Results 81 to 90 of about 2,272 (184)

The Luminosity Function and Clustering of Hα Emitting Galaxies at z ≈ 4−6 from a Complete NIRCam Grism Redshift Survey

open access: yesThe Astrophysical Journal
We study the luminosity function (LF) and clustering properties of 888 H α emitters (HAEs) at 3.75 
Xiaojing Lin   +22 more
doaj   +1 more source

The brightest UV-selected galaxies in protoclusters at $z\sim4$: Ancestors of Brightest Cluster Galaxies?

open access: yes, 2019
We present the results of a survey of the brightest UV-selected galaxies in protoclusters. These proto-brightest cluster galaxy (proto-BCG) candidates are drawn from 179 overdense regions of $g$-dropout galaxies at $z\sim4$ from the Hyper Suprime-Cam ...
Higuchi, Ryo   +15 more
core   +1 more source

LATIS: A Sample of IGM-selected Protoclusters and Protogroups at z ∼ 2.5

open access: yesThe Astrophysical Journal
The Ly α Tomography IMACS Survey (LATIS) has produced large 3D maps of the intergalactic medium (IGM), providing a new window on the cosmic web at z ∼ 2.5.
Andrew B. Newman   +13 more
doaj   +1 more source

A Massive Protocluster Anchored by a Luminous Quasar at z = 6.63

open access: yesThe Astrophysical Journal Letters
Protoclusters, the progenitors of galaxy clusters, trace large scale structures in the early Universe and are important to our understanding of structure formation and galaxy evolution. To date, only a handful of protoclusters have been identified in the
Feige Wang   +15 more
doaj   +1 more source

The Overdense Environments of WISE-Selected, Ultra-Luminous, High-Redshift AGN in the Submillimeter

open access: yesFrontiers in Astronomy and Space Sciences, 2017
The environments around WISE-selected hot dust obscured galaxies (Hot DOGs) and WISE/radio-selected active galactic nuclei (AGNs) at average redshifts of z = 2.7 and z = 1.7, respectively, were found to have overdensities of companion Submillimeter ...
Suzy F. Jones
doaj   +1 more source

Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation

open access: yesThe Astrophysical Journal
We use the TNG-Cluster simulation to investigate how stellar mass and star formation rate (SFR) incompleteness affect the identification of density peaks within galaxy protoclusters at different redshifts.
Devontae C. Baxter   +9 more
doaj   +1 more source

Properties of Ly-alpha emitters around the radio galaxy MRC 0316-257

open access: yes, 2005
Observations of the radio galaxy MRC 0316-257 at z=3.13 and the surrounding field are presented. Using narrow- and broad-band imaging obtained with the VLT, 77 candidate Ly-alpha emitters with a rest-frame equivalent width of > 15 A were selected in a ~7'
Adelberger   +115 more
core   +1 more source

ADF22-WEB: ALMA and JWST (Sub)kiloparsec-scale Views of Dusty Star-forming Galaxies in a z ≈ 3 Protocluster

open access: yesThe Astrophysical Journal
We present a morphological analysis of Atacama Large Millimeter/submillimeter Array (ALMA) and James Webb Space Telescope (JWST) NIRCam images of nine dusty star-forming galaxies (DSFGs) at z _spec  ≈ 3.09, all embedded within the cosmic web filaments at
Hideki Umehata   +6 more
doaj   +1 more source

The HST-Hyperion Survey: Grism Observations of a z ∼ 2.5 Protosupercluster

open access: yesThe Astrophysical Journal
We present the first results and catalogs from the HST-Hyperion survey. This survey has collected 50 orbits of WFC3/F160W imaging and WFC3/G141 grism spectroscopy in the most overdense regions of the Hyperion protosupercluster at z  ∼ 2.45, which are ...
Ben Forrest   +21 more
doaj   +1 more source

ALMA High-resolution Spectral Survey of Thioformaldehyde (H2CS) toward Massive Protoclusters

open access: yesThe Astrophysical Journal
Investigating the temperature and density structures of gas in massive protoclusters is crucial for understanding the chemical properties therein. In this study, we present observations of the continuum and thioformaldehyde (H _2 CS) lines at 345 GHz of ...
Li Chen   +14 more
doaj   +1 more source

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