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
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New limits on galaxy formation at high redshift [PDF]
I. M. Parkes+2 more
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The Thickness of Galaxy Disks from z = 5 to 0 Probed by JWST
Although a thick disk is a structure prevalent in local disk galaxies and also present in our home Galaxy, its formation and evolution are still unclear.
Jianhui Lian, Li Luo
doaj +1 more source
Strong limits on the 20- m emission from the high-redshift galaxy IRAS 10214 + 4724 [PDF]
C. M. Telesco
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A Simple Model of the Radio–Infrared Correlation Depending on Gas Surface Density and Redshift
We introduce a simple parametric model of the radio–infrared correlation (i.e., the ratio between the IR luminosity and the 1.4 GHz radio luminosity, q _IR ) by considering the energy loss rate of high-energy cosmic-ray (CR) electrons governed by ...
Ilsang Yoon
doaj +1 more source
The Metallicity of High‐Redshift Galaxies: The Abundance of Zinc in 34 Damped Lyα Systems fromz= 0.7 to 3.4 [PDF]
Max Pettini+3 more
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Lack of Evolution in the Iron Abundance in Clusters of Galaxies and Implications for the Global Star Formation Rate at High Redshift [PDF]
R. F. Mushotzky, M. Loewenstein
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High-redshift galaxies, their active nuclei and central black holes [PDF]
Martin G. Haehnelt+2 more
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The Average Stellar Population Age and Metallicity of Intermediate-redshift Quiescent Galaxies
The HectoMAP spectroscopic survey provides a unique mass-limited sample of more than 35,000 quiescent galaxies ( D _n 4000 > 1.5) covering the redshift range 0.2 10 ^11 M _⊙ ) assemble the bulk of their stars at earlier epochs.
Ivana Damjanov+2 more
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