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Related papers: Evolution of central dark matter of early-type gal…

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Dynamical studies of local ETGs and the Fundamental Plane point to a strong dependence of M/L ratio on luminosity (and stellar mass) with a relation of the form $M/L \propto L^{\gamma}$. The "tilt" $\gamma$ may be caused by various factors,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 C. Tortora , N. R. Napolitano , A. J. Romanowsky , M. Capaccioli , G. Covone

ABRIDGED: We study the evolution since z~1 of the rest-frame B luminosity function of the early-type galaxies (ETGs) in ~0.7 deg^2 in the COSMOS field. In order to identify ALL progenitors of local ETGs we construct the sample of high-z…

We present a new measurement of the dark and luminous matter distribution of massive elliptical galaxies, and their evolution with redshift, by combining strong lensing and dynamical observables. Our sample of 56 lens galaxies covers a…

Spectroscopic + photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging to determine the galaxy size-mass distribution over the…

We study the total density distribution in the central regions (~ 1 effective radius, $R_e$) of early-type galaxies (ETGs), using data from SPIDER and $\rm ATLAS^{3D}$. Our analysis extends the range of galaxy stellar mass ($M_{\star}$)…

Astrophysics of Galaxies · Physics 2015-06-22 C. Tortora , F. La Barbera , N. R. Napolitano , A. J. Romanowsky , I. Ferreras , R. R. de Carvalho

Aims: In this work we aim to investigate the late evolution of ETGs, both observationally and theoretically, by focusing on the stellar mass density profile inside a fixed aperture, within $10 ~\rm{kpc}$ from the galaxy center. Methods: We…

Astrophysics of Galaxies · Physics 2025-09-18 Rongfu Liu , Alessandro Sonnenfeld , Carlo Nipoti , Rui Li

We present a comprehensive analysis of the dark matter (DM) content and its structural dependence in star-forming disk-like galaxies at intermediate redshifts ($0.1 \lesssim z \lesssim 0.85$), utilizing spatially resolved kinematic data…

This work aims to study the distribution of luminous and dark matter in Coma early-type galaxies. Dynamical masses obtained under the assumption that mass follows light do not match with the masses of strong gravitational lens systems of…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 J. Thomas , R. P. Saglia , R. Bender , D. Thomas , K. Gebhardt , J. Magorrian , E. M. Corsini , G. Wegner , S. Seitz

We examine correlations between the masses, sizes, and star formation histories for a large sample of low-redshift early-type galaxies, using a simple suite of dynamical and stellar populations models. We confirm an anti-correlation between…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Nicola R. Napolitano , Aaron J. Romanowsky , Crescenzo Tortora

We present an optical analysis of a sample of 11 clusters built from the EXCPRES sample of X-ray selected clusters at intermediate redshift (z ~ 0.5). With a careful selection of the background galaxies we provide the mass maps…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-02 Genevieve Soucail , Gael Foex , Etienne Pointecouteau , Monique Arnaud , Marceau Limousin

We constrain the evolution of the galaxy mass and luminosity functions from the analysis of (public) multi-wavelength data in the Chandra Deep Field South (CDFS) area, obtained from the GOODS and other projects, and including very deep…

We have constructed self-consistent light and mass distribution models for four disk galaxies at redshifts z = 0.48, 0.58, 0.81 and 0.88, using the HST archive WFPC2 observations and rotation curves measured by Vogt et al. (1996) and…

Astrophysics · Physics 2007-05-23 A. Tamm , P. Tenjes

We present the deepest clustering analysis of early galaxies to date, analyzing $N_{\rm{g}} \simeq 6500$ photometrically-selected Lyman Break Galaxies from JWST's Advanced Deep Extragalactic Survey (JADES) to reveal how galaxies and dark…

Astrophysics of Galaxies · Physics 2026-01-06 Nicolò Dalmasso , Giovanni Ferrami , Nicha Leethochawalit , Emanuele M. Ventura , Michele Trenti

We investigate the redshift evolution of the intrinsic alignments (IA) of galaxies in the \texttt{MassiveBlackII} (MBII) simulation. We select galaxy samples above fixed subhalo mass cuts ($M_h>10^{11,12,13}~M_{\odot}/h$) at $z=0.6$ and…

Cosmology and Nongalactic Astrophysics · Physics 2020-01-08 Aklant K Bhowmick , Yingzhang Chen , Ananth Tenneti , Tiziana Di Matteo , Rachel Mandelbaum

We present a joint gravitational lensing and stellar-dynamical analysis of 11 early-type galaxies (median deflector redshift $\zd=0.5$) from Strong Lenses in the Legacy Survey (SL2S). Using newly measured redshifts and stellar velocity…

Cosmology and Nongalactic Astrophysics · Physics 2011-01-14 Andrea J. Ruff , Raphael Gavazzi , Philip J. Marshall , Tommaso Treu , Matthew W. Auger , Florence Brault

We determine an absolute calibration of stellar mass-to-light ratios for the densest \simeq 3% of early-type galaxies in the local universe (redshift z\simeq 0.08) from SDSS DR7. This sample of \sim 4000 galaxies has, assuming a Chabrier…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Aaron A. Dutton , J. Trevor Mendel , Luc Simard

We present the results on the stellar Initial Mass Function (IMF) normalisation of 68 massive ($M_\ast=10^{11}-10^{12}$$M_\odot$) Early-Type Galaxies (ETGs) at redshift of $\sim$1. This was achieved by deriving the stellar Mass-to-Light…

Astrophysics of Galaxies · Physics 2015-06-23 Shravan Shetty , Michele Cappellari

We investigate the total mass density slope evolution in massive early-type galaxies (ETGs) over the last 6.5 billion years ($0 < z < 0.75$). We perform a detailed dynamical analysis of approximately 200 ETGs spanning the redshift range…

Astrophysics of Galaxies · Physics 2026-02-12 Pritom Mozumdar , Michele Cappellari , Christopher D. Fassnacht , Tommaso Treu

We use the Fundamental Plane (FP) to measure the redshift evolution of the dynamical mass-to-light ratio ($M_{\mathrm{dyn}}/L$) and the dynamical-to-stellar mass ratio ($M_{\mathrm{dyn}}/M_*$). Although conventionally used to study the…

We aim to discern scenarios of structural evolution of intermediate to high-mass star-forming galaxies (SFGs) since cosmic noon by comparing their stellar mass profiles with present-day stellar masses of…

Astrophysics of Galaxies · Physics 2024-10-10 Maryam Hasheminia , Moein Mosleh , S. Zahra Hosseini-ShahiSavandi , Sandro Tacchella