Reionization era bright emission line survey: selection and characterization of luminous interstellar medium reservoirs in the z> 6.5 Universe
RJ Bouwens, R Smit, S Schouws… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …
Large Program (LP) that is identifying and performing a first characterization of many of the …
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 …
A survey of high-z galaxies: serra simulations
We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
The ALMA REBELS survey: the dust content of z ∼ 7 Lyman break galaxies
We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-
analytic model of galaxy formation to explain the dust content of 13 Lyman break galaxies …
analytic model of galaxy formation to explain the dust content of 13 Lyman break galaxies …
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 …
A search for h-dropout lyman break galaxies at z∼ 12–16
We present two bright galaxy candidates at z∼ 12–13 identified in our H-dropout Lyman
break selection with 2.3 deg 2 near-infrared deep imaging data. These galaxy candidates …
break selection with 2.3 deg 2 near-infrared deep imaging data. These galaxy candidates …
The evolution of the IR luminosity function and dust-obscured star formation over the past 13 billion years
JA Zavala, CM Casey, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the first results from the Map** Obscuration to Reionization with ALMA
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …
Bursty star formation naturally explains the abundance of bright galaxies at cosmic dawn
G Sun, CA Faucher-Giguère… - The Astrophysical …, 2023 - iopscience.iop.org
Recent discoveries of a significant population of bright galaxies at cosmic dawn $\left
(z\gtrsim 10\right) $ have enabled critical tests of cosmological galaxy formation models. In …
(z\gtrsim 10\right) $ have enabled critical tests of cosmological galaxy formation models. In …
The ALMA REBELS survey: the dust-obscured cosmic star formation rate density at redshift 7
HSB Algera, H Inami, PA Oesch… - Monthly Notices of …, 2023 - academic.oup.com
Cosmic dust is an essential component sha** both the evolution of galaxies and their
observational signatures. How quickly dust builds up in the early Universe remains an open …
observational signatures. How quickly dust builds up in the early Universe remains an open …
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 …