Search Publications

A JWST investigation into the bar fraction at redshifts 1 ≤ z ≤ 3
DOI: 10.1093/mnras/stae921 Bibcode: 2024MNRAS.530.1984L

Conselice, Christopher J.; Fragkoudi, Francesca; Ferreira, Leonardo +7 more

The presence of a stellar bar in a disc galaxy indicates that the galaxy hosts in its main part a dynamically settled disc and that bar-driven processes are taking place in shaping its evolution. Studying the cosmic evolution of the bar fraction in disc galaxies is therefore essential to understand galaxy evolution in general. Previous studies hav…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 42
Bursty star formation and galaxy-galaxy interactions in low-mass galaxies 1 Gyr after the Big Bang
DOI: 10.1093/mnras/stad3902 Bibcode: 2024MNRAS.52711372A

Willott, Chris J.; Harshan, Anishya; Bradač, Maruša +14 more

We use CANUCS JWST/NIRCam imaging of galaxies behind the gravitationally-lensing cluster MACS J0417.5-1154 to investigate star formation burstiness in low-mass (M ~ 108 M) galaxies at z ~ 4.7-6.5. Our sample of 123 galaxies is selected using the Lyman break selection and photometric emission-line excess methods. …

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 42
JADES + JEMS: A Detailed Look at the Buildup of Central Stellar Cores and Suppression of Star Formation in Galaxies at Redshifts 3 < z < 4.5
DOI: 10.3847/1538-4357/ad6e7f Bibcode: 2024ApJ...974..135J

Chevallard, Jacopo; Maseda, Michael V.; Carniani, Stefano +30 more

We present a spatially resolved study of stellar populations in six galaxies with stellar masses M * ∼ 1010 M at z ∼ 3.7 using 14-filter James Webb Space Telescope (JWST)/NIRCam imaging from the JADES and JEMS surveys. The six galaxies are visually selected to have clumpy substructures with distinct colors over r…

2024 The Astrophysical Journal
Gaia eHST JWST 42
White dwarfs as a probe of exceptionally light QCD axions
DOI: 10.1103/PhysRevD.109.095032 Bibcode: 2024PhRvD.109i5032B

Balkin, Reuven; Serra, Javi; Springmann, Konstantin +2 more

We study the effects of exceptionally light QCD axions on the stellar configuration of white dwarfs. At finite baryon density, the nonderivative coupling of the axion to nucleons displaces the axion from its in-vacuum minimum, which implies a reduction of the nucleon mass. This dramatically alters the composition of stellar remnants. In particular…

2024 Physical Review D
Gaia 42
Size–Stellar Mass Relation and Morphology of Quiescent Galaxies at z ≥ 3 in Public JWST Fields
DOI: 10.3847/1538-4357/ad2512 Bibcode: 2024ApJ...964..192I

Heintz, Kasper E.; Brammer, Gabriel; Ilbert, Olivier +19 more

We present the results of a systematic study of the rest-frame optical morphology of quiescent galaxies at z ≥ 3 using the Near-Infrared Camera (NIRCam) on board the James Webb Space Telescope (JWST). Based on a sample selected by UVJ color or NUVUVJ color, we focus on 26 quiescent galaxies with $9.8\lt \mathrm{log}({M}_{\star }/{M}_{\odot })\lt 1…

2024 The Astrophysical Journal
eHST JWST 41
A high internal heat flux and large core in a warm Neptune exoplanet
DOI: 10.1038/s41586-024-07514-w Bibcode: 2024Natur.630..836W

Fortney, Jonathan J.; McGill, Peter; Bell, Taylor J. +16 more

Interactions between exoplanetary atmospheres and internal properties have long been proposed to be drivers of the inflation mechanisms of gaseous planets and apparent atmospheric chemical disequilibrium conditions1. However, transmission spectra of exoplanets have been limited in their ability to observationally confirm these theories …

2024 Nature
eHST JWST 41
Unveiling the Distant Universe: Characterizing z ≥ 9 Galaxies in the First Epoch of COSMOS-Web
DOI: 10.3847/1538-4357/ad5e6a Bibcode: 2024ApJ...973...23F

Finkelstein, Steven L.; Bagley, Micaela B.; Casey, Caitlin M. +48 more

We report the identification of 15 galaxy candidates at z ≥ 9 using the initial COSMOS-Web JWST observations over 77 arcmin2 through four Near Infrared Camera filters (F115W, F150W, F277W, and F444W) with an overlap with the Mid-Infrared Imager (F770W) of 8.7 arcmin2. We fit the sample using several publicly available spectra…

2024 The Astrophysical Journal
Gaia eHST JWST 40
EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4–10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models
DOI: 10.3847/1538-4357/ad13ff Bibcode: 2024ApJ...962...50W

Ono, Yoshiaki; Ouchi, Masami; Harikane, Yuichi +14 more

We present gas-phase elemental abundance ratios of thirteen local extremely metal-poor galaxies (EMPGs), including our new Keck/LRIS spectroscopy determinations together with 33 James Webb Space Telescope z ∼ 4–10 star-forming galaxies in the literature, and compare chemical evolution models. We develop chemical evolution models with the yields of…

2024 The Astrophysical Journal
JWST 40
Building the First Galaxies—Chapter 2. Starbursts Dominate the Star Formation Histories of 6 < z < 12 Galaxies
DOI: 10.3847/1538-4357/ad1923 Bibcode: 2024ApJ...964..150D

Carniani, Stefano; Bunker, Andrew J.; Stark, Daniel P. +12 more

We use SEDz*—a code designed to chart the star formation histories (SFHs) of 6 < z < 12 galaxies—to analyze the spectral energy distributions (SEDs) of 894 galaxies with deep JWST/NIRCam imaging by JADES in the GOODS-S field. We show how SEDz* matches observed SEDs using stellar-population templates, graphing the contribution of each epoch b…

2024 The Astrophysical Journal
JWST 40
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
DOI: 10.1038/s41550-024-02230-x Bibcode: 2024NatAs...8..879B

Carter, Aarynn L.; Gibson, Neale P.; Helling, Christiane +80 more

Hot Jupiters are among the best-studied exoplanets, but it is still poorly understood how their chemical composition and cloud properties vary with longitude. Theoretical models predict that clouds may condense on the nightside and that molecular abundances can be driven out of equilibrium by zonal winds. Here we report a phase-resolved emission s…

2024 Nature Astronomy
JWST 40