Search Publications

Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS
DOI: 10.3847/1538-4357/ad0a98 Bibcode: 2024ApJ...961..163B

Maiolino, Roberto; Conselice, Christopher J.; Bluck, Asa F. L. +10 more

We present an analysis of the quenching of star formation in massive galaxies (M * > 109.5 M ) within the first 0.5–3 Gyr of the Universe's history utilizing JWST-CEERS data. We utilize a combination of advanced statistical methods to accurately constrain the intrinsic dependence of quenching in a multidimensio…

2024 The Astrophysical Journal
eHST JWST 22
Young Star Clusters Dominate the Production of Detached Black Hole–Star Binaries
DOI: 10.3847/1538-4357/ad2f2c Bibcode: 2024ApJ...965...22D

Breivik, Katelyn; Rodriguez, Carl L.; Di Carlo, Ugo Niccolò +1 more

The recent discovery of two detached black hole–star (BH–star) binaries from Gaia's third data release has sparked interest in understanding the formation mechanisms of these systems. We investigate the formation of these systems by dynamical processes in young star clusters (SCs) and via isolated binary (IB) evolution, using a combination of dire…

2024 The Astrophysical Journal
Gaia 22
Effect of Extinction on Quasar Luminosity Distances Determined from UV and X-Ray Flux Measurements
DOI: 10.3847/1538-4357/ad11dc Bibcode: 2024ApJ...961..229Z

Zajaček, Michal; Czerny, Bożena; Khadka, Narayan +4 more

In Khadka et al., a sample of X-ray-detected reverberation-mapped quasars was presented and applied for the comparison of cosmological constraints inferred using two well-established relations in active galactic nuclei—the X-ray/UV luminosity (L X –L UV) relation and the broad-line region radius–luminosity (R–L) relation. L …

2024 The Astrophysical Journal
XMM-Newton 22
The APO-K2 Catalog. I. 7500 Red Giants with Fundamental Stellar Parameters from APOGEE DR17 Spectroscopy and K2-GAP Asteroseismology
DOI: 10.3847/1538-3881/ad0b13 Bibcode: 2024AJ....167...50S

Pinsonneault, Marc; Stassun, Keivan G.; García, Rafael A. +14 more

We present a catalog of fundamental stellar properties for ~7500 evolved stars, including stellar radii and masses, determined from the combination of spectroscopic observations from the Apache Point Observatory Galactic Evolution Experiment, part of the Sloan Digital Sky Survey IV, and asteroseismology from K2. The resulting APO-K2 catalog provid…

2024 The Astronomical Journal
Gaia 22
RR Lyrae from binary evolution: abundant, young, and metal-rich
DOI: 10.1093/mnras/stad3996 Bibcode: 2024MNRAS.52712196B

Belokurov, Vasily; Bobrick, Alexey; Iorio, Giuliano +3 more

RR Lyrae are a well-known class of pulsating horizontal branch stars widely used as tracers of old, metal-poor stellar populations. However, mounting observational evidence shows that a significant fraction of these stars may be young and metal-rich. Here, through detailed binary stellar evolution modelling, we show that all such metal-rich RR Lyr…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 22
Transmission Spectroscopy of the Habitable Zone Exoplanet LHS 1140 b with JWST/NIRISS
DOI: 10.3847/2041-8213/ad5afa Bibcode: 2024ApJ...970L...2C

MacDonald, Ryan J.; Dang, Lisa; Cowan, Nicolas B. +20 more

LHS 1140 b is the second-closest temperate transiting planet to Earth with an equilibrium temperature low enough to support surface liquid water. At 