800 citations · 17.1k across the 210 of their papers we have counts for
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The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2
B. Magnelli, R. J. Ivison, D. Lutz +21
[Abridged] We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate-stellar masse (i.e. SFR-M*) plane up to z 2. W…
Detailed modelling of a large sample of Herschel sources in the Lockman Hole: identification of cold dust and of lensing candidates through their anomalous SEDs
Michael Rowan-Robinson, Lingyu Wang, Julie Wardlow +12
We have studied in detail a sample of 967 SPIRE sources with 5-sigma detections at 350 and 500 micron and associations with Spitzer-SWIRE 24 micron galaxies in the HerMES-Lockman s…
The temperature dependence of the far-infrared-radio correlation in the Herschel-ATLAS
D. J. B. Smith, M. J. Jarvis, M. J. Hardcastle +12
We use 10,387 galaxies from the Herschel Astrophysical TeraHertz Large Area Survey (H-ATLAS) to probe the far-infrared radio correlation (FIRC) of star forming galaxies as a functi…
The SCUBA-2 Cosmology Legacy Survey: the submillimetre properties of Lyman break galaxies at z=3-5
K. E. K. Coppin, J. E. Geach, O. Almaini +28
We present statistically significant detections at 850um of the Lyman Break Galaxy (LBG) population at z=3, 4, and 5 using data from the Submillimetre Common User Bolometer Array 2…
Linking the X-ray and infrared properties of star-forming galaxies at z<1.5
M. Symeonidis, A. Georgakakis, M. J. Page +16
We present the most complete study to date of the X-ray emission from star-formation in high redshift (median z=0.7; z<1.5), IR-luminous (L_IR=10^10-10^13 L_sun) galaxies detected…
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…