Early results from GLASS-JWST. XIX. A high density of bright galaxies at z≈ 10 in the A2744 region

M Castellano, A Fontana, T Treu, E Merlin… - The Astrophysical …, 2023 - iopscience.iop.org
We report the detection of a high density of redshift z≈ 10 galaxies behind the foreground
cluster A2744, selected from imaging data obtained recently with NIRCam on board JWST …

Seen and unseen: bursty star formation and its implications for observations of high-redshift galaxies with JWST

G Sun, CA Faucher-Giguère… - Monthly Notices of the …, 2023 - academic.oup.com
Both observations and simulations have shown strong evidence for highly time-variable star
formation in low-mass and/or high-redshift galaxies, which has important observational …

Blue monsters. Why are JWST super-early, massive galaxies so blue?

F Ziparo, A Ferrara, L Sommovigo… - Monthly Notices of the …, 2023 - academic.oup.com
ABSTRACT The recent James Webb Space Telescope tentative discovery of a population of
super-early (redshift z> 10), relatively massive (stellar mass M*= 108–109M⊙) and evolved …

Spatially resolved Kennicutt–Schmidt relation at z ≈ 7 and its connection with the interstellar medium properties

L Vallini, J Witstok, L Sommovigo… - Monthly Notices of …, 2024 - academic.oup.com
We exploit moderately resolved [O],[C] and dust continuum ALMA observations to derive the
gas density (n), the gas-phase metallicity (Z), and the deviation from the Kennicutt–Schmidt …

JWST and ALMA Multiple-line Study in and around a Galaxy at z= 8.496: Optical to Far-Infrared Line Ratios and the Onset of an Outflow Promoting Ionizing Photon …

S Fujimoto, M Ouchi, K Nakajima… - The Astrophysical …, 2024 - iopscience.iop.org
JWST and ALMA Multiple-line Study in and around a Galaxy at z = 8.496: Optical to Far-Infrared
Line Ratios and the Onset of an Outflow Promoting Ionizing Photon Escape - IOPscience Skip …

ALMA Observation of az≳ 10 Galaxy Candidate Discovered with JWST

I Yoon, CL Carilli, S Fujimoto… - The Astrophysical …, 2023 - iopscience.iop.org
We report the observation by the Atacama Large Millimeter/submillimeter Array (ALMA) of
az≳ 10 galaxy candidate (GHZ1) discovered from the GLASS–JWST Early Release Science …

ALMA Detection of [O III] 88 μm at z= 12.33: Exploring the Nature and Evolution of GHZ2 as a Massive Compact Stellar System

JA Zavala, T Bakx, I Mitsuhashi… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract We present Atacama Large Millimeter/submillimeter Array observations on the high-
redshift galaxy GHZ2 and report a successful detection of the rest-frame 88 μm atomic …

To see or not to see az∼ 13 galaxy, that is the question-Targeting the [C II] 158 μm emission line of HD1 with ALMA

M Kaasinen, J van Marrewijk, G Popping… - Astronomy & …, 2023 - aanda.org
Context. Determining when the first galaxies formed remains an outstanding goal of modern
observational astronomy. Theory and current stellar population models imply that the first …

Simulations of High-redshift [O iii] Emitters: Chemical Evolution and Multiline Diagnostics

Y Nakazato, N Yoshida, D Ceverino - The Astrophysical Journal, 2023 - iopscience.iop.org
Recent observations by the James Webb Space Telescope discovered a number of high-
redshift galaxies with strong emission lines from doubly ionized oxygen. Combined with …

Detection of [OIII]88m in JADES-GS-z14-0 at z=14.1793

S Schouws, RJ Bouwens, K Ormerod, R Smit… - arXiv preprint arXiv …, 2024 - arxiv.org
We report the first successful ALMA follow-up observations of a secure $ z> 10$ JWST-
selected galaxy, by robustly detecting ($6.6\sigma $) the [OIII] $ _ {88\mu m}\, $ line in …