The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys

J Schaye, R Kugel, M Schaller, JC Helly… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT We introduce the Virgo Consortium's FLAMINGO suite of hydrodynamical
simulations for cosmology and galaxy cluster physics. To ensure the simulations are …

On the Stellar Populations of Galaxies at z= 9–11: The Growth of Metals and Stellar Mass at Early Times

S Tacchella, SL Finkelstein, M Bagley… - The Astrophysical …, 2022 - iopscience.iop.org
We present a detailed stellar population analysis of 11 bright (H< 26.6) galaxies at z= 9–11
(three spectroscopically confirmed) to constrain the chemical enrichment and growth of …

Dusty starbursts masquerading as ultra-high redshift galaxies in JWST CEERS observations

JA Zavala, V Buat, CM Casey… - The Astrophysical …, 2023 - iopscience.iop.org
Lyman-break galaxy (LBG) candidates at z≳ 10 are rapidly being identified in James Webb
Space Telescope (JWST)/NIRCam observations. Due to the (redshifted) break produced by …

On the ages of bright galaxies ∼500 Myr after the big bang: insights into star formation activity at z ≳ 15 with JWST

L Whitler, R Endsley, DP Stark… - Monthly Notices of …, 2023 - academic.oup.com
With JWST, new opportunities to study the evolution of galaxies in the early Universe are
emerging. Spitzer constraints on rest-optical properties of z≳ 7 galaxies demonstrated the …

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 shaping both the evolution of galaxies and their
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 …

Star formation histories of UV-luminous galaxies at z ≃ 6.8: implications for stellar mass assembly at early cosmic times

L Whitler, DP Stark, R Endsley, J Leja… - Monthly Notices of …, 2023 - academic.oup.com
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 …

The ALMA REBELS Survey: specific star formation rates in the reionization era

MW Topping, DP Stark, R Endsley… - Monthly Notices of …, 2022 - academic.oup.com
We present specific star formation rates (sSFRs) for 40 ultraviolet (UV)-bright galaxies at z∼
7–8 observed as part of the Reionization Era Bright Emission Line Survey (REBELS) …

The dust enrichment of early galaxies in the JWST and ALMA era

V Mauerhofer, P Dayal - Monthly Notices of the Royal …, 2023 - academic.oup.com
Recent observations with the JWST are yielding tantalizing hints of an early population of
massive, bright galaxies at z> 10, with Atacama Large Millimeter/submillimeter Array (ALMA) …

Mapping 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 …