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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 …
Astronomia ex machina: a history, primer and outlook on neural networks in astronomy
In this review, we explore the historical development and future prospects of artificial
intelligence (AI) and deep learning in astronomy. We trace the evolution of connectionism in …
intelligence (AI) and deep learning in astronomy. We trace the evolution of connectionism in …
A comprehensive study of galaxies at z∼ 9–16 found in the early JWST data: ultraviolet luminosity functions and cosmic star formation history at the pre-reionization …
We conduct a comprehensive study on dropout galaxy candidates at z∼ 9–16 using the first
90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by …
90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by …
Normal, dust-obscured galaxies in the epoch of reionization
Y Fudamoto, PA Oesch, S Schouws, M Stefanon… - Nature, 2021 - nature.com
Over the past decades, rest-frame ultraviolet (UV) observations have provided large
samples of UV luminous galaxies at redshift (z) greater than 6 (refs.,–), during the so-called …
samples of UV luminous galaxies at redshift (z) greater than 6 (refs.,–), during the so-called …
The ALMA REBELS Survey: dust continuum detections at z > 6.5
H Inami, HSB Algera, S Schouws… - Monthly Notices of …, 2022 - academic.oup.com
We report 18 dust continuum detections (≥ 3.3 σ) at∼ 88 and 158 out of 49 ultraviolet (UV)-
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …
Star formation histories of UV-luminous galaxies at z ≃ 6.8: implications for stellar mass assembly at early cosmic times
The variety of star formation histories (SFHs) of z≳ 6 galaxies provides important insights
into early star formation, but has been difficult to systematically quantify. Some observations …
into early star formation, but has been difficult to systematically quantify. Some observations …
The hyper suprime-cam software pipeline
J Bosch, R Armstrong, S Bickerton… - Publications of the …, 2018 - academic.oup.com
In this paper, we describe the optical imaging data processing pipeline developed for the
Subaru Telescope's Hyper Suprime-Cam (HSC) instrument. The HSC Pipeline builds on the …
Subaru Telescope's Hyper Suprime-Cam (HSC) instrument. The HSC Pipeline builds on the …
The Frontier Fields: survey design and initial results
What are the faintest distant galaxies we can see with the Hubble Space Telescope (HST)
now, before the launch of the James Webb Space Telescope? This is the challenge taken …
now, before the launch of the James Webb Space Telescope? This is the challenge taken …
UV luminosity functions at redshifts z∼ 4 to z∼ 10: 10,000 galaxies from HST legacy fields
RJ Bouwens, GD Illingworth, PA Oesch… - The Astrophysical …, 2015 - iopscience.iop.org
UV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST
LEGACY FIELDS - IOPscience Skip to content IOP Science home Accessibility Help Search …
LEGACY FIELDS - IOPscience Skip to content IOP Science home Accessibility Help Search …
The ALPINE-ALMA [CII] survey-Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4< z< 6
The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …