Search Publications

JWST Measurements of Neutral Hydrogen Fractions and Ionized Bubble Sizes at z = 7–12 Obtained with Lyα Damping Wing Absorptions in 27 Bright Continuum Galaxies
DOI: 10.3847/1538-4357/ad554e Bibcode: 2024ApJ...971..124U

Ono, Yoshiaki; Ouchi, Masami; Harikane, Yuichi +5 more

We present volume-averaged neutral hydrogen fractions x H I and ionized bubble radii R b measured with Lyα damping wing absorption of galaxies at the epoch of reionization. We combine JWST/NIRSpec spectra taken by the CEERS, GO-1433, DDT-2750, and JADES programs and obtain a sample containing 27 bright UV-continuum (M UV…

2024 The Astrophysical Journal
JWST 92
Strong damped Lyman-α absorption in young star-forming galaxies at redshifts 9 to 11
DOI: 10.1126/science.adj0343 Bibcode: 2024Sci...384..890H

Finkelstein, Steven L.; Arrabal Haro, Pablo; Heintz, Kasper E. +18 more

Primordial neutral atomic gas, mostly composed of hydrogen, is the raw material for star formation in galaxies. However, there are few direct constraints on the amount of neutral atomic hydrogen (H I) in galaxies at early cosmic times. We analyzed James Webb Space Telescope (JWST) near-infrared spectroscopy of distant galaxies, at redshifts ≳8. Fr…

2024 Science
Gaia JWST 91
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr after the Big Bang
DOI: 10.3847/1538-4357/ad463d Bibcode: 2024ApJ...970...31R

Pérez-González, Pablo G.; Chevallard, Jacopo; Maseda, Michael V. +33 more

We characterize the earliest galaxy population in the JADES Origins Field, the deepest imaging field observed with JWST. We make use of ancillary Hubble Space Telescope optical images (five filters spanning 0.4–0.9 µm) and novel JWST images with 14 filters spanning 0.8‑5 µm, including seven medium-band filters, and reaching total expos…

2024 The Astrophysical Journal
Gaia eHST JWST 90
Nebular dominated galaxies: insights into the stellar initial mass function at high redshift
DOI: 10.1093/mnras/stae1547 Bibcode: 2024MNRAS.534..523C

Bunker, Andrew J.; Cameron, Alex J.; Saxena, Aayush +3 more

We identify a low-metallicity ($12+\log ({\rm O}/{\rm H})=7.59$) Ly $\alpha$-emitting galaxy at $z=5.943$

2024 Monthly Notices of the Royal Astronomical Society
JWST 90
ULTRASAT: A Wide-field Time-domain UV Space Telescope
DOI: 10.3847/1538-4357/ad2704 Bibcode: 2024ApJ...964...74S

Mazeh, T.; Gal-Yam, A.; Tal-Or, L. +41 more

The Ultraviolet Transient Astronomy Satellite (ULTRASAT) is scheduled to be launched to geostationary orbit in 2027. It will carry a telescope with an unprecedentedly large field of view (204 deg2) and near-ultraviolet (NUV; 230–290 nm) sensitivity (22.5 mag, 5σ, at 900 s). ULTRASAT will conduct the first wide-field survey of transient …

2024 The Astrophysical Journal
Gaia XMM-Newton 89
GN-z11 in Context: Possible Signatures of Globular Cluster Precursors at Redshift 10
DOI: 10.3847/1538-4357/ad235e Bibcode: 2024ApJ...966...92S

Charlot, Stéphane; James, Bethan L.; Mingozzi, Matilde +5 more

The first JWST spectroscopy of the luminous galaxy GN-z11 simultaneously established its redshift at z = 10.6 and revealed a rest-ultraviolet spectrum dominated by signatures of highly ionized nitrogen, which has so far defied clear interpretation. We present a reappraisal of this spectrum in the context of both detailed nebular modeling and nearb…

2024 The Astrophysical Journal
eHST JWST 89
First Detection of an Overmassive Black Hole Galaxy UHZ1: Evidence for Heavy Black Hole Seed Formation from Direct Collapse
DOI: 10.3847/2041-8213/ad0e76 Bibcode: 2024ApJ...960L...1N

Goulding, Andy D.; Natarajan, Priyamvada; Bogdán, Ákos +3 more

The recent Chandra-JWST discovery of a quasar in the z ≈ 10.1 galaxy UHZ1 reveals that accreting supermassive black holes were already in place 470 million years after the Big Bang. The Chandra X-ray source detected in UHZ1 is a Compton-thick quasar with a bolometric luminosity of L bol ~ 5 × 1045 erg s-1, which co…

2024 The Astrophysical Journal
JWST 87
A fast-rotator post-starburst galaxy quenched by supermassive black-hole feedback at z = 3
DOI: 10.1038/s41550-024-02345-1 Bibcode: 2024NatAs...8.1443D

Pérez-González, Pablo G.; Chevallard, Jacopo; Parlanti, Eleonora +23 more

The most massive galaxies in the Universe stopped forming stars due to the time-integrated feedback from central supermassive black holes (SMBHs). However, the exact quenching mechanism is not yet understood, because local massive galaxies were quenched billions of years ago. Here we present JWST/NIRSpec integral-field spectroscopy observations of…

2024 Nature Astronomy
eHST JWST 87
JADES: The production and escape of ionizing photons from faint Lyman-alpha emitters in the epoch of reionization
DOI: 10.1051/0004-6361/202347132 Bibcode: 2024A&A...684A..84S

Chevallard, Jacopo; Carniani, Stefano; Arribas, Santiago +32 more

We present the properties of 17 faint Lyman-α emitting galaxies (LAEs) at z > 5.8 from the JWST Advanced Deep Extragalactic Survey (JADES) spectroscopic data in the Hubble Ultra Deep Field/GOODS-S. These LAEs span a redshift range z ≈ 5.8 − 8.0 and a UV magnitude range MUV ≈ −17 to −20.6, with the Lyα equivalent width (EW) in the ran…

2024 Astronomy and Astrophysics
JWST 87
Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry
DOI: 10.1051/0004-6361/202449763 Bibcode: 2024A&A...686L...2G

Valtchanov, I.; Prusti, T.; Mazeh, T. +413 more

Context. Gravitational waves from black-hole (BH) merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected based on most stellar evolution models - and also higher than known stellar-origin black holes in our Galaxy. It has been proposed that those high-mass BHs are…

2024 Astronomy and Astrophysics
Gaia 86