Results 71 to 80 of about 252,176 (198)
Abundances in Damped Lyα Galaxies [PDF]
Damped Lyα galaxies provide a sample of young galaxies where chemical abundances can be derived throughout the whole universe with an accuracy comparable to that for the local universe.
P. Molaro
semanticscholar +1 more source
We report the large scale structure and clustering analysis of Ly α emitters (LAEs) and Ly α blobs (LABs) at z = 2.2–2.3. Using 3341 LAEs, 117 LABs, and 58 bright (Ly α luminosity L _Ly _α > 10 ^43.4 erg s ^−1 ) LABs at z = 2.2–2.3 selected with ...
Haibin Zhang +12 more
doaj +1 more source
Do galaxies that leak ionizing photons have extreme outflows?
To reionize the early universe, high-energy photons must escape the galaxies that produce them. It has been suggested that stellar feedback drives galactic outflows out of star-forming regions, creating low density channels through which ionizing photons
Chisholm, J. +7 more
core +1 more source
The Relationship Between Galaxies and Low Redshift Weak Lyman alpha Absorbers in the Directions of H1821+643 and PG1116+215 [PDF]
To study the nature of low z Lya absorbers in the spectra of QSOs, we have obtained high signal-to-noise UV spectra of H 1821+643 (z = 0.297) and PG 1116+215 (z = 0.177) with the GHRS on the HST.
Blair D. Savage +8 more
core +2 more sources
The Lyα Dependence on Nebular Properties from the HETDEX and MOSDEF Surveys
Investigating the impact of galaxy properties on emergent Ly α emission is crucial for reionization studies, given the sensitivity of Ly α to neutral hydrogen.
Óscar A. Chávez Ortiz +16 more
doaj +1 more source
Galaxies Inside Stromgren Spheres of Luminous Quasars at z>6: Detection of The First Galaxies
The intrinsic Lyman-alpha emission lines of normal galaxies before reionization are much absorbed by the damping wing of the Gunn-Peterson trough, rendering their direct detection nearly impossible, if their intrinsic line widths are less than ~100km/s ...
Antonucci R. R. J. +2 more
core +1 more source
MAMMOTH-Subaru. III. Lyα Halo Identified by Stacking ∼3300 Lyα Emitters at z = 2.2–2.3
In this paper, we present a Ly α halo (LAH) identified by stacking ∼3300 Ly α emitters (LAEs) at z = 2.2–2.3. We carry out imaging observations and data reduction with Subaru/Hyper Suprime-Cam.
Haibin Zhang +10 more
doaj +1 more source
SIMPLE: Simple Intensity Map Producer for Line Emission
We present the Simple Intensity Map Producer for Line Emission ( Simple ), a public code for quickly simulating mock line-intensity maps, and an analytical framework for modeling intensity maps including observational effects.
Maja Lujan Niemeyer +2 more
doaj +1 more source
Recent Advances in Cosmological Hydrogen Reionization
I discuss recent advances in the study of hydrogen reionization, focusing on progress that was achieved during the years 2010-2011. First, I discuss recent measurements of the progress of reionization.
Finlator, Kristian
core +1 more source
Assembly of Massive Galaxies in a High-z Protocluster [PDF]
We present the results of wide-field deep JHK imaging of the SSA22 field using MOIRCS instrument equipped with Subaru telescope. The observed field is 112 arcmin^2 in area, which covers the z=3.1 protocluster characterized by the overdensities of Ly ...
Akiyama, Masayuki +14 more
core +2 more sources

