Results 151 to 160 of about 210,144 (261)
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
A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function
We present a new sample of 158 galaxies at redshift z > 7.5 selected from deep James Webb Space Telescope (JWST) NIRCam imaging of five widely separated sight lines in the CANUCS survey.
Chris J. Willott +17 more
doaj +1 more source
Utilizing the COSMOS H I Large Extragalactic Survey (CHILES) data set, we investigate the evolution of the average atomic neutral hydrogen (H I ) properties of galaxies over the continuous redshift range 0.09
Nicholas Luber +11 more
doaj +1 more source
Characterising the relationship between dense gas and star formation is critical for understanding the assembly of galaxies throughout cosmic history. However, due to the faintness of standard dense-gas tracers – HCN, HCO+, and HNC – dense gas in high ...
Rybak M. +9 more
doaj +1 more source
Cosmic Magnification of High-Redshift Submillimeter Galaxies
Weak lensing magnification probes the correlation between galaxies and the underlying matter field in a similar fashion to galaxy–galaxy lensing shear. Although it has long been sidelined in favor of the latter on the grounds of poorer performance in terms of statistical significance, the provision of a large sample of high-redshift submillimeter ...
Marcos M. Cueli +3 more
openaire +3 more sources
BEACON: JWST NIRCam Pure-parallel Imaging Survey. I. Survey Design and Initial Results
We introduce the Bias-free Extragalactic Analysis for Cosmic Origins with NIRCam (BEACON) survey, a JWST Cycle 2 program allocated up to 600 pure-parallel hours of observations.
Takahiro Morishita +34 more
doaj +1 more source
Unveiling the Formation of Massive Galaxies
Massive galaxies, such as nearby ellipticals, have relatively low number densities, yet they host the majority of the stellar mass in the universe. Understanding their origin is a central problem of galaxy formation.
Conselice, Christopher J.
core +1 more source
JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34
We spectroscopically confirm the M _UV = −20.5 mag galaxy GHZ2/GLASS-z12 to be at redshift z = 12.34. The source was selected via NIRCam photometry in GLASS-JWST Early Release Science data, providing the first evidence of a surprising abundance of bright
Marco Castellano +30 more
doaj +1 more source
Photometric Redshift Estimation Using Scaled Ensemble Learning
The development of the state-of-the-art telescopic systems capable of performing expansive sky surveys such as the Sloan Digital Sky Survey, Euclid, and the Rubin Observatory’s Legacy Survey of Space and Time (LSST) has significantly advanced efforts to ...
Swagata Biswas +7 more
doaj +1 more source
The distribution and lifetime of powerful radio galaxies as a function of environment and redshift
Correlations between jet power and active time for z
David Garofalo +2 more
doaj +1 more source

