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The bivariate gas–stellar mass distributions and the mass functions of early- and late-type galaxies at
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A substantial population of low-mass stars in luminous elliptical galaxies
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Galaxy merging, the fundamental plane of elliptical galaxies and the MBH -- 0 relation
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On the survival of metallicity gradients to major dry-mergers
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The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1
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Resolving galaxies in time and space: II. Uncertainties in the spectral synthesis of datacubes
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A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA
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Mapping a stellar disk into a boxy bulge: The outside-in part of the Milky Way bulge formation
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Why the Milky Way’s bulge is not only a bar formed from a cold thin disk
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The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies⋆
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Star formation along the Hubble sequence: Radial structure of the star formation of CALIFA galaxies
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Size evolution of star-forming galaxies with 2 < z < 4.5 in the VIMOS Ultra-Deep Survey
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The VIMOS Public Extragalactic Redshift Survey (VIPERS): The distinct build-up of dense and normal massive passive galaxies⋆
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The spatially resolved star formation history of CALIFA galaxies: Cosmic time scales
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Cosmic evolution of the spatially resolved star formation rate and stellar mass of the CALIFA survey
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Color gradients reflect an inside-out growth in early-type galaxies of the cluster MACS J1206.2-0847
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September 2018 |
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Uncertainties in gas kinematics arising from stellar continuum modeling in integral field spectroscopy data: the case of NGC 2906 observed with VLT/MUSE
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May 2019 |
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SDSS-IV MaNGA: Global and local stellar population properties of elliptical galaxies
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December 2020 |
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Evidence for radially independent size growth of early-type galaxies in clusters
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August 2020 |
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Evolution of UV–NIR structural properties of cluster galaxies
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June 2002 |
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July 2003 |
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New York University Value-Added Galaxy Catalog: A Galaxy Catalog Based on New Public Surveys
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June 2005 |
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Passively Evolving Early‐Type Galaxies at 1.4 ≲ z ≲ 2.5 in the Hubble Ultra Deep Field
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The Size Evolution of Galaxies since z ∼3: Combining SDSS, GEMS, and FIRES
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Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse
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Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks
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The Dramatic Size Evolution of Elliptical Galaxies and the Quasar Feedback
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The Manga Integral Field unit Fiber feed System for the Sloan 2.5 m Telescope
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OBSERVING STRATEGY FOR THE SDSS-IV/MaNGA IFU GALAXY SURVEY
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RED NUGGETS AT z ∼ 1.5: COMPACT PASSIVE GALAXIES AND THE FORMATION OF THE KORMENDY RELATION
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The Relation Between Compact, Quiescent High-Redshift Galaxies and Massive Nearby Elliptical Galaxies: Evidence for Hierarchical, Inside-Out Growth
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THE GREATER IMPACT OF MERGERS ON THE GROWTH OF MASSIVE GALAXIES: IMPLICATIONS FOR MASS ASSEMBLY AND EVOLUTION SINCE z ≃ 1
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May 2009 |
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On the size and Comoving mass Density Evolution of Early-Type Galaxies
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Minor Mergers and the size Evolution of Elliptical Galaxies
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June 2009 |
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THE ORIGIN OF COLOR GRADIENTS IN EARLY-TYPE SYSTEMS AND THEIR COMPACTNESS AT HIGH- z
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THE GROWTH OF MASSIVE GALAXIES SINCE z = 2
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The two Phases of Galaxy Formation
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Can Minor Merging Account for the size Growth of Quiescent Galaxies? new Results from the Candels Survey
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THE STRUCTURES AND TOTAL (MINOR + MAJOR) MERGER HISTORIES OF MASSIVE GALAXIES UP TO z ∼ 3 IN THE HST GOODS NICMOS SURVEY: A POSSIBLE SOLUTION TO THE SIZE EVOLUTION PROBLEM
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Forming Early-Type Galaxies in Λcdm Simulations. i. Assembly Histories
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July 2012 |
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CANDELS: THE PROGENITORS OF COMPACT QUIESCENT GALAXIES AT z ∼ 2
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February 2013 |
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HST /WFC3 CONFIRMATION OF THE INSIDE-OUT GROWTH OF MASSIVE GALAXIES AT 0 < z < 2 AND IDENTIFICATION OF THEIR STAR-FORMING PROGENITORS AT z ∼ 3
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March 2013 |
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Newly Quenched Galaxies as the Cause for the Apparent Evolution in Average size of the Population
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CONSTRAINING THE ASSEMBLY OF NORMAL AND COMPACT PASSIVELY EVOLVING GALAXIES FROM REDSHIFT z = 3 TO THE PRESENT WITH CANDELS
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ON THE ROBUSTNESS OF z = 0-1 GALAXY SIZE MEASUREMENTS THROUGH MODEL AND NON-PARAMETRIC FITS
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The Evolution of the Number Density of Compact Galaxies
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PURELY DRY MERGERS DO NOT EXPLAIN THE OBSERVED EVOLUTION OF MASSIVE EARLY-TYPE GALAXIES SINCE z ∼ 1
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BULGE GROWTH AND QUENCHING SINCE z = 2.5 IN CANDELS/3D-HST
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3D-HST+CANDELS: THE EVOLUTION OF THE GALAXY SIZE-MASS DISTRIBUTION SINCE z = 3
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May 2014 |
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Central Galaxies in Different Environments: do they have Similar Properties?
