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相关论文: The Fundamental Plane for z=0.8-0.9 cluster galaxi…

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We present the Fundamental Plane (FP) of early-type galaxies in the clusters of galaxies RXJ1415.1+3612 at z=1.013. This is the first detailed FP investigation of cluster early-type galaxies at redshift z=1. The distant cluster galaxies…

宇宙学与河外天体物理 · 物理学 2009-10-22 Alexander Fritz , Inger Jorgensen , Ricardo P. Schiavon , Kristin Chiboucas

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 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 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

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 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 study the fundamental plane relation in high redshift clusters using a sample of 26 galaxies in MS 2053-04 (z=0.583) and 22 galaxies in MS 1054-03 (z=0.83). The zeropoint and scatter are compared to results for lower redshift clusters in…

天体物理学 · 物理学 2009-11-10 Stijn Wuyts , Pieter G. van Dokkum , Daniel D. Kelson , Marijn Franx , Garth D. Illingworth

We present the analysis of the fundamental plane (FP) for a sample of 19 massive red-sequence galaxies ($M_{\star} >4\times10^{10} M_{\odot}$) in 3 known overdensities at $1.39<z<1.61$ from the KMOS Cluster Survey, a guaranteed time program…

Using deep HST ACS imaging and VLT FORS2 spectra, we determined the velocity dispersions, effective radii and surface brightnesses for four early-type galaxies in the $z=1.237$ cluster \cl. All four galaxies are massive, $> 10^{11}…

We present the Fundamental Plane (FP) in the z = 0.28 cluster of galaxies RX J0142.0+2131. There is no evidence for a difference in the slope of the FP when compared with the Coma cluster, although the internal scatter is larger. On…

天体物理学 · 物理学 2011-02-11 Jordi Barr , Inger Jorgensen , Kristin Chiboucas , Roger Davies , Marcel Bergmann

We present results on the Fundamental Plane of early-type galaxies in the rich cluster CL 0024+16 at z=0.391. The galaxies satisfy a tight Fundamental Plane relation which is similar to that at low redshift. The scatter is 15 % in log re.…

天体物理学 · 物理学 2015-06-24 Pieter van Dokkum , Marijn Franx

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 present a spectroscopic sample of 48 early-type galaxies in the rich cluster Abell 2218 and 50 galaxies in Abell 2390. Since both samples are very similar, we combine them and investigate a total number of 98 early-type galaxies at…

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

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

The Fundamental Plane (FP) of early-type galaxies, relating the effective radius, velocity dispersion, and surface brightness, has long been recognized as a unique tool for analyzing galaxy structure and evolution. With the discovery of…

星系天体物理 · 物理学 2015-06-22 Jesse van de Sande , Mariska Kriek , Marijn Franx , Rachel Bezanson , Pieter G. van Dokkum

We report on the study of a sample of 25 field early-type galaxies, in the redshift range z~0.1-0.5, selected on the basis of colours and morphology from the HST-MDS. Field early-type galaxies define a tight Fundamental Plane (FP) out to…

天体物理学 · 物理学 2009-11-06 T. Treu , M. Stiavelli , G. Bertin , S. Casertano , P. Møller

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 Fundamental Plane (FP) is an empirical relation between the size, surface brightness, and velocity dispersion of early-type galaxies. This relation has been studied extensively for early-type galaxies in the local universe to constrain…

宇宙学与河外天体物理 · 物理学 2015-06-17 Rachel Bezanson , Pieter G. van Dokkum , Jesse van de Sande , Marijn Franx , Joel Leja , Mariska Kriek

RXJ0848.6+4453 (Lynx W) at redshift 1.27 is part of the Lynx Supercluster of galaxies. Our analysis of stellar populations and star formation history in the cluster covers 24 members and is based on deep optical spectroscopy from Gemini…

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…

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