Search Publications

A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields
DOI: 10.3847/1538-4357/ad4265 Bibcode: 2024ApJ...968...38K

Labbé, Ivo; Fujimoto, Seiji; Trebitsch, Maxime +9 more

Observations with the James Webb Space Telescope (JWST) have uncovered numerous faint active galactic nuclei (AGN) at z ∼ 5 and beyond. These objects are key to our understanding of the formation of supermassive black holes (SMBHs), their coevolution with host galaxies, as well as the role of AGN in cosmic reionization. Using photometric colors an…

2024 The Astrophysical Journal
Gaia eHST JWST 123
Extremely Red Galaxies at z = 5–9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?
DOI: 10.3847/1538-4357/ad167e Bibcode: 2024ApJ...963..128B

Papovich, Casey; Yang, Guang; Barro, Guillermo +31 more

We study a new population of extremely red objects (EROs) recently discovered by the James Webb Space Telescope (JWST) based on their NIRCam colors F277W ‑ F444W > 1.5 mag. We find 37 EROs in the Cosmic Evolution Early Release Science Survey (CEERS) field with F444W < 28 mag and photometric redshifts between 5 < z < 7, with median $z={…

2024 The Astrophysical Journal
Gaia eHST JWST 120
What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition
DOI: 10.3847/1538-4357/ad38bb Bibcode: 2024ApJ...968....4P

Barro, Guillermo; Pérez-González, Pablo G.; Bunker, Andrew J. +20 more

We study 31 little red dots (LRD) detected by JADES/NIRCam and covered by the SMILES/MIRI survey, of which ∼70% are detected in the two bluest MIRI bands and 40% in redder MIRI filters. The median/quartiles redshifts are z=6.9

2024 The Astrophysical Journal
eHST JWST 117
A recently quenched galaxy 700 million years after the Big Bang
DOI: 10.1038/s41586-024-07227-0 Bibcode: 2024Natur.629...53L

Chevallard, Jacopo; Maseda, Michael V.; Carniani, Stefano +42 more

Local and low-redshift (z < 3) galaxies are known to broadly follow a bimodal distribution: actively star-forming galaxies with relatively stable star-formation rates and passive systems. These two populations are connected by galaxies in relatively slow transition. By contrast, theory predicts that star formation was stochastic at early cosmic…

2024 Nature
JWST 116
JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34
DOI: 10.3847/1538-4357/ad5f88 Bibcode: 2024ApJ...972..143C

Santini, Paola; Arrabal Haro, Pablo; Calabrò, Antonello +28 more

We spectroscopically confirm the M UV = ‑20.5 mag galaxy GHZ2/GLASS-z12 to be at redshift z = 12.34. The source was selected via NIRCam photometry in GLASS-JWST Early Release Science data, providing the first evidence of a surprising abundance of bright galaxies at z ≳ 10. The NIRSpec PRISM spectrum shows detections of N IV, C IV, He II…

2024 The Astrophysical Journal
JWST 113
The galaxy UV luminosity function at z ≃ 11 from a suite of public JWST ERS, ERO, and Cycle-1 programs
DOI: 10.1093/mnras/stad3471 Bibcode: 2024MNRAS.527.5004M

Cullen, F.; McLure, R. J.; Dunlop, J. S. +8 more

We present a new determination of the evolving galaxy ultraviolet (UV) luminosity function (LF) over the redshift range 9.5 < z < 12.5 based on a wide-area (>250 arcmin2) data set of JWST NIRCam near-infrared imaging assembled from 13 public JWST surveys. Our relatively large-area search allows us to uncover a sample of 61 robu…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 110
EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin2 of Deep, Blank Fields from the PEARLS Survey and Public JWST Data
DOI: 10.3847/1538-4357/ad2a7b Bibcode: 2024ApJ...965..169A

Grogin, Norman A.; Hathi, Nimish P.; Koekemoer, Anton M. +34 more

We present an analysis of the ultraviolet luminosity function (UV LF) and star formation rate density of distant galaxies (7.5 < z < 13.5) in the "blank" fields of the Prime Extragalactic Areas for Reionization and Lensing Science (PEARLS) survey combined with Early Release Science data from the CEERS, GLASS, and NGDEEP surveys/fields and th…

2024 The Astrophysical Journal
Gaia eHST JWST 108
The Galaxies Missed by Hubble and ALMA: The Contribution of Extremely Red Galaxies to the Cosmic Census at 3 < z < 8
DOI: 10.3847/1538-4357/ad3f17 Bibcode: 2024ApJ...968...34W

Pérez-González, Pablo G.; Maseda, Michael V.; Carniani, Stefano +35 more

Using deep JWST imaging from JADES, JEMS, and SMILES, we characterize optically faint and extremely red galaxies at z > 3 that were previously missing from galaxy census estimates. The data indicate the existence of abundant, dusty, and poststarburst-like galaxies down to 108 M , below the sensitivity limit of Spitzer an…

2024 The Astrophysical Journal
eHST JWST 103
Ionised gas kinematics and dynamical masses of z ≳ 6 galaxies from JADES/NIRSpec high-resolution spectroscopy
DOI: 10.1051/0004-6361/202347755 Bibcode: 2024A&A...684A..87D

Charlot, Stéphane; Chevallard, Jacopo; Maseda, Michael V. +28 more

We explore the kinematic gas properties of six 5.5 < z < 7.4 galaxies in the JWST Advanced Deep Extragalactic Survey (JADES), using high-resolution JWST/NIRSpec multi-object spectroscopy of the rest-frame optical emission lines [OIII] and Hα. The objects are small and of low stellar mass (∼1 kpc; M* ∼ 107 − 9 M

2024 Astronomy and Astrophysics
JWST 102
An Updated Mass-Radius Analysis of the 2017-2018 NICER Data Set of PSR J0030+0451
DOI: 10.3847/1538-4357/acfb83 Bibcode: 2024ApJ...961...62V

Chakrabarty, Deepto; Bogdanov, Slavko; Salmi, Tuomo +12 more

In 2019 the NICER collaboration published the first mass and radius inferred for PSR J0030+0451, thanks to NICER observations, and consequent constraints on the equation of state characterizing dense matter. Two independent analyses found a mass of ~1.3-1.4 M and a radius of ~13 km. They also both found that the hot spots were all loc…

2024 The Astrophysical Journal
XMM-Newton 102