Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey
A&A, 457 3 (2006) 841-856
Published online: 2006-09-12
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The dust mass function from z ∼0 to z ∼2.5
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PS1-STRM: neural network source classification and photometric redshift catalogue for PS1 3π DR1
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A New Census of the 0.2 < z < 3.0 Universe. I. The Stellar Mass Function
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Photometric redshifts for galaxies in the Subaru Hyper Suprime-Cam and unWISE and a catalogue of identified clusters of galaxies
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Building the Largest Spectroscopic Sample of Ultracompact Massive Galaxies with the Kilo Degree Survey
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A3COSMOS: the dust attenuation of star-forming galaxies at z = 2.5–4.0 from the COSMOS-ALMA archive
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The Role of Environment in Galaxy Evolution in the SERVS Survey. I. Density Maps and Cluster Candidates
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Quiescent Galaxies 1.5 Billion Years after the Big Bang and Their Progenitors
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Discovery of Two Einstein Crosses from Massive Post-blue Nugget Galaxies at z > 1 in KiDS*
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Photometric Redshift Estimation with Galaxy Morphology Using Self-organizing Maps
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Star Formation in Massive Galaxies at Redshift z ∼ 0.5
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Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
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A systematic search for galaxy proto-cluster cores at z ∼ 2
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The XXL Survey
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Type IIn supernova light-curve properties measured from an untargeted survey sample
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Tests of Catastrophic Outlier Prediction in Empirical Photometric Redshift Estimation with Redshift Probability Distributions
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Coevolution of black hole accretion and star formation in galaxies up to z = 3.5
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Thermal Regulation and the Star-forming Main Sequence
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Structural analysis of massive galaxies using HST deep imaging at z < 0.5
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AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
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Simulating JWST deep extragalactic imaging surveys and physical parameter recovery
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The Next Generation Virgo Cluster Survey (NGVS). XIV. The Discovery of Low-mass Galaxies and a New Galaxy Catalog in the Core of the Virgo Cluster∗
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CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters
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