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May 2014 |
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OVERVIEW OF THE SDSS-IV MaNGA SURVEY: MAPPING NEARBY GALAXIES AT APACHE POINT OBSERVATORY
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December 2014 |
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STELLAR POPULATIONS FROM SPECTROSCOPY OF A LARGE SAMPLE OF QUIESCENT GALAXIES AT Z > 1: MEASURING THE CONTRIBUTION OF PROGENITOR BIAS TO EARLY SIZE GROWTH
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January 2015 |
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AVOIDING PROGENITOR BIAS: THE STRUCTURAL AND MASS EVOLUTION OF BRIGHTEST GROUP AND CLUSTER GALAXIES IN HIERARCHICAL MODELS SINCE z ≲ 1
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March 2015 |
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Forming Compact Massive Galaxies
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October 2015 |
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THE MORPHOLOGY OF PASSIVELY EVOLVING GALAXIES AT z ∼ 2 FROM HUBBLE SPACE TELESCOPE /WFC3 DEEP IMAGING IN THE HUBBLE ULTRA DEEP FIELD
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April 2010 |
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RED NUGGETS AT HIGH REDSHIFT: STRUCTURAL EVOLUTION OF QUIESCENT GALAXIES OVER 10 Gyr OF COSMIC HISTORY
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The Fundamental Plane in CL 0024 at z = 0.4: implications for the evolution of the mass-to-light ratio
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SDSS-IV MaNGA: Excavating the fossil record of stellar populations in spiral galaxies
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January 2020 |
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Galaxy properties as revealed by MaNGA – III. Kinematic profiles and stellar population gradients in S0s
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May 2020 |
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Stellar velocity dispersion and initial mass function gradients in dissipationless galaxy mergers
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September 2020 |
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The evolution of compact massive quiescent and star-forming galaxies derived from the R e– R h and M star– M h relations
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May 2021 |
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SDSS-IV DR17: final release of MaNGA PyMorph photometric and deep-learning morphological catalogues
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October 2021 |
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Size evolution of spheroids in a hierarchical Universe
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October 2012 |
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How do minor mergers promote inside-out growth of ellipticals, transforming the size, density profile and dark matter fraction?
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The stellar IMF in early-type galaxies from a non-degenerate set of optical line indices
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December 2013 |
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Wet disc contraction to galactic blue nuggets and quenching to red nuggets
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December 2013 |
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SPIDER VIII – constraints on the stellar initial mass function of early-type galaxies from a variety of spectral features
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June 2013 |
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Galaxy And Mass Assembly (GAMA): mass–size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphology
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January 2015 |
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Radial variations in the stellar initial mass function of early-type galaxies
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The green valley is a red herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early- and late-type galaxies★
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March 2014 |
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Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5
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Galaxy And Mass Assembly (GAMA): the wavelength-dependent sizes and profiles of galaxies revealed by MegaMorph
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A new population of recently quenched elliptical galaxies in the SDSS
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June 2014 |
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Galaxy Zoo: evidence for diverse star formation histories through the green valley
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April 2015 |
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Galaxy And Mass Assembly (GAMA): the wavelength dependence of galaxy structure versus redshift and luminosity
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September 2015 |
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The diverse evolutionary paths of simulated high- z massive, compact galaxies to z = 0
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December 2015 |
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P-MaNGA: full spectral fitting and stellar population maps from prototype observations
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March 2015 |
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Compaction and quenching of high-z galaxies in cosmological simulations: blue and red nuggets
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May 2015 |
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The fate of high-redshift massive compact galaxies
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SDSS IV MaNGA: the global and local stellar mass assemby histories of galaxies
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Radial gradients in initial mass function sensitive absorption features in the Coma brightest cluster galaxies
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October 2016 |
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Size evolution of normal and compact galaxies in the EAGLE simulation
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Evolution of density profiles in high- z galaxies: compaction and quenching inside-out
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SDSS-IV MaNGA: Spatially resolved star formation histories in galaxies as a function of galaxy mass and type
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The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
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Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 at z = 1.39
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Colour gradients in cluster ellipticals at z ∼ 1.4: the hidden content of the galaxy central regions
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Constraining the galaxy–halo connection over the last 13.3 Gyr: star formation histories, galaxy mergers and structural properties
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The size evolution of star-forming and quenched galaxies in the IllustrisTNG simulation
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November 2017 |
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Dynamical masses and non-homology of massive elliptical galaxies grown by dry mergers
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April 2017 |
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Galaxy Zoo: the interplay of quenching mechanisms in the group environment★
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April 2017 |
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MUSE observations of M87: radial gradients for the stellar initial-mass function and the abundance of sodium
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May 2018 |
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KINETyS II: Constraints on spatial variations of the stellar initial mass function from K-band spectroscopy
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May 2018 |
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The stellar population and initial mass function of NGC 1399 with MUSE
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June 2018 |
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The SELGIFS data challenge: generating synthetic observationsof CALIFA galaxies from hydrodynamical simulations
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June 2018 |
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Evolution of galaxy size–stellar mass relation from the Kilo-Degree Survey
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July 2018 |
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Inferring the star formation histories of massive quiescent galaxies with bagpipes: evidence for multiple quenching mechanisms
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August 2018 |
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SDSS-IV MaNGA – an archaeological view of the cosmic star formation history
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October 2018 |
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SDSS-IV MaNGA PyMorph Photometric and Deep Learning Morphological Catalogues and implications for bulge properties and stellar angular momentum
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November 2018 |
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Optical integral field spectroscopy observations applied to simulated galaxies: testing the fossil record method
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November 2018 |
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SDSS-IV MaNGA: local and global chemical abundance patterns in early-type galaxies
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December 2018 |
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A galaxy classification grid that better recognises early-type galaxy morphology
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June 2019 |
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SDSS-IV MaNGA: effects of morphology in the global and local star formation main sequences
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July 2019 |
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IMF radial gradients in most massive early-type galaxies
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August 2019 |
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Galaxy properties as revealed by MaNGA – I. Constraints on IMF and M*/L gradients in ellipticals
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September 2019 |
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SDSS-IV MaNGA: stellar initial mass function variation inferred from Bayesian analysis of the integral field spectroscopy of early-type galaxies
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March 2019 |
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SDSS-IV MaNGA: when is morphology imprinted on galaxies?
