Results 61 to 70 of about 1,021 (168)

ALMA-IMF. XIV. Free–Free Templates Derived from H41α and Ionized Gas Content in 15 Massive Protoclusters

open access: yesThe Astrophysical Journal Supplement Series
We use the H41 α recombination line to create templates of the millimeter free–free emission in the ALMA-IMF continuum maps, which allows us to separate it from dust emission.
Roberto Galván-Madrid   +27 more
doaj   +1 more source

Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at z ≥ 10?

open access: yesThe Astrophysical Journal Letters, 2023
Recent photometric detections of extreme ( z > 10) redshift galaxies from the JWST have been shown to be in strong tension with existing simulation models for galaxy formation and in the most acute case, in tension with ΛCDM itself.
B. W. Keller   +3 more
doaj   +1 more source

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

MeerKAT observations of Herschel protocluster candidates

open access: yesMonthly Notices of the Royal Astronomical Society
ABSTRACT High-redshift protoclusters consisting of dusty starbursts are thought to play an important role in galaxy evolution. Their dusty nature makes them bright in the far-infrared (FIR)/submm but difficult to find in optical/near-infrared (NIR) surveys.
Y Ding   +11 more
openaire   +2 more sources

The Young and the Wild: What happens to Protoclusters forming at z = 4? [PDF]

open access: yes, 2022
Using one of the largest volumes of the hydrodynamical cosmological simulation suit Magneticum, we study the evolution of protoclusters identified at redshift = 4, with properties similar to SPT2349-56.
Dannerbauer, Helmut   +2 more
core   +1 more source

Searching for the shadows of giants: characterizing protoclusters with line of sight Lyman-α absorption [PDF]

open access: yes, 2019
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We use state-of-the-art hydrodyamical simulations from the Sherwood, EAGLE, and Illustris projects to examine the signature of Mz = 0 ≃ 1014 M ...
Hatch, Nina   +2 more
core   +1 more source

Monte Carlo simulations of galaxy protoclusters in Cosmos Survey [PDF]

open access: yes, 2015
Jata tj. skupovi galaksija su veliki virializirani skupovi galaksija. Galaksije doprinose oko 5% mase jata, unutar-klasterski medij oko 10% mase i tamna tvar do 85% mase. Te strukture su nastale iz protojata galaksija.
Tomičić, Neven
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

ODIN: Confirmation and 3D Reconstruction of Six Massive Protoclusters at Cosmic Noon

open access: yesThe Astrophysical Journal
Protoclusters represent sites of accelerated galaxy formation and extreme astrophysical activity characteristic of dense environments. Identifying massive protoclusters and mapping their spatial structures are therefore crucial for understanding how ...
Ashley Ortiz   +66 more
doaj   +1 more source

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