Search Publications

Gas-phase metallicity gradients in galaxies at z ∼ 6–8
DOI: 10.1051/0004-6361/202449855 Bibcode: 2024A&A...691A..19V

Maiolino, R.; Castellano, M.; Pentericci, L. +18 more

The study of gas-phase metallicity and its spatial distribution at high redshift is crucial to understand the processes that shaped the growth and evolution of galaxies in the early Universe. Here we study the spatially resolved metallicity in three systems at z ∼ 6 ‑ 8, namely A2744-YD4, BDF-3299, and COSMOS24108, with JWST NIRSpec IFU low-resolu…

2024 Astronomy and Astrophysics
JWST 36
JADES: The emergence and evolution of Lyα emission and constraints on the intergalactic medium neutral fraction
DOI: 10.1051/0004-6361/202347099 Bibcode: 2024A&A...683A.238J

Chevallard, Jacopo; Maseda, Michael V.; Parlanti, Eleonora +32 more

The rest-frame UV recombination emission line Lyα can be powered by ionising photons from young massive stars in star-forming galaxies, but the fact that it can be resonantly scattered by neutral gas complicates its interpretation. For reionisation-era galaxies, a neutral intergalactic medium will scatter Lyα from the line of sight, making Lyα a u…

2024 Astronomy and Astrophysics
JWST 36
The SARAO MeerKAT 1.3 GHz Galactic Plane Survey
DOI: 10.1093/mnras/stae1166 Bibcode: 2024MNRAS.531..649G

Umana, G.; Heywood, I.; Camilo, F. +127 more

We present the SARAO MeerKAT Galactic Plane Survey (SMGPS), a 1.3 GHz continuum survey of almost half of the Galactic Plane (251° ≤l ≤ 358° and 2° ≤l ≤ 61° at |b| ≤ $1{_{.}^{\circ}}5$). SMGPS is the largest, most sensitive, and highest angular resolution 1 GHz survey of the plane yet carried out, with an angular resolution of 8 arcsec and a broad-…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 36
Medium Bands, Mega Science: A JWST/NIRCam Medium-band Imaging Survey of A2744
DOI: 10.3847/1538-4357/ad75fe Bibcode: 2024ApJ...976..101S

Maseda, Michael V.; Franx, Marijn; Muzzin, Adam +40 more

In this paper, we describe the "Medium Bands, Mega Science" JWST Cycle 2 survey (JWST-GO-4111) and demonstrate the power of these data to reveal both the spatially integrated and spatially resolved properties of galaxies from the local Universe to the era of cosmic dawn. Executed in 2023 November, MegaScience obtained ∼30 arcmin2 of dee…

2024 The Astrophysical Journal
eHST JWST 36
Quasi-periodic X-ray eruptions years after a nearby tidal disruption event
DOI: 10.1038/s41586-024-08023-6 Bibcode: 2024Natur.634..804N

Berger, E.; Angus, C. R.; Dhillon, V. S. +61 more

Quasi-periodic eruptions (QPEs) are luminous bursts of soft X-rays from the nuclei of galaxies, repeating on timescales of hours to weeks1–5. The mechanism behind these rare systems is uncertain, but most theories involve accretion disks around supermassive black holes (SMBHs) undergoing instabilities6–8 or interacting with a…

2024 Nature
eHST 35
The Discovery of the Faintest Known Milky Way Satellite Using UNIONS
DOI: 10.3847/1538-4357/ad0d9f Bibcode: 2024ApJ...961...92S

Smith, Simon E. T.; Cerny, William; Hayes, Christian R. +14 more

We present the discovery of Ursa Major III/UNIONS 1, the least luminous known satellite of the Milky Way, which is estimated to have an absolute V-band magnitude of $+{2.2}_{-0.3}^{+0.4}$ mag, equivalent to a total stellar mass of ${16}_{-5}^{+6}$ M . Ursa Major III/UNIONS 1 was uncovered in the deep, wide-field Ultraviolet Near Infrar…

2024 The Astrophysical Journal
Gaia 35
EIGER. VI. The Correlation Function, Host Halo Mass, and Duty Cycle of Luminous Quasars at z ≳ 6
DOI: 10.3847/1538-4357/ad778b Bibcode: 2024ApJ...974..275E

Hennawi, Joseph F.; Simcoe, Robert A.; Naidu, Rohan P. +13 more

We expect luminous (M 1450 ≲ ‑26.5) high-redshift quasars to trace the highest-density peaks in the early Universe. Here, we present observations of four z ≳ 6 quasar fields using JWST/NIRCam in the imaging and wide-field slitless spectroscopy mode and report a wide range in the number of detected [O III]-emitting galaxies in the quasar…

2024 The Astrophysical Journal
JWST 35
Widespread Rapid Quenching at Cosmic Noon Revealed by JWST Deep Spectroscopy
DOI: 10.3847/1538-4357/ad7e15 Bibcode: 2024ApJ...976...72P

Conroy, Charlie; Johnson, Benjamin D.; Belli, Sirio +16 more

Massive quiescent galaxies in the young Universe are expected to be quenched rapidly, but it is unclear whether they all experience starbursts before quenching and what physical mechanism drives rapid quenching. We study 14 massive quiescent galaxies ( log(

2024 The Astrophysical Journal
eHST JWST 35
JADES - the Rosetta stone of JWST-discovered AGN: deciphering the intriguing nature of early AGN
DOI: 10.1093/mnras/stae2367 Bibcode: 2024MNRAS.535..853J

Pérez-González, Pablo G.; Charlot, Stéphane; Parlanti, Eleonora +23 more

JWST has discovered a large population of active galactic nuclei (AGN) at high redshift, which are weak in the X-rays. Here we present the NIRSpec spectrum of the most extreme of these objects, GN-28074, an AGN at $z=2.26$ with prominent hydrogen and He I broad line…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 35
Characterization of JWST NIRCam PSFs and Implications for AGN+host Image Decomposition
DOI: 10.3847/1538-4357/ad1183 Bibcode: 2024ApJ...962..139Z

Shen, Yue; Zhuang, Ming-Yang

We present a detailed analysis of the point-spread function (PSF) of JWST NIRCam imaging in eight filters: F070W, F115W, F150W, F200W, F277W, F356W, F444W, and F480M, using publicly available data. Spatial variations in the PSF FWHM generally decrease with wavelength: the maximum and rms fractional variations are ∼20% and 5% in F070W, reduced to ∼…

2024 The Astrophysical Journal
Gaia JWST 35