Search Publications

Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys
DOI: 10.3847/1538-4357/ad2345 Bibcode: 2024ApJ...963..129M

Maseda, Michael V.; van Dokkum, Pieter; Chisholm, John +25 more

Characterizing the prevalence and properties of faint active galactic nuclei (AGNs) in the early Universe is key for understanding the formation of supermassive black holes (SMBHs) and determining their role in cosmic reionization. We perform a spectroscopic search for broad Hα emitters at z ≈ 4–6 using deep JWST/NIRCam imaging and wide field slit…

2024 The Astrophysical Journal
JWST 346
UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z > 5
DOI: 10.3847/1538-4357/ad1e5f Bibcode: 2024ApJ...964...39G

Papovich, Casey; Maseda, Michael V.; Glazebrook, Karl +33 more

The James Webb Space Telescope is revealing a new population of dust-reddened broad-line active galactic nuclei (AGN) at redshifts z ≳ 5. Here we present deep NIRSpec/Prism spectroscopy from the Cycle 1 Treasury program Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) of 15 AGN candidates selected to be compact,…

2024 The Astrophysical Journal
JWST 266
The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization
DOI: 10.3847/1538-4357/ad66cf Bibcode: 2024ApJ...974...92B

Papovich, Casey; Franx, Marijn; Muzzin, Adam +40 more

In this paper we describe the survey design for the Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program, which executed its early imaging component in 2022 November. The UNCOVER survey includes ultradeep (∼29–30AB) imaging of ∼45 arcmin2 on and around the well-studied A2744 …

2024 The Astrophysical Journal
Gaia eHST JWST 184
Pure Spectroscopic Constraints on UV Luminosity Functions and Cosmic Star Formation History from 25 Galaxies at z spec = 8.61-13.20 Confirmed with JWST/NIRSpec
DOI: 10.3847/1538-4357/ad0b7e Bibcode: 2024ApJ...960...56H

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

We present pure spectroscopic constraints on the UV luminosity functions and cosmic star formation rate (SFR) densities from 25 galaxies at z spec = 8.61-13.20. By reducing the JWST/NIRSpec spectra taken in multiple programs of Early Release Observation, Early Release Science, General Observer, and Director's Discretionary Time observat…

2024 The Astrophysical Journal
JWST 170
The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5–14.5
DOI: 10.3847/2041-8213/ad4495 Bibcode: 2024ApJ...969L...2F

Papovich, Casey; Finkelstein, Steven L.; Pérez-González, Pablo G. +52 more

We present a sample of 88 candidate z ∼ 8.5–14.5 galaxies selected from the completed NIRCam imaging from the Cosmic Evolution Early Release Science survey. These data cover ∼90 arcmin2 (10 NIRCam pointings) in six broadband imaging filters and one medium-band imaging filter. With this sample we confirm at higher confidence early JWST c…

2024 The Astrophysical Journal
eHST JWST 154
Direct T e-based Metallicities of z = 2–9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon
DOI: 10.3847/1538-4357/ad15fc Bibcode: 2024ApJ...962...24S

Shapley, Alice E.; Reddy, Naveen A.; Sanders, Ryan L. +2 more

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 Release Science (CEERS) survey program. We combine this CEERS sample with 9 objects from the literature at z = 4‑9 with auroral-line detections from JWST/NIRSpec and 2…

2024 The Astrophysical Journal
eHST JWST 142
The Cosmos in Its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N
DOI: 10.3847/1538-4357/ad1ee4 Bibcode: 2024ApJ...964...71H

Chevallard, Jacopo; Carniani, Stefano; D'Eugenio, Francesco +43 more

We present a catalog of 717 candidate galaxies at z > 8 selected from 125 square arcmin of NIRCam imaging as part of the JWST Advanced Deep Extragalactic Survey (JADES). We combine the full JADES imaging data set with data from the JWST Extragalactic Medium Survey and First Reionization Epoch Spectroscopic COmplete Survey (FRESCO) along with ex…

2024 The Astrophysical Journal
Gaia eHST JWST 131
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