about
The Masses and Shapes of Dark Matter Halos from Galaxy‐Galaxy Lensing in the CFHT Legacy SurveyThe correlation between the sizes of globular cluster systems and their host dark matter haloesThe dependence of halo mass on galaxy size at fixed stellar mass using weak lensingChemical Mapping of the Milky Way with The Canada–France Imaging Survey: A Non-parametric Metallicity–Distance Decomposition of the GalaxyThe Canada–France Imaging Survey: First Results from the u-Band ComponentDynamical friction in the primordial neutrino seaThe weak-lensing masses of filaments between luminous red galaxiesLarge-scale structure: Going with the flowSatellite quenching time-scales in clusters from projected phase space measurements matched to simulated orbitsCosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density fieldCFHTLenS: weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignmentBeyond Sérsic + exponential disc morphologies in the Coma ClusterKinematic bias in cosmological distance measurement: Figure 1Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density fieldDark matter halos in galaxies and globular cluster populations. II. Metallicity and morphologyOn the perturbation of the luminosity distance by peculiar motionsCFHTLenS: a weak lensing shear analysis of the 3D-Matched-Filter galaxy clustersCFHTLenS: co-evolution of galaxies and their dark matter haloesThe phase space and stellar populations of cluster galaxies at z ~ 1: simultaneous constraints on the location and timescale of satellite quenchingDark matter halos in galaxies and globular cluster populationsDissecting the red sequence: the bulge and disc colours of early-type galaxies in the Coma clusterQuenching star formation in cluster galaxiesCFHTLenS: the relation between galaxy dark matter haloes and baryons from weak gravitational lensingCFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignmentsCFHTLenS tomographic weak lensing: quantifying accurate redshift distributionsDisentangling satellite galaxy populations using orbit tracking in simulationsCFHTLenS: combined probe cosmological model comparison using 2D weak gravitational lensingFirst measurement of the bulk flow of nearby galaxies using the cosmic microwave backgroundCFHTLenS: testing the laws of gravity with tomographic weak lensing and redshift-space distortionsProbing satellite haloes with weak gravitational lensingCFHTLenS: the Canada–France–Hawaii Telescope Lensing SurveyThe growth rate of cosmic structure from peculiar velocities at low and high redshiftsCosmic flows in the nearby universe from Type Ia supernovaeEnvironmental quenching and hierarchical cluster assembly: evidence from spectroscopic ages of red-sequence galaxies in ComaThe 2M++ galaxy redshift catalogueCosmic smoothnessThe HST/ACS Coma cluster survey. IV. Intergalactic globular clusters and the massive globular cluster system at the core of the Coma galaxy clusterGroup-finding with photometric redshifts: the photo-z probability peaks algorithmColours of bulges and discs within galaxy clusters and the signature of disc fading on infallThe HST/ACS Coma cluster survey. II. Data description and source catalogs
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description
researcher ORCID id 0000-0002-1437-3786
@en
wetenschapper
@nl
name
Michael J. Hudson
@ast
Michael J. Hudson
@en
Michael J. Hudson
@es
Michael J. Hudson
@nl
type
label
Michael J. Hudson
@ast
Michael J. Hudson
@en
Michael J. Hudson
@es
Michael J. Hudson
@nl
altLabel
Mike
@en
prefLabel
Michael J. Hudson
@ast
Michael J. Hudson
@en
Michael J. Hudson
@es
Michael J. Hudson
@nl
P1053
H-3238-2012
P106
P31
P3829
P3835
mike-hudson
P496
0000-0002-1437-3786