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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 …
GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with∼ 4,000,000 Galaxies at z∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and …
We present new measurements of rest-UV luminosity functions and angular correlation
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
Euclid. I. Overview of the Euclid mission
Y Mellier, A Abdurroúf, JAA Barroso… - Astronomy & …, 2024 - aanda.org
The current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. is a …
but the nature of its main ingredients, dark matter and dark energy, remains unknown. is a …
Photometric redshifts for Hyper Suprime-Cam Subaru strategic program data release 1
M Tanaka, J Coupon, BC Hsieh, S Mineo… - Publications of the …, 2018 - academic.oup.com
Photometric redshifts are a key component of many science objectives in the Hyper Suprime-
Cam Subaru Strategic Program (HSC-SSP). In this paper, we describe and compare the …
Cam Subaru Strategic Program (HSC-SSP). In this paper, we describe and compare the …
Near infrared spectroscopy and star-formation histories of 3≤ z≤ 4 quiescent galaxies
We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …
The alpine–alma [c ii] survey: Multiwavelength ancillary data and basic physical measurements
We present the ancillary data and basic physical measurements for the galaxies in the
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …
Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z∼ 4–7 derived with the half-million dropouts on the 100 …
We study the UV luminosity functions (LFs) at z∼ 4, 5, 6, and 7 based on the deep large-
area optical images taken by the Hyper Suprime-Cam (HSC) Subaru Strategic Program …
area optical images taken by the Hyper Suprime-Cam (HSC) Subaru Strategic Program …
The ALPINE-ALMA [C II] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe
We study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158
μm emission in a large sample of normal star-forming galaxies at 4< z< 6 from the ALMA …
μm emission in a large sample of normal star-forming galaxies at 4< z< 6 from the ALMA …
“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 …
[HTML][HTML] The VLA-COSMOS 3 GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to z≲ 6
We examine the behaviour of the infrared-radio correlation (IRRC) over the range 0< z≲ 6
using new, highly sensitive 3 GHz observations with the Karl G. Jansky Very Large Array …
using new, highly sensitive 3 GHz observations with the Karl G. Jansky Very Large Array …