Star-forming galaxies at cosmic noon
NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …
star-formation history, which culminated around; this period is often nicknamed “cosmic …
Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
M Magliocchetti - The Astronomy and Astrophysics Review, 2022 - Springer
Despite their relative sparseness, during the recent years it has become more and more
clear that extragalactic radio sources (both AGN and star-forming galaxies) constitute an …
clear that extragalactic radio sources (both AGN and star-forming galaxies) constitute an …
The LOFAR Two-metre Sky Survey: Deep Fields data release 1. V. Survey description, source classifications, and host galaxy properties
PN Best, R Kondapally, WL Williams… - Monthly Notices of …, 2023 - academic.oup.com
Source classifications, stellar masses, and star-formation rates are presented for≈ 80 000
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …
A dusty compact object bridging galaxies and quasars at cosmic dawn
Understanding how super-massive black holes form and grow in the early Universe has
become a major challenge, since it was discovered that luminous quasars existed only 700 …
become a major challenge, since it was discovered that luminous quasars existed only 700 …
The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to z∼ 5
The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
Map** Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies
CM Casey, JA Zavala, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
“Super-deblended” Dust Emission in Galaxies. II. Far-IR to (Sub) millimeter Photometry and High-redshift Galaxy Candidates in the Full COSMOS Field
We present a" super-deblended" far-infrared (FIR) to (sub) millimeter photometric catalog in
the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by …
the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by …
The infrared-radio correlation of star-forming galaxies is strongly M⋆-dependent but nearly redshift-invariant since z∼ 4
Over the past decade, several works have used the ratio between total (rest 8− 1000 μm)
infrared and radio (rest 1.4 GHz) luminosity in star-forming galaxies (q IR), often referred to …
infrared and radio (rest 1.4 GHz) luminosity in star-forming galaxies (q IR), often referred to …
Prevalence of radio jets associated with galactic outflows and feedback from quasars
Abstract We present 1–7 GHz high-resolution radio imaging (VLA and e-MERLIN) and
spatially resolved ionized gas kinematics for 10 z< 0.2 type 2 'obscured'quasars (log [L …
spatially resolved ionized gas kinematics for 10 z< 0.2 type 2 'obscured'quasars (log [L …
The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population
We study the composition of the faint radio population selected from the Karl G. Jansky Very
Large Array Cosmic Evolution Survey (VLA-COSMOS) 3 GHz Large Project, which is a radio …
Large Array Cosmic Evolution Survey (VLA-COSMOS) 3 GHz Large Project, which is a radio …