The Role of Radio Observations in Studies of Infrared-Bright Galaxies: Prospects for a Next-Generation Very Large Array
The bulk of the present-day stellar mass was formed in galaxies when the universe was less than half its current age (i.e., <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>1</mn><mo>≲...
Main Author: | Eric Joseph Murphy |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2022-06-01
|
Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/8/6/329 |
Similar Items
-
A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web
by: Jed McKinney, et al.
Published: (2023-01-01) -
Does the fir-radio correlation evolve with redshift in irregular and disk galaxies?
by: Pavlović M.S.
Published: (2021-01-01) -
Searching for High-<i>z</i> Radio Galaxies with the MGCLS
by: Kenda Knowles, et al.
Published: (2021-11-01) -
What is driving the evolution of the far-infrared radio correlation?
by: Pavlović Marina S., et al.
Published: (2019-01-01) -
Radio-only and Radio-to-far-ultraviolet Spectral Energy Distribution Modeling of 14 ULIRGs: Insights into the Global Properties of Infrared Bright Galaxies
by: Subhrata Dey, et al.
Published: (2024-01-01)