David Sobral
home.strw.leidenuniv.nl
0000-0001-8823-4845
Lancaster University
134 papers found
Refreshing results…
The brightest Ly α emitter: Pop III or black hole?
A large narrow-band Hα survey at z∼ 0.2: the bright end of the luminosity function, cosmic variance and clustering across cosmic time
Evolution of the H β + [O iii] and [O ii] luminosity functions and the [O ii] star formation history of the Universe up toz ∼ 5 from HiZELS
EVIDENCE FOR PopIII-LIKE STELLAR POPULATIONS IN THE MOST LUMINOUS LyαEMITTERS AT THE EPOCH OF REIONIZATION: SPECTROSCOPIC CONFIRMATION
Neutral hydrogen gas, past and future star formation in galaxies in and around the ‘Sausage’ merging galaxy cluster
On the nature of Hα emitters atz∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence
CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O iii] + Hβ and [O ii] luminosity functions at z = 0.8, 1.4 and 2.2
Mc2: Galaxy Imaging and Redshift Analysis of the Merging Cluster Ciza J2242.8+5301
Identification of the brightest Lyα emitters at z = 6.6: implications for the evolution of the luminosity function in the reionization era
A COMPARATIVE STUDY OF DENSITY FIELD ESTIMATION FOR GALAXIES: NEW INSIGHTS INTO THE EVOLUTION OF GALAXIES WITH ENVIRONMENT IN COSMOS OUT TOz∼ 3
MC2: boosted AGN and star formation activity in CIZA J2242.8+5301, a massive post-merger cluster at z = 0.19★
The rise and fall of star formation in z ∼ 0.2 merging galaxy clusters
Mc2: Constraining the Dark Matter Distribution of the Violent Merging Galaxy Cluster Ciza J2242.8+5301 by Piercing Through the Milky Way
COSMIC WEB AND STAR FORMATION ACTIVITY IN GALAXIES ATz∼ 1
A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS
MOONS: the Multi-Object Optical and Near-infrared Spectrograph for the VLT
Spectral and morphological signatures of cluster merger shocks
The highest frequency detection of a radio relic: 16 GHz AMI observations of the ‘Sausage’ cluster
A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: strong constraints on the luminosity function and implications for other surveys★
Mapping the large-scale structure around a z = 1.46 galaxy cluster in 3D using two adjacent narrow-band filters
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