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相关论文: K-luminous galaxies at z~2. Metallicity and B star…

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We present the analysis of the coadded rest-frame UV spectrum (1200<z<2000 A) of five K-luminous galaxies at z~2 from the K20 survey. The composite spectrum is characterized by strong absorption lines over the UV continuum from C, N, O, Al,…

天体物理学 · 物理学 2009-11-10 Duilia de Mello , E. Daddi , A. Renzini , A. Cimatti , S. di Serego Alighieri , L. Pozzetti , G. Zamorani

We present results of near-IR spectroscopic measurements of 7 star-forming galaxies at 2.1<z<2.5. Drawn from a large spectroscopic survey of galaxies photometrically pre-selected by their U_nGR colors to lie at z~2, these galaxies were…

天体物理学 · 物理学 2009-07-09 A. E. Shapley , D. K. Erb , M. Pettini , C. C. Steidel , K. L. Adelberger

We characterize massive stars (M>8 M_sun) in the nearby (D~0.8 Mpc) extremely metal-poor (Z~5% Z_sun) galaxy Leo A using Hubble Space Telescope ultra-violet (UV), optical, and near-infrared (NIR) imaging along with Keck/LRIS and…

Spectroscopic redshifts have been measured for 9 K-band luminous galaxies at 1.7 < z < 2.3, selected with Ks < 20 in the "K20 survey" region of the Great Observatories Origins Deep Survey area. Star formation rates (SFRs) of ~100-500…

We present the rest-frame optical spectrum of a strongly lensed galaxy at redshift z =1.7 behind the cluster Abell 1689. We detect the temperature sensitive auroral line [O III] 4363, which allows the first direct metallicity measurement…

宇宙学与河外天体物理 · 物理学 2009-07-09 T. -T. Yuan , L. J. Kewley

We have obtained optical spectra of four galaxies associated with MgII QSO absorbers at redshifts 0.10 < z < 0.45. We calculate the gas-phase oxygen abundance of these galaxies using the empirical R23 strong line method. The absolute B-band…

天体物理学 · 物理学 2009-11-10 Sara L. Ellison , Lisa J. Kewley , Gabriela Mallen-Ornelas

New high-resolution maps with the IRAM Interferometer of the redshifted [C II] 158 micron line and the 0.98mm dust continuum of HDF850.1 at z = 5.185 show the source to have a blueshifted northern component and a redshifted southern…

星系天体物理 · 物理学 2015-06-18 R. Neri , D. Downes , P. Cox , F. Walter

We present new Keck observations of giant arcs in the cluster Abell 2390. High resolution two-dimensional spectra of two arcs show metal lines at z=4.040 +/- 0.005 with Lyman-alpha emission spatially separated from the stellar continuum. In…

天体物理学 · 物理学 2007-05-23 B. L. Frye , T. J. Broadhurst , H. Spinrad , A. Bunker

We report on the surprisingly high metallicity measured in two absorption systems at high redshift, detected in the Very Large Telescope spectrum of the afterglow of the gamma-ray burst GRB 090323. The two systems, at redshift z=3.5673 and…

We present the first detection of the [N II] 122 $\mu$m and [O III] 52 $\mu$m lines for a reionisation-epoch galaxy. Based on these lines and previous [C II] 158 $\mu$m and [O III] 88 $\mu$m measurements, using two different radiative…

This study presents Keck optical and infrared spectroscopy of the rest-frame ultraviolet and optical emission lines in two Lyman alpha emitting galaxies at z>2. These data provide insight on the evolution of fundamental galaxy scaling…

天体物理学 · 物理学 2007-05-23 Chip Kobulnicky , David Koo

We present K-band imaging of fields around 30 strong CaII absorption line systems, at 0.7<z<1.1, three of which are confirmed Damped Lyman-alpha systems. A significant excess of galaxies is found within 6"0 (~50kpc) from the absorber…

天体物理学 · 物理学 2009-06-23 Paul Hewett , Vivienne Wild

High resolution, 1.1, 1.6, and 2.2 micron imaging of the luminous infrared galaxy NGC 6090 obtained with NICMOS of the Hubble Space Telescope are presented. These new observations are centered on the two nuclei of the merger, and reveal the…

天体物理学 · 物理学 2009-10-31 N. Dinshaw , A. S. Evans , H. Epps , N. Z. Scoville , M. Rieke

We discuss the spectral character of Lyman-limit-selected, star-forming galaxies at z>3. The rest-frame UV spectra of these faint galaxies may show Ly-alpha in either absorption or emission, probably depending upon their local ISM content…

天体物理学 · 物理学 2007-05-23 Hyron Spinrad , Arjun Dey , Daniel Stern , Andrew Bunker

We analyse subarcsecond resolution interferometric CO line data for twelve sub-millimetre-luminous (S850um > 5mJy) galaxies with redshifts between 1 and 3, presenting new data for four of them. Morphologically and kinematically most of the…

宇宙学与河外天体物理 · 物理学 2010-11-03 H. Engel , L. J. Tacconi , R. I. Davies , R. Neri , I. Smail , S. C. Chapman , R. Genzel , P. Cox , T. R. Greve , R. J. Ivison , A. Blain , F. Bertoldi , A. Omont

We have discovered a sample of 17 metal-poor, yet luminous, star-forming galaxies at redshifts z~0.7. They were selected from the initial phase of the DEEP2 survey of 3900 galaxies and the Team Keck Redshift Survey (TKRS) of 1536 galaxies…

We present and analyse near-infrared spectroscopy for a sample of 28 gravitationally- lensed star-forming galaxies in the redshift range 1.5 < z < 5, observed mostly with the Keck II telescope. With typical magnifications of ~1.5-4…

宇宙学与河外天体物理 · 物理学 2015-05-20 Johan Richard , Tucker Jones , Richard S. Ellis , Daniel P. Stark , Rachael Livermore , Mark Swinbank

In order to reveal the stellar mass distribution of z~3 galaxies, we are conducting deep imaging observations of U-dropout Lyman Break Galaxies (LBGs) with Adaptive Optics (AO) systems in K-band, which corresponds to rest-frame V-band of…

天体物理学 · 物理学 2009-11-13 M. Akiyama , Y. Minowa , N. Kobayashi , K. Ohta , I. Iwata

We present a detailed analysis of a large-scale galactic outflow in the CGM of a massive (M_h ~ 10^12.5 Msun), star-forming (6.9 Msun/yr), sub-L* (0.5 L_B*) galaxy at z=0.39853 that exhibits a wealth of metal-line absorption in the spectra…

We present initial results of a deep near-IR spectroscopic survey covering the 15 fields of the Keck Baryonic Structure Survey (KBSS) using MOSFIRE on the Keck 1 telescope, focusing on a sample of 251 galaxies with redshifts 2.0< z < 2.6,…

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