutional neural networks, , , , , , , und . (2022)cite arxiv:2209.14226Comment: 22 pages; accepted for publication in A&A.CF-HiZELS, a 10 deg$^2$ emission-line survey with spectroscopic follow-up: H\alpha, OIII+H\beta\ and OII luminosity functions at z=0.8, 1.4 and 2.2, , , , , , , , , und 1 andere Autor(en). (2015)cite arxiv:1502.06602Comment: 22 pages, 15 figures, submitted to MNRAS.The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS, , , , , , , , und . (2013)cite arxiv:1310.3822Comment: Accepted for publication in ApJ. 8 pages, 3 figures.Evolution of the H$\beta$+OIII and OII luminosity functions and the OII star-formation history of the Universe up to $z$ ~ 5 from HiZELS, , , , , , , und . (2015)cite arxiv:1503.00004Comment: 23 pages, 14 figures, 7 Tables, submitted to MNRAS.The interstellar medium in OIII-selected star-forming galaxies at $z\sim3.2$, , , , , , , , , und 4 andere Autor(en). (2017)cite arxiv:1709.06731Comment: 20 pages, 11 figures, Accepted for publication in ApJ.The clustering of H$\beta$+OIII and OII emitters since $z 5$: dependencies with line luminosity and stellar mass, , , , , , , , , und . (2017)cite arxiv:1705.01101Comment: 19 pages, 11 figures, 4 tables, submitted to MNRAS.