2.7k citations · 19.2k across the 178 of their papers we have counts for
13 papers · 2 filters
SINFONI-HiZELS: The dynamics, merger rates & metallicity gradients of `typical' star-forming galaxies at = 0.8-2.2
J. Molina, E. Ibar, A. M. Swinbank +5
We present adaptive optics (AO) assisted SINFONI integral field unit (IFU) spectroscopy of eleven H emitting galaxies selected from the High-Z Emission Line Survey (HiZELS). We…
The growth of typical star-forming galaxies and their super massive black holes across cosmic time since z~2
João Calhau, David Sobral, Andra Stroe +5
Understanding galaxy formation and evolution requires studying the interplay between the growth of galaxies and the growth of their black holes across cosmic time. Here we explore…
The Lockman Hole project: LOFAR observations and spectral index properties of low-frequency radio sources
E. K. Mahony, R. Morganti, I. Prandoni +21
The Lockman Hole is a well-studied extragalactic field with extensive multi-band ancillary data covering a wide range in frequency, essential for characterising the physical and ev…
The CALYMHA survey: Lya luminosity function and global escape fraction of Lya photons at z=2.23
David Sobral, Jorryt Matthee, Philip Best +6
We present the CAlibrating LYMan- with H (CALYMHA) pilot survey and new results on Lyman- (Lya) selected galaxies at z~2. We use a custom-built Lya narrow-band filter at t…
[OIII] emission line as a tracer of star-forming galaxies at high redshifts: Comparison between H and [OIII] emitters at =2.23 in HiZELS
T. L. Suzuki, T. Kodama, D. Sobral +10
We investigate the properties of =2.23 H and [OIII]5007 emitters using the narrow-band-selected samples obtained from the High- Emission Line Survey (HiZELS: Sobral et…
LOFAR/H-ATLAS: A deep low-frequency survey of the Herschel-ATLAS North Galactic Pole field
M. J. Hardcastle, G. Gürkan, R. J. van Weeren +25
We present LOFAR High-Band Array (HBA) observations of the Herschel-ATLAS North Galactic Pole survey area. The survey we have carried out, consisting of four pointings covering aro…
A deep ALMA image of the Hubble Ultra Deep Field
J. S. Dunlop, R. J. McLure, A. D. Biggs +33
We present the results of the first, deep ALMA imaging covering the full 4.5 sq arcmin of the Hubble Ultra Deep Field (HUDF) as previously imaged with WFC3/IR on HST. Using a mosai…
The production and escape of Lyman-Continuum radiation from star-forming galaxies at z~2 and their redshift evolution
Jorryt Matthee, David Sobral, Philip Best +4
We study the production rate of ionizing photons of a sample of 588 H emitters (HAEs) and 160 Lyman- emitters (LAEs) at in the COSMOS field in order to assess the imp…
The KMOS Redshift One Spectroscopic Survey (KROSS): The Tully-Fisher Relation at z ~ 1
Alfred L. Tiley, John P. Stott, A. M. Swinbank +11
We present the stellar mass (), and K-corrected -band absolute magnitude () Tully-Fisher relations (TFRs) for sub-samples of the 584 galaxies spatially resolved in…
FR II radio galaxies at low frequencies I: morphology, magnetic field strength and energetics
Jeremy J. Harwood, Judith H. Croston, Huib T. Intema +14
Due to their steep spectra, low-frequency observations of FR II radio galaxies potentially provide key insights in to the morphology, energetics and spectrum of these powerful radi…
The CALYMHA survey: Ly escape fraction and its dependence on galaxy properties at
Jorryt Matthee, David Sobral, Ivàn Oteo +4
We present the first results from our CAlibrating LYMan- with H (CALYMHA) pilot survey at the Isaac Newton Telescope. We measure Ly emission for 488 H selected galaxies…
The KMOS Redshift One Spectroscopic Survey (KROSS): Dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies
John P. Stott, A. M. Swinbank, Helen L. Johnson +12
The KMOS Redshift One Spectroscopic Survey (KROSS) is an ESO guaranteed time survey of 795 typical star-forming galaxies in the redshift range z=0.8-1.0 with the KMOS instrument on…
The most luminous H emitters at z~0.8-2.23 from HiZELS: evolution of AGN and star-forming galaxies
David Sobral, Saul A. Kohn, Philip N. Best +5
We use new near-infrared spectroscopic observations to investigate the nature and evolution of the most luminous Hα(Ha) emitters at z~0.8-2.23, which evolve strongly in number dens…