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January 2020 |
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Evolutionary stellar population synthesis at high spectral resolution: optical wavelengths
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March 2005 |
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Strong size evolution of the most massive galaxies since z ∼ 2
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The size evolution of galaxy discs formed within Λ cold dark matter haloes
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The origin of the light distribution in spiral galaxies
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Evolutionary stellar population synthesis with MILES - I. The base models and a new line index system
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SPIDER - I. Sample and galaxy parameters in the grizYJHK wavebands: SPIDER - I. Sample and data analysis
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SPIDER - II. The Fundamental Plane of early-type galaxies in grizYJHK: SPIDER - II. The FP in grizYJHK
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Dissecting the size evolution of elliptical galaxies since z∼ 1: puffing-up versus minor-merging scenarios: Dissecting the size evolution of the ellipticals
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Size and velocity-dispersion evolution of early-type galaxies in a Λ cold dark matter universe: Evolution of early-type galaxies
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Spatially Resolved Spectroscopic Properties of Low-Redshift Star-Forming Galaxies
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Modeling the Panchromatic Spectral Energy Distributions of Galaxies
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THE DATA REDUCTION PIPELINE FOR THE SDSS-IV MaNGA IFU GALAXY SURVEY
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Zens. iv. Similar Morphological Changes Associated with mass Quenching and Environment Quenching and the Relative Importance of Bulge Growth Versus the Fading of Disks
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RESOLVING THE DISCREPANCY OF GALAXY MERGER FRACTION MEASUREMENTS AT z ∼ 0–3
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Minor Mergers or Progenitor Bias? the Stellar ages of Small and Large Quenched Galaxies
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The Evolution of star Formation Histories of Quiescent Galaxies
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The SDSS-IV MaNGA Sample: Design, Optimization, and Usage Considerations
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Overview of the DESI Legacy Imaging Surveys
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Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2
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The Mass, Color, and Structural Evolution of Today’s Massive Galaxies Since z ∼ 5
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Constraints on Quenching of Z ≲ 2 Massive Galaxies from the Evolution of the Average Sizes of Star-forming and Quenched Populations in COSMOS
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April 2017 |
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Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and Quiescent Galaxies
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May 2017 |
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Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
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May 2017 |
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The Stellar Initial Mass Function in Early-type Galaxies from Absorption Line Spectroscopy. III. Radial Gradients
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May 2017 |
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The Global and Radial Stellar Mass Assembly of Milky Way-sized Galaxies
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The KMOS Cluster Survey (KCS). II. The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift 1.39 < z < 1.61
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Half-mass Radii for ∼7000 Galaxies at 1.0 ≤ z ≤ 2.5: Most of the Evolution in the Mass–Size Relation Is Due to Color Gradients
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May 2019 |
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Unbiased Differential Size Evolution and the Inside-out Growth of Galaxies in the Deep CANDELS GOODS Fields at 1 ≤ z ≤ 7
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Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies
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Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy Size−Mass Relation at z < 1
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Stellar Population and Elemental Abundance Gradients of Early-type Galaxies*
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The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library
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Spatially Resolved star Formation main Sequence of Galaxies in the Califa Survey
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A Mass-dependent Slope of the Galaxy Size–Mass Relation out to z ∼ 3: Further Evidence for a Direct Relation between Median Galaxy Size and Median Halo Mass
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Half-mass Radii of Quiescent and Star-forming Galaxies Evolve Slowly from 0 ≲ z ≤ 2.5: Implications for Galaxy Assembly Histories
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Optical-Near Infrared Color Gradients of Elliptical Galaxies and Their Environmental Dependence
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