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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2018, Volume 474, Issue 4, pp. 4648 - 4659
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622
Aims. We wish to determine the distribution of dark matter halo masses as a function of the stellar mass and the stellar mass profile for massive galaxies in... 
Galactic halos | Galaxies | Galactic evolution | Stars & galaxies | Sky surveys (astronomy) | Stellar evolution | Halos | Stellar mass | Dark matter | Morphology | Astronomical models | Dependence | Stellar oscillations | Sampling methods | Galaxy distribution | Bayesian analysis | Photometry
Journal Article
Astrophysical Journal, ISSN 0004-637X, 05/2014, Volume 786, Issue 2, pp. 1 - 8
Several studies have suggested that the observed size evolution of massive early-type galaxies (ETGs) can be explained as a combination of dry mergers and... 
galaxies: elliptical and lenticular, cD | galaxies: evolution | Acquisitions | Slopes | Galactic evolution | Dissipation | Constants | Mathematical models | Density | Drying | Physics - Cosmology and Nongalactic Astrophysics | DENSITY | RED SHIFT | EVOLUTION | NONLUMINOUS MATTER | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | APPROXIMATIONS | MASS | STARS | GALAXIES | SIMULATION | LENSES
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2018, Volume 477, Issue 4, pp. 5460 - 5476
We present a Bayesian hierarchical inference formalism to study the relation between the properties of dark matter haloes and those of their central galaxies... 
Dark matter | Methods: statistical | Gravitational lensing: weak | FIELD | DARK-MATTER HALOES | ENVIRONMENT | MAPPING STELLAR CONTENT | gravitational lensing: weak | DEPENDENCE | methods: statistical | PROFILE | CLUSTERS | ASTRONOMY & ASTROPHYSICS | MASS | SDSS | REDSHIFT | dark matter | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 465, Issue 2, p. 2397
  The stellar initial mass function (IMF) of early-type galaxies is the combination of the IMF of the stellar population formed in situ and that of accreted... 
Correlation analysis | Cosmology | Star & galaxy formation | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 465, Issue 2, pp. 2397 - 2397
The stellar initial mass function (IMF) of early-type galaxies is the combination of the IMF of the stellar population formed in situ and that of accreted... 
Acquisitions | Correlation | Galaxies | Stellar mass | Galactic evolution | Mathematical models | Dispersion | Drying
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622, p. A30
Aims. We wish to determine the distribution of dark matter halo masses as a function of the stellar mass and the stellar mass profile for massive galaxies in... 
Galaxies: fundamental parameters | Galaxies: elliptical and lenticular | Gravitational lensing: weak | MATTER | PROJECT | galaxies: fundamental parameters | DARK | gravitational lensing: weak | galaxies: elliptical and lenticular, cD | WEAK | ENVIRONMENTAL DEPENDENCE | EVOLUTION | ASTRONOMY & ASTROPHYSICS | SDSS | QUIESCENT GALAXIES | CONSTRAINTS | MERGERS
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 04/2014, Volume 786, Issue 2, p. 89
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 08/2017, Volume 469, Issue 2, pp. 1824 - 1848
Early-type galaxies provide unique tests for the predictions of the cold dark matter cosmology and the baryonic physics assumptions entering models for galaxy... 
ELLIPTIC GALAXIES | 2-DIMENSIONAL KINEMATICS | cosmology: theory | galaxies: structure | SCALING RELATIONS | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | gravitational lensing: strong | DARK-MATTER FRACTIONS | INITIAL MASS FUNCTION | FUNDAMENTAL PLANE | STELLAR MASS | dark matter | galaxies: haloes | LENS ACS SURVEY | DENSITY PROFILE
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2019, Volume 483, Issue 4, pp. 4615 - 4627
Journal Article