Search Publications

To High Redshift and Low Mass: Exploring the Emergence of Quenched Galaxies and Their Environments at 3 < z < 6 in the Ultra-deep JADES MIRI F770W Parallel
DOI: 10.3847/1538-4357/ad66cc Bibcode: 2024ApJ...975...85A

Parlanti, Eleonora; Carniani, Stefano; D'Eugenio, Francesco +25 more

We present the robust selection of high-redshift quiescent galaxies (QG) and poststarburst (PSB) galaxies using ultra-deep NIRCam and MIRI imaging from the JWST Advanced Deep Extragalactic Survey (JADES). At 3 < z < 6, MIRI 7.7 µm imaging provides rest-frame J band, which is commonly used to break the degeneracy between old stellar pop…

2024 The Astrophysical Journal
Gaia eHST JWST 33
Tip of the Red Giant Branch Distances with JWST: An Absolute Calibration in NGC 4258 and First Applications to Type Ia Supernova Hosts
DOI: 10.3847/1538-4357/ad2e0a Bibcode: 2024ApJ...966...89A

Casertano, Stefano; Dolphin, Andrew; Li, Siyang +12 more

The tip of the red giant branch (TRGB) allows for the measurement of precise and accurate distances to nearby galaxies based on the brightest ascent of low-mass red giant branch stars before they undergo the helium flash. With the advent of JWST, there is great promise to utilize the technique to measure galaxy distances out to at least 50 Mpc, si…

2024 The Astrophysical Journal
JWST 31
Robust Evidence for the Breakdown of Standard Gravity at Low Acceleration from Statistically Pure Binaries Free of Hidden Companions
DOI: 10.3847/1538-4357/ad0ed5 Bibcode: 2024ApJ...960..114C

Chae, Kyu-Hyun

It is found that Gaia Data Release 3 binary stars selected with stringent requirements on astrometric measurements and radial velocities naturally satisfy Newtonian dynamics without hidden close companions when the projected separation s ≲ 2 kau, showing that pure binaries can be selected. It is then found that pure binaries selected with the same…

2024 The Astrophysical Journal
Gaia 31
UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at z spec = 3.97
DOI: 10.3847/1538-4357/ad6a18 Bibcode: 2024ApJ...974..145S

Glazebrook, Karl; Nanayakkara, Themiya; van Dokkum, Pieter +28 more

We report the spectroscopic confirmation of a massive ( log(M/M

2024 The Astrophysical Journal
JWST 31
Ionized Gas Kinematics with FRESCO: An Extended, Massive, Rapidly Rotating Galaxy at z = 5.4
DOI: 10.3847/2041-8213/ad7b17 Bibcode: 2024ApJ...976L..27N

Maseda, Michael V.; Übler, Hannah; Bunker, Andrew J. +43 more

With the remarkable sensitivity and resolution of JWST in the infrared, measuring rest-optical kinematics of galaxies at z > 5 has become possible for the first time. This study pilots a new method for measuring galaxy dynamics for highly multiplexed, unbiased samples by combining FRESCO NIRCam grism spectroscopy and JADES medium-band imaging. …

2024 The Astrophysical Journal
JWST 31
Diverse Oxygen Abundance in Early Galaxies Unveiled by Auroral Line Analysis with JWST
DOI: 10.3847/1538-4357/ad5290 Bibcode: 2024ApJ...971...43M

Stiavelli, Massimo; Treu, Tommaso; Trenti, Michele +10 more

We present deep JWST NIRSpec observations in the sight line of MACS J1149.5+2223, a massive cluster of galaxies at z = 0.54. We report the spectroscopic redshift of 28 sources at 3 < z < 9.1, including nine sources with the detection of the

2024 The Astrophysical Journal
eHST JWST 31
Testing EMRI Models for Quasi-periodic Eruptions with 3.5 yr of Monitoring eRO-QPE1
DOI: 10.3847/1538-4357/ad2941 Bibcode: 2024ApJ...965...12C

Remillard, Ronald A.; Maccarone, Thomas J.; Burdge, Kevin B. +13 more

Quasi-periodic eruptions (QPEs) are luminous X-ray outbursts recurring on hour timescales, observed from the nuclei of a growing handful of nearby low-mass galaxies. Their physical origin is still debated, and usually modeled as (a) accretion disk instabilities or (b) interaction of a supermassive black hole (SMBH) with a lower mass companion in a…

2024 The Astrophysical Journal
XMM-Newton 30
Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13
DOI: 10.3847/1538-4357/ad7d03 Bibcode: 2024ApJ...975..178K

Finkelstein, Steven L.; Casey, Caitlin M.; Larson, Rebecca L. +8 more

The James Webb Space Telescope (JWST) has uncovered a ubiquitous population of dust-obscured compact sources at z ≳ 4. Many of these objects exhibit signs of active galactic nucleus (AGN) activity, making their study crucial for understanding the formation of supermassive black holes (SMBHs) and their growth with host galaxies. In this work, we ex…

2024 The Astrophysical Journal
JWST 30
The Three-phase Evolution of the Milky Way
DOI: 10.3847/1538-4357/ad5b60 Bibcode: 2024ApJ...972..112C

Conroy, Charlie; Hernquist, Lars; Li, Jiadong +6 more

We illustrate the formation and evolution of the Milky Way over cosmic time, utilizing a sample of 10 million red giant stars with full chemodynamical information, including metallicities and α-abundances from low-resolution Gaia XP spectra. The evolution of angular momentum as a function of metallicity—a rough proxy for stellar age, particularly …

2024 The Astrophysical Journal
Gaia 30
GJ 367b Is a Dark, Hot, Airless Sub-Earth
DOI: 10.3847/2041-8213/ad1a07 Bibcode: 2024ApJ...961L..44Z

Knutson, Heather A.; Hu, Renyu; Dai, Fei +6 more

We present the mid-infrared (5–12 µm) phase curve of GJ 367b observed by the Mid-Infrared Instrument on the James Webb Space Telescope (JWST). GJ 367b is a hot (T eq = 1370 K), extremely dense (10.2 ± 1.3 g cm‑3) sub-Earth orbiting an M dwarf on a 0.32 day orbit. We measure an eclipse depth of 79 ± 4 ppm, a nightside pl…

2024 The Astrophysical Journal
JWST 29