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相关论文: Luminosity Evolution of Field Early-Type Galaxies …

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We analyse the Fundamental Plane (FP) of 26 strong gravitational lens galaxies with redshifts up to z~1, using tabulated data from Kochanek et al. (2000) and Rusin et al. (2003). The lens galaxies effectively form a mass-selected sample of…

天体物理学 · 物理学 2009-11-07 G. van de Ven , P. G. van Dokkum , M. Franx

We present an analysis of the Fundamental Plane for a sample of 27 field early-type galaxies in the redshift range 0.6<z<1.15. The galaxies in this sample have high S/N spectra obtained at the VLT and high resolution imaging from the ACS.…

天体物理学 · 物理学 2008-11-26 A. van der Wel , M. Franx , P. G. van Dokkum , H. -W. Rix , G. D. Illingworth , P. Rosati

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 introduce a framework for simultaneously investigating the structure and luminosity evolution of early-type gravitational lens galaxies. The method is based on the fundamental plane, which we interpret using the aperture mass-radius…

天体物理学 · 物理学 2009-11-10 D. Rusin , C. S. Kochanek

Keck spectroscopy and Hubble Space Telescope WFPC2 imaging over a 1.5x1.5 Mpc field of CL1358+62 at z=0.33 are used to study the Fundamental Plane of galaxies based on a new, large sample of 53 galaxies. First, we have constructed the…

天体物理学 · 物理学 2009-10-31 Daniel D. Kelson , Garth D. Illingworth , Pieter G. van Dokkum , Marijn Franx

We report on a uniform comparative analysis of the fundamental parameters of early-type galaxies at z~1 down to a well defined magnitude limit (M_B\leq -20.0 in the field and M_B\leq -20.5 in the clusters). The changes in the M/L_B ratio…

天体物理学 · 物理学 2011-02-11 Sperello di Serego Alighieri , Barbara Lanzoni , Inger Jorgensen

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 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 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 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 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

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 present deep Keck spectroscopy for a sample of I<22.5 field early-type galaxies selected morphologically in the redshift range 0.56<z<1.02 in the HDF-N. Using velocity dispersions determined from the Keck spectra in conjunction with…

天体物理学 · 物理学 2009-11-10 Pieter G. van Dokkum , Richard S. Ellis

We present deep spectroscopy with the Keck telescope of eight galaxies in the luminous X-ray cluster MS1054-03 at z=0.83. The data are combined with imaging observations from the Hubble Space Telescope (HST). The spectroscopic data are used…

天体物理学 · 物理学 2009-10-30 Pieter G. van Dokkum , Marijn Franx , Daniel D. Kelson , Garth D. Illingworth

We explore the properties of 24 field early-type galaxies at 0.20<z<0.75 down to M_B<=-19.30 in a sample extracted from the FORS Deep Field and the William Herschel Deep Field. High S/N intermediate-resolution VLT spectroscopy was…

宇宙学与河外天体物理 · 物理学 2009-11-13 Alexander Fritz , Asmus Boehm , Bodo L. Ziegler

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 deep VLT spectra of early type galaxies at z~1 in the Chandra Deep Field South, from which we derive velocity dispersions. Together with structural parameters from Hubble Space Telescope imaging, we can study the Fundamental…

天体物理学 · 物理学 2009-11-10 A. van der Wel , M. Franx , P. G. van Dokkum , H. -W. Rix

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…

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}…

The study of the ages of early-type galaxies and their dependence on galaxy mass and environment is crucial for understanding the formation and early evolution of galaxies. We review recent works on the M/L ratio evolution, as derived from…

天体物理学 · 物理学 2007-05-23 Sperello di Serego Alighieri , Alessandro Bressan , Lucia Pozzetti
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