De re metallica: the cosmic chemical evolution of galaxies

R Maiolino, F Mannucci - The Astronomy and Astrophysics Review, 2019 - Springer
The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

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 …

The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8

M Curti, F d'Eugenio, S Carniani… - Monthly Notices of …, 2023 - academic.oup.com
We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster
SMACS J0723. 3-7327, observed as part of the Early Release Observations programme of …

GA-NIFS: A massive black hole in a low-metallicity AGN at z∼ 5.55 revealed by JWST/NIRSpec IFS

H Übler, R Maiolino, E Curtis-Lake… - Astronomy & …, 2023 - aanda.org
We present rest-frame optical data of the compact z= 5.55 galaxy GS_3073 obtained using
the integral field spectroscopy mode of the Near-InfraRed Spectrograph on board the James …

JWST/NIRSpec spectroscopy of z = 7–9 star-forming galaxies with CEERS: new insight into bright Lyα emitters in ionized bubbles

M Tang, DP Stark, Z Chen, C Mason… - Monthly Notices of …, 2023 - academic.oup.com
We describe new JWST/NIRSpec observations of galaxies at z≳ 7 taken from the CEERS
survey. Previous observations of this area have revealed associations of Lyα emitters at …

JADES: Probing interstellar medium conditions at z∼ 5.5–9.5 with ultra-deep JWST/NIRSpec spectroscopy

AJ Cameron, A Saxena, AJ Bunker… - Astronomy & …, 2023 - aanda.org
We present emission-line ratios from a sample of 27 Lyman-break galaxies from z∼ 5.5− 9.5
with− 17.0< M 1500<− 20.4, measured from ultra-deep JWST/NIRSpec multi-object …

The MOSDEF Survey: The Evolution of the Mass–Metallicity Relation from z= 0 to z∼ 3.3

RL Sanders, AE Shapley, T Jones… - The Astrophysical …, 2021 - iopscience.iop.org
We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z= 0–3.3
using samples of∼ 300 galaxies at z∼ 2.3 and∼ 150 galaxies at z∼ 3.3 from the MOSDEF …

GA-NIFS: The ultra-dense, interacting environment of a dual AGN at z∼ 3.3 revealed by JWST/NIRSpec IFS

M Perna, S Arribas, M Marshall, F D'Eugenio… - Astronomy & …, 2023 - aanda.org
Context. LBQS 0302− 0019 is a blue quasar (QSO) at z∼ 3.3 that hosts powerful outflows
and resides in a complex environment consisting of an obscured active galactic nucleus …

Direct T e-based metallicities of z= 2–9 galaxies with JWST/NIRSpec: empirical metallicity calibrations applicable from reionization to cosmic noon

RL Sanders, AE Shapley, MW Top**… - The Astrophysical …, 2024 - iopscience.iop.org
We report detections of the [O iii] λ4364 auroral emission line for 16 galaxies at z= 2.1–8.7,
measured from JWST/NIRSpec observations obtained as part of the Cosmic Evolution Early …

The physical conditions of emission-line galaxies at cosmic dawn from JWST/NIRSpec spectroscopy in the SMACS 0723 early release observations

JR Trump, PA Haro, RC Simons… - The Astrophysical …, 2023 - iopscience.iop.org
We present rest-frame optical emission-line flux ratio measurements for five z> 5 galaxies
observed by the James Webb Space Telescope Near-Infared Spectrograph (NIRSpec) in …