Leiden University Scholarly Publications

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(1 - 20 of 21)

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An ALMA survey of the S2CLS UDS field
Cosmic evolution of the H2 mass density and the epoch of molecular gas
The VANDELS ESO public spectroscopic survey
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies
An ALMA survey of the SCUBA-2 cosmology legacy survey UKIDSS/UDS field: dust attenuation in high-redshift Lyman-break galaxies
An ALMA survey of the SCUBA-2 cosmology legacy survey UKIDSS/UDS field: the far-infrared/radio correlation for high-redshift dusty star-forming galaxies
Radio Spectra and Sizes of Atacama Large Millimeter/submillimeter Array-identified Submillimeter Galaxies: Evidence of Age-related Spectral Curvature and Cosmic-Ray Diffusion?
Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Number Counts of Submillimeter Galaxies
An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Identifying Candidate z 4.5 [C II] Emitters
The VANDELS ESO public spectroscopic survey: Observations and first data release
A direct calibration of the IRX-β relation in Lyman-break Galaxies at z = 3-5
A Machine-learning Method for Identifying Multiwavelength Counterparts of Submillimeter Galaxies: Training and Testing Using AS2UDS and ALESS
The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS
The SCUBA-2 Cosmology Legacy Survey: the clustering of submillimetre galaxies in the UKIDSS UDS field
A consistent measure of the merger histories of massive galaxies using close-pair statistics - I. Major mergers at z < 3.5
The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts
CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ~ 2
The SCUBA-2 Cosmology Legacy Survey: Multiwavelength Counterparts to 10^3 Submillimeter Galaxies in the UKIDSS-UDS Field
The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation

Pages