Search Publications

Environmental Effects on the Stellar Mass Function in a z ∼ 3.3 Overdensity of Galaxies in the COSMOS Field
DOI: 10.3847/1538-4357/ad5e78 Bibcode: 2024ApJ...971..169F

Cooper, M. C.; Urbano Stawinski, Stephanie M.; Hathi, Nimish +17 more

We present an analysis of the number density of galaxies as a function of stellar mass (i.e., the stellar mass function (SMF)) in the COSMOS field at z ∼ 3.3, making a comparison between the SMF in overdense environments and the SMF in the coeval field. In particular, this region contains the Elentári proto-supercluster, a system of six extended o…

2024 The Astrophysical Journal
eHST 11
Active Dwarf Galaxy Database. I. Overlap between Active Galactic Nuclei Selected by Different Techniques
DOI: 10.3847/1538-4357/ad5442 Bibcode: 2024ApJ...971...68W

Wasleske, Erik J.; Baldassare, Vivienne F.

We assemble a sample of 733 dwarf galaxies (M * ≤ 109.5 M ) with signatures of active galactic nuclei (AGN) and explore the intersection between different AGN-selection techniques. Objects in our database are compiled from previous studies that identify AGN in dwarf galaxies through spectroscopy, X-ray emission, i…

2024 The Astrophysical Journal
XMM-Newton 11
Multiphase Black Hole Feedback and a Bright [C II] Halo in a LoBAL Quasar at z ∼ 6.6
DOI: 10.3847/1538-4357/ad4a77 Bibcode: 2024ApJ...970....9B

Carniani, Stefano; Tripodi, Roberta; Lai, Samuel +18 more

Although the mass growth of supermassive black holes during the epoch of reionization is expected to play a role in shaping the concurrent growth of their host galaxies, observational evidence of feedback at z ≳ 6 is still sparse. We perform the first multiscale and multiphase characterization of black-hole-driven outflows in the z ∼ 6.6 quasar J0…

2024 The Astrophysical Journal
JWST 11
Constraints on the Lyman Continuum Escape from Low-mass Lensed Galaxies at 1.3 ≤ z ≤ 3.0
DOI: 10.3847/1538-4357/ad554d Bibcode: 2024ApJ...971..175J

Finkelstein, Steven L.; Ferguson, Henry C.; Grazian, Andrea +17 more

Low-mass galaxies can significantly contribute to reionization due to their potentially high Lyman continuum (LyC) escape fraction and relatively high space density. We present a constraint on the LyC escape fraction from low-mass galaxies at z = 1.3–3.0. We obtained rest-frame UV continuum imaging with the ACS/SBC and the WFC3/UVIS from the Hubbl…

2024 The Astrophysical Journal
eHST 11
Tip of the Red Giant Branch Distances with JWST. II. I-band Measurements in a Sample of Hosts of 10 Type Ia Supernova Match HST Cepheids
DOI: 10.3847/1538-4357/ad84f3 Bibcode: 2024ApJ...976..177L

Casertano, Stefano; Li, Siyang; Riess, Adam G. +7 more

The Hubble Tension, a >5σ discrepancy between direct and indirect measurements of the Hubble constant (H 0), has persisted for a decade and motivated intense scrutiny of the paths used to infer H 0. Comparing independently derived distances for a set of galaxies with different standard candles, such as the tip of the red g…

2024 The Astrophysical Journal
JWST 11
An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. II. JWST NIRCam Wide Filters
DOI: 10.3847/1538-4357/ad79f8 Bibcode: 2024ApJ...975..195N

McQuinn, Kristen B. W.; Dolphin, Andrew E.; Skillman, Evan D. +4 more

The tip of the red giant branch (TRGB) is a standardizable candle, identifiable as the discontinuity at the bright extreme of the red giant branch (RGB) stars in color–magnitude diagram space. The TRGB-based distance method has been used to measure distances to galaxies out to D ≤ 20 Mpc with the Hubble Space Telescope F814W filter, and is an impo…

2024 The Astrophysical Journal
JWST 11
Rotation and Abundances of the Benchmark Brown Dwarf HD 33632 Ab from Keck/KPIC High-resolution Spectroscopy
DOI: 10.3847/1538-4357/ad58d3 Bibcode: 2024ApJ...971....9H

Fitzgerald, Michael P.; López, Ronald A.; Skemer, Andrew +24 more

We present the projected rotational velocity and molecular abundances for HD 33632 Ab obtained via Keck Planet Imager and Characterizer (KPIC) high-resolution spectroscopy. HD 33632 Ab is a nearby benchmark brown dwarf companion at a separation of ∼20 au that straddles the L–T transition. Using a forward-modeling framework with on-axis host star s…

2024 The Astrophysical Journal
Gaia 11
White Dwarf Merger Remnants: The DAQ Subclass
DOI: 10.3847/1538-4357/ad3440 Bibcode: 2024ApJ...965..159K

Blouin, Simon; Bergeron, Pierre; Kilic, Mukremin +3 more

Four years after the discovery of a unique DAQ white dwarf with a hydrogen-dominated and carbon-rich atmosphere, we report the discovery of four new DAQ white dwarfs, including two that were not recognized properly in the literature. We find all five DAQs in a relatively narrow mass and temperature range of M = 1.14–1.19 M and T

2024 The Astrophysical Journal
Gaia 11
First JWST Observations of JAGB Stars in the SN Ia Host Galaxies: NGC 7250, NGC 4536, NGC 3972
DOI: 10.3847/1538-4357/ad12c7 Bibcode: 2024ApJ...961..132L

Madore, Barry F.; Freedman, Wendy L.; Jang, In Sung +2 more

The J-region Asymptotic Giant Branch (JAGB) method is a standard candle that leverages the constant luminosities of color-selected, carbon-rich AGB stars, measured in the near-infrared at 1.2 µm. The Chicago-Carnegie Hubble Program has obtained JWST imaging of the SN Ia host galaxies NGC 7250, NGC 4536, and NGC 3972. With these observations,…

2024 The Astrophysical Journal
JWST 11
Stellar Mergers or Truly Young? Intermediate-age Stars on Highly Radial Orbits in the Milky Way's Stellar Halo
DOI: 10.3847/1538-4357/ad58de Bibcode: 2024ApJ...971..170H

Price-Whelan, Adrian M.; Ness, Melissa K.; Horta, Danny +2 more

Reconstructing the mass assembly history of the Milky Way relies on obtaining detailed measurements of the properties of many stars in the galaxy, especially in the stellar halo. One of the most constraining quantities is stellar age, as it can shed light on the accretion time and quenching of star formation in merging satellites. However, obtaini…

2024 The Astrophysical Journal
Gaia 11