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We present a study of the H$\alpha$ line emission from a sample of 1482 optically-selected, morphologically-classified bright galaxies (median redshift of 0.05) derived from the Sloan Digital Sky Survey. The luminosity function is…

天体物理学 · 物理学 2009-11-10 Osamu Nakamura , Masataka Fukugita , Jon Brinkmann , Donald P. Schneider

We report on a complete sample of 7 luminous early-type galaxies in the Hubble Ultra Deep Field (UDF) with spectroscopic redshifts between 1.39 and 2.47 and to K<23 AB. Using the BzK selection criterion we have pre-selected a set of objects…

We focus on an analysis of galaxies of high stellar mass and low metallicity. We cross-correlated the Millenium Galaxy Catalogue (MGC) and the Sloan Digital Sky Survey (SDSS) galaxy catalogue to provide a sample of MGC objects with high…

宇宙学与河外天体物理 · 物理学 2010-02-20 M. S. Alonso , L. Michel-Dansac , D. G. Lambas

We have studied a sample of 11 blue, luminous, metal-poor galaxies at redshift 0.744 < z < 0.835 from the DEEP2 redshift survey. They were selected by the presence of the [OIII]4363 auroral line and the [OII]3726,3729 doublet together with…

星系天体物理 · 物理学 2014-12-15 J. M. Perez-Martinez

We present the analysis of 10 massive early-type galaxies at $z\sim1.5$. They have been identified by means of a near-IR low resolution spectroscopic follow-up of a complete sample of 36 bright (K' $<$ 18.5) Extremely Red Objects (EROs,…

天体物理学 · 物理学 2009-11-11 M. Longhetti , P. Saracco , P. Severgnini , R. Della Ceca , V. Braito , F. Mannucci , R. Bender , N. Drory , G. Feulner , U. Hopp

Our understanding of early-type galaxies (ETGs) has grown in the past decade with the advance of full-spectrum fitting techniques used to infer the properties of the stellar populations that make-up the galaxy. We present ages, central…

星系天体物理 · 物理学 2024-06-25 Nicholas Barth , George C. Privon , Rana Ezzeddine , Aaron S. Evans , Ezequiel Treister

We studied the radio properties of very young massive regions of star formation in HII galaxies, with the aim of detecting episodes of recent star formation in an early phase of evolution where the first supernovae start to appear. Our…

天体物理学 · 物理学 2008-11-26 D. Rosa-Gonzalez , H. R. Schmitt , E. Terlevich , R. Terlevich

We present Very Large Telescope/Xshooter spectrophotometric observations of eleven low-redshift (z<0.085) compact star-forming galaxies (`high O32 sample'). These galaxies are characterised by extremely high emission-line ratios…

星系天体物理 · 物理学 2026-05-08 Y. I. Izotov , N. G. Guseva , D. Schaerer , R. O. Amorin

We have analyzed 17 early-type galaxies, 13 ellipticals and 4 S0's, observed with Suzaku, and investigated metal abundances (O, Mg, Si, and Fe) and abundance ratios (O/Fe, Mg/Fe, and Si/Fe) in the interstellar medium (ISM). The emission…

星系天体物理 · 物理学 2015-06-18 Saori Konami , Kyoko Matsushita , Ryo Nagino , Toru Tamagawa

We analysed the nuclear region of all 56 early-type galaxies from the DIVING$^\mathrm{3D}$ Project, which is a statistically complete sample of objects that contains all 170 galaxies of the Southern Hemisphere with B < 12.0 mag and galactic…

星系天体物理 · 物理学 2023-04-28 T. V. Ricci , J. E. Steiner , R. B. Menezes , K. Slodkowski Clerici , M. D. da Silva

We have investigated the properties of a bright K-band selected sample of early-type galaxies in the Hubble Deep Field, as representative of the field galaxy population. This dataset is unique as for the morphological information on faint…

天体物理学 · 物理学 2007-05-23 Alberto Franceschini , Laura Silva , Gian Luigi Granato , Alessandro Bressan , Luigi Danese

We present UFTI K-band imaging observations of 222 galaxies that are selected from the Sloan Digital Sky Survey to have unusually strong Hdelta absorption equivalent widths, W(Hd)>4A. Using GIM2D, the images are fit with two-dimensional…

天体物理学 · 物理学 2009-11-10 Michael L. Balogh , Chris Miller , Robert Nichol , Ann Zabludoff , Tomo Goto

(Abridged) We present a comprehensive analysis of the spatially resolved stellar population properties of 26 early-type dwarf (dE) galaxies in the Virgo cluster. Using Lick/IDS absorption line indices we derive simple stellar…

星系天体物理 · 物理学 2015-05-20 Sanjaya Paudel , Thorsten Lisker , Harald Kuntschner

Using the \prospector\ spectral energy distribution (SED) fitting code, we analyze the properties of 19 Extreme Emission Line Galaxies (EELGs) identified in the bluest composite SED in the \zfourge\ survey at $2.5 \leq z \leq 4$.…

We present a sample of 48 metal-poor galaxies at $ z < 0.14$ selected from 92,510 galaxies in the LAMOST survey. These galaxies are identified for their detection of the auroral emission line \oiii$\lambda$4363 above $3\sigma$ level, which…

星系天体物理 · 物理学 2017-05-10 Yulong Gao , Jianhui Lian , Xu Kong , Zesen Lin , Ning Hu , Haiyang Liu , Enci Wang , Zihuang Cao , Yonghui Hou , Yuefei Wang , Yong Zhang

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

The presence of transitional dwarf galaxies in filaments and cluster outskirts may be closely related to pre-processing in the filament; however, the underlying mechanism is not yet comprehensively understood. We present the spatially…

星系天体物理 · 物理学 2023-06-07 Jiwon Chung , Joon Hyeop Lee , Hyunjin Jeong , Suk Kim

We present the gas-phase oxygen abundance (O/H) for a sample of 131 star-forming galaxies at intermediate redshifts ($0.2<z<1.0$). The sample selection, the spectroscopic observations (mainly with VLT/FORS) and associated data reduction,…

We present HI data cubes of four low-luminosity early-type galaxies which are currently forming stars. These galaxies have absolute magnitudes in the range M_B=-17.9 to -19.9 (H_o=50 km/s/Mpc). Their HI masses range between a few times 10^8…

天体物理学 · 物理学 2016-08-30 E. Sadler , T. Oosterloo , R. Morganti

We examine the evolutionary status of luminous, star-forming galaxies in intermediate-redshift clusters by considering their star formation rates and the chemical and ionsiation properties of their interstellar emitting gas. Our sample…

天体物理学 · 物理学 2009-11-11 M. Mouhcine , S. P. Bamford , A. Aragon-Salamanca , O. Nakamura
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