most citedThe dust budget crisis in high-redshift submillimetre galaxies

119 citations · 355 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

Under Pressure: UV Emission Line Ratios as Barometers of AGN Feedback Mechanisms

Elise Fuller, Sean D. Johnson, Jonathan Stern +16

Feedback from active galactic nuclei (AGN) is widely acknowledged to regulate the growth of massive galaxies, though its driving mechanisms are debated. Prevailing theories suggest…

astro-ph.GA2014★ 103 cited

The evolution of the cold interstellar medium in galaxies following a starburst

K. Rowlands, V. Wild, N. Nesvadba +4

We present the evolution of dust and molecular gas properties in a sample of 11 starburst to post-starburst (PSB) galaxies selected to span an age sequence from ongoing…

astro-ph.GA2014★ 16 cited

Colour matters: the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel-ATLAS

N. Bourne, S. J. Maddox, L. Dunne +9

We report an unexpected variation in the positional offset distributions between Herschel-ATLAS sub-millimetre (submm) sources and their optical associations, depending on both 250…

astro-ph.GA2014★ 45 cited

Herschel-ATLAS and ALMA: HATLAS J142935.3-002836, a lensed major merger at redshift 1.027

Hugo Messias, Simon Dye, Neil Nagar +29

[Abridged] Aims: This work focuses on one lensed system, HATLAS J142935.3-002836 (H1429-0028), selected in the Herschel-ATLAS field. Gathering a rich, multi-wavelength dataset, we…

astro-ph.GA2014★ 119 cited

The dust budget crisis in high-redshift submillimetre galaxies

K. Rowlands, H. L. Gomez, L. Dunne +5

We apply a chemical evolution model to investigate the sources and evolution of dust in a sample of 26 high-redshift () submillimetre galaxies (SMGs) from the literature, with…

astro-ph.GA2014★ 72 cited

Herschel-ATLAS: Properties of dusty massive galaxies at low and high redshifts

K. Rowlands, L. Dunne, S. Dye +16

We present a comparison of the physical properties of a rest-frame m selected sample of massive, dusty galaxies from . Our sample comprises 29 high-redshift submilli…