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相关论文: The Evolution of Cluster Early-Type Galaxies over …

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We present the Fundamental Plane (FP) for 38 early-type galaxies in the two rich galaxy clusters RXJ0152.7-1357 (z=0.83) and RXJ1226.9+3332 (z=0.89), reaching a limiting magnitude of M_B =-19.8 mag in the rest frame of the clusters. While…

天体物理学 · 物理学 2009-11-11 Inger Jorgensen , Kristin Chiboucas , Kathleen Flint , Marcel Bergmann , Jordi Barr , Roger Davies

We present the Fundamental Plane (FP) of field early-type galaxies at 0.5<z<1.0. Our project is a continuation of our efforts to understand the formation and evolution of early-type galaxies in different environments. The target galaxies…

宇宙学与河外天体物理 · 物理学 2015-05-18 Alexander Fritz , Inger Jorgensen , Ricardo P. Schiavon

We present new results on the Fundamental Plane of galaxies in two rich clusters, Cl1358+62 at $z=0.33$ and MS2053--04 at $z=0.58$, based on Keck and HST observations. Our new data triple the sample of galaxies with measured Fundamental…

We present an analysis of stellar populations and evolutionary history of galaxies in three similarly rich galaxy clusters MS0451.6-0305 (z=0.54), RXJ0152.7-1357 (z=0.83), and RXJ1226.9+3332 (z=0.89); based on high S/N ground-based optical…

宇宙学与河外天体物理 · 物理学 2013-02-28 Inger Jorgensen , Kristin Chiboucas

We present results from an optical-IR photometric study of early-type galaxies in 19 galaxy clusters out to z=0.9. The galaxy sample is selected on the basis of morphologies determined from HST WFPC2 images, and is photometrically defined…

天体物理学 · 物理学 2009-10-30 S. A. Stanford , Peter R. Eisenhardt , Mark Dickinson

We present results on the Fundamental Plane (FP) of early-type galaxies in the cluster RDCS J0848+4453 at z=1.27. Internal velocity dispersions of three K-selected early-type galaxies are determined from deep Keck spectra. Structural…

天体物理学 · 物理学 2011-05-05 Pieter G. van Dokkum , S. A. Stanford

We perform a morphological study of 124 spectroscopically confirmed cluster galaxies in the z=0.84 galaxy cluster RX J0152.7-1357. Our classification scheme includes color information, visual morphology, and 1-component and 2-component…

宇宙学与河外天体物理 · 物理学 2015-06-15 Julie B. Nantais , Hector Flores , Ricardo Demarco , Chris Lidman , Piero Rosati , M. James Jee

The slow evolution of the M/L ratios, colors, and line strengths of cluster early-type galaxies to z=1 suggests that their stars were formed at very high redshift. At the same time, morphological studies of distant clusters indicate…

天体物理学 · 物理学 2007-05-23 P. G. van Dokkum , M. Franx , D. D. Kelson , G. D. Illingworth , D. Fabricant

We have measured the Fundamental Plane (FP) parameters for a sample of 30 field early-type galaxies (E/S0) in the redshift range 0.1<z<0.66. We find that: i) the FP is defined and tight out to the highest redshift bin; ii) the intercept…

天体物理学 · 物理学 2014-10-13 T. Treu , M. Stiavelli , S. Casertano , P. Møller , G. Bertin

We use new models of stellar population synthesis to estimate the fraction of stars formed during the last major bursts of star formation in E/S0 galaxies in low-redshift clusters ($z\simlt0.4$) from the spectral signatures of…

天体物理学 · 物理学 2009-10-22 S. Charlot , J. Silk

We present spectroscopic observations obtained at the {\it Large Binocular Telescope} in the field of the cluster XLSSJ0223-0436 at $z=1.22$. We confirm 12 spheroids cluster members and determine stellar velocity dispersion for 7 of them.…

星系天体物理 · 物理学 2019-11-06 P. Saracco , A. Gargiulo , F. La Barbera , M. Annunziatella , D. Marchesini

Morphological and spectroscopic studies of high redshift clusters indicate that a significant fraction of present-day early-type galaxies was transformed from star forming galaxies at z<1. On the other hand, the slow luminosity evolution of…

天体物理学 · 物理学 2007-05-23 Pieter G. van Dokkum , Marijn Franx

We introduce our project that investigates the kinematic properties of early-type galaxies in 6 distant poor clusters at z~0.25. This study represents a continuation of our efforts to understand galaxy evolution in low-density environments.…

天体物理学 · 物理学 2009-11-10 Alexander Fritz , Bodo L. Ziegler

A magnitude limited sample of nearly 9000 early-type galaxies, in the redshift range 0.01 < z < 0.3, was selected from the Sloan Digital Sky Survey using morphological and spectral criteria. The Fundamental Plane relation in this sample is…

We present a study of the galaxy population in the cluster RXJ0848+4453 at z=1.27, using deep HST NICMOS and WFPC2 images. We morphologically classify all galaxies to K_s=20.6 that are covered by the HST imaging, and determine photometric…

天体物理学 · 物理学 2009-11-06 P. G. van Dokkum , S. A. Stanford , B. P. Holden , P. R. Eisenhardt , M. Dickinson , R. Elston

We present preliminary results on the evolution of the stellar populations of field early-type galaxies (E/S0) from z=0.4 to z=0. The diagnostic tool used in this study is the Fundamental Plane (FP), a tight empirical correlation between…

天体物理学 · 物理学 2007-05-23 T. Treu , M. Stiavelli , S. Casertano , P. Moller , G. Bertin

We study the Fundamental Plane of field early-type galaxies at intermediate redshift, using HST WFPC2 observations and deep Keck spectroscopy. Structural parameters and internal velocity dispersions are measured for eighteen galaxies at…

天体物理学 · 物理学 2009-11-06 Pieter G. van Dokkum , Marijn Franx , Daniel D. Kelson , Garth D. Illingworth

By exploting the data of three large surveys (WINGS, NFPS and SDSS), we present here a comparative analysis of the Fundamental Plane (FP hereafter) of the early-type galaxies (ETGs) belonging to 59 galaxy clusters in the redshift range…

We present new Keck spectroscopy of early-type galaxies in three galaxy clusters at z~0.5. We focus on the fundamental plane (FP) relation, and combine the kinematics with structural parameters determined from HST images. The galaxies obey…

天体物理学 · 物理学 2008-11-26 Pieter G. van Dokkum , Roeland P. van der Marel

We present the ellipticity distribution and its evolution for early-type galaxies in clusters from z~0.8 to z~0, based on the WIde-field Nearby Galaxy-cluster Survey (WINGS)(0.04<z<0.07), and the ESO Distant Cluster Survey…

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