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We have derived colour gradients for a sample of 20 early-type galaxies (ETGs) at 1 < z_spec < 2 selected from the GOODS-South field. The sample includes both normal ETGs (13) having effective radii comparable to the mean radius of local…

宇宙学与河外天体物理 · 物理学 2015-05-20 A. Gargiulo , P. Saracco , M. Longhetti

In this Letter, we present mean optical+NIR color gradient estimates for 5080 early-type galaxies (ETGs) in the grizYJHK wavebands of the Sloan Digital Sky Survey (SDSS) plus UKIRT Infrared Deep Sky Survey (UKIDSS). The color gradient is…

宇宙学与河外天体物理 · 物理学 2015-05-13 La Barbera , F. , de Carvalho , R. R

Radial trends of stellar populations in galaxies provide a valuable tool to understand the mechanisms of galaxy growth. In this paper, we present the first comprehensive analysis of optical-optical and optical-NIR colours, as a function of…

宇宙学与河外天体物理 · 物理学 2015-06-11 F. La Barbera , I. Ferreras , R. R. de Carvalho , G. Bruzual , S. Charlot , A. Pasquali , E. Merlin

We analyze the color gradients (CGs) of ~50000 nearby SDSS galaxies. From synthetic spectral models based on a simplified star formation recipe, we derive the mean spectral properties, and explain the observed radial trends of the color as…

宇宙学与河外天体物理 · 物理学 2015-05-18 C. Tortora , N. R. Napolitano , V. F. Cardone , M. Capaccioli , Ph. Jetzer , R. Molinaro

Using optical-optical and optical-NIR colors, we analyze the radial dependence of age and metallicity inside massive (M* > 10^10.5 MSun), low-redshift (z<0.1), early-type galaxies (ETGs), residing in both high-density group regions and the…

宇宙学与河外天体物理 · 物理学 2015-05-30 F. La Barbera , I. Ferreras , R. R. de Carvalho , P. A. A. Lopes , A. Pasquali , I. G. de la Rosa , G. De Lucia

We present an analysis of stellar population gradients in 4,546 Early-Type Galaxies with photometry in $grizYHJK$ along with optical spectroscopy. A new approach is described which utilizes color information to constrain age and metallicity…

宇宙学与河外天体物理 · 物理学 2015-05-19 F. La Barbera , R. R. de Carvalho , I. G. de la Rosa , R. R. Gal , R. Swindle , P. A. A. Lopes

[Abridged]We present the morphological analysis based on HST-NICMOS observations in the F160W filter of a sample of 32 early-type galaxies (ETGs) at 1<z<2 with spectroscopic confirmation of their redshift and spectral type. We find that…

天体物理学 · 物理学 2009-11-13 P. Saracco , M. Longhetti , S. Andreon

We analyse the Fundamental Plane (FP) relation of $39,993$ early-type galaxies (ETGs) in the optical (griz) and $5,080$ ETGs in the Near-Infrared (YJHK) wavebands, forming an optical$+$NIR sample of $4,589$ galaxies. We focus on the…

宇宙学与河外天体物理 · 物理学 2015-05-18 F. La Barbera , P. A. A. Lopes , R. R. de Carvalho , I. G. de la Rosa , A. A. Berlind

We study a sample of 936 early-type galaxies (ETGs) located in 48 low-z regular galaxy clusters with $M_{200}\geq 10^{14}~ M_\odot$ at $z< 0.1$. We examine variations in the concentration index, radius, and color gradient of ETGs as a…

星系天体物理 · 物理学 2023-03-01 A. L. B. Ribeiro , R. S. Nascimento , D. F. Morell , P. A. A. Lopes , C. C. Dantas , M. H. S. Fonseca

Stellar population studies of early-type galaxies (ETGs) based on their optical stellar continuum suggest that these are quiescent systems. However, emission lines and ultraviolet photometry reveal a diverse population. We use a new version…

We study surface brightness fluctuations (SBF) in a sample of 8 elliptical galaxies using Advanced Camera for Surveys (ACS) Wide Field Channel (WFC) data drawn from the Hubble Space Telescope (HST) archive. SBF magnitudes in the F814W…

We study the internal radial gradients of the stellar populations in a sample comprising 522 early-type galaxies (ETGs) from the SAMI (Sydney- AAO Multi-object Integral field spectrograph) Galaxy Survey. We stack the spectra of individual…

We have investigated the radial g-r color gradients of early-type galaxies in the Sloan Digital Sky Survey (SDSS) DR6 in the redshift range 0.00<z<0.06. The majority of massive early-type galaxies show a negative color gradient (red-cored)…

星系天体物理 · 物理学 2015-05-18 Hyewon Suh , Hyunjin Jeong , Kyuseok Oh , Sukyoung K. Yi , Ignacio Ferreras , Kevin Schawinski

We present a detailed spatial analysis of stellar populations based on long-slit optical spectra in a sample of eight luminous early-type galaxies selected from nearby sparse groups and pairs, three of them may be interacting with a galaxy…

星系天体物理 · 物理学 2018-06-11 D. A. Rosa , A. C. Milone , A. C. Krabbe , I. Rodrigues

Context: The radial variations of the stellar populations properties within passive galaxies at high redshift contain information about their assembly mechanisms, based on which galaxy formation and evolution scenarios may be distinguished.…

星系天体物理 · 物理学 2022-04-27 F. R. Ditrani , S. Andreon , M. Longhetti , A. Newman

We present radial stellar population parameters for a subsample of 12 galaxies from the 36 isolated early-type galaxies of Reda et al. Using new long-slit spectra, central values and radial gradients for the stellar age, metallicity [Z/H]…

天体物理学 · 物理学 2008-11-26 Fatma M. Reda , Robert N. Proctor , Duncan A. Forbes , George K. T. Hau , Søren S. Larsen , ;

The evolution of galaxies is imprinted in their stellar populations. Several stellar population properties in massive early-type galaxies have been shown to correlate with intrinsic galaxy properties like the galaxy's central velocity…

星系天体物理 · 物理学 2021-12-22 A. Feldmeier-Krause , I. Lonoce , W. L. Freedman

We report the detection of color gradients in six massive (stellar mass > 10^{10} M_{sun}) and passively evolving (specific SFR < 10^{-11}/yr) galaxies at redshift 1.3<z<2.5 identified in the HUDF using HST ACS and WFC3/IR images. After…

We present results of age and metallicity gradient analysis inferred from both optical and near-infrared surface photometry. The analysis is based on a sample of 36 nearby early-type galaxies, obtained from the Early Data Release of the…

天体物理学 · 物理学 2008-11-26 Hong Wu , Zhengyi Shao , H. J. Mo , Xiaoyang Xia , Zugan Deng

We present a technique that permits the analysis of stellar population gradients in a relatively low cost way compared to IFU surveys analyzing a vastly larger samples as well as out to larger radii. We developed a technique to analyze…

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