Browsing by Author "Jarvis, M. J."
Now showing items 1-7 of 7
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Comparing galaxy clustering in horizon-agn simulated light-cone mocks and video observations
Hatfield, P. W.; Laigle, C.; Jarvis, M. J. (Oxford University Press, 2019-04-12)Hydrodynamical cosmological simulations have recently made great advances in reproducing galaxy mass assembly over cosmic time – as often quantified from the comparison of their predicted stellar mass functions to observed ... -
Deep extragalactic visible legacy survey (DEVILS):Evolution of the σsFR-M relation and implications for self-regulated star formation
Jarvis, M. J.; Davies, L. J. M.; Thorne, J.E (University of the Western Cape, 2022)We present the evolution of the star formation dispersion–stellar mass relation ( σSFR –M ) in the DEVILS D10 region using new measurements derived using the PROSPECT spectral energy distribution fitting code. We find ... -
The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): Overview and survey description
Jarvis, M. J.; Muxlow, T. W. B.; Thomson, A. P. (Oxford University Press, 2020)We present an overview and description of the e-MERGE Survey (e-MERLIN Galaxy Evolution Survey) Data Release 1 (DR1), a large program of high-resolution 1.5-GHz radio observations of the GOODS-N field comprising ∼140 h of ... -
The faint radio source population at 15.7 GHz – IV. The dominance of core emission in faint radio galaxies
Whittam, I. H.; Green, D. A.; Jarvis, M. J. (Oxford University Press, 2020)We present 15-GHz Karl G. Jansky Very Large Array observations of a complete sample of radio galaxies selected at 15.7 GHz from the Tenth Cambridge (10C) survey. 67 out of the 95 sources (71 per cent) are unresolved in the ... -
A lack of evolution in the very bright end of the galaxy luminosity function from z 8 to 10
Dunlop, J. S.; Bowler, R. A. A.; Jarvis, M. J. (Oxford University Press, 2020)ABSTRACT We utilize deep near-infrared survey data from the UltraVISTA fourth data release (DR4) and the VIDEO survey, in combination with overlapping optical and Spitzer data, to search for bright star-forming galaxies ... -
The rest-frame UV luminosity function at z 4: A significant contribution of AGNs to the bright end of the galaxy population
Jarvis, M. J.; Adams, N. J.; Bowler, R. A. A. (Oxford University Press, 2020)We measure the rest-frame ultraviolet (UV) luminosity function (LF) at z ∼ 4 self-consistently over a wide range in absolute magnitude (−27 ≲ MUV ≲ −20). The LF is measured with 46 904 sources selected using a photometric ... -
The VANDELS survey: a strong correlation between Ly α equivalent width and stellar metallicity at 3 ≤ z ≤ 5
Jarvis, M. J.; Cullen, F.; McLure, R. J. (Oxford University Press, 2020)We present the results of a new study investigating the relationship between observed Ly α equivalent width (Wλ(Ly α)) and the metallicity of the ionizing stellar population ( Z⋆) for a sample of 768 star-forming galaxies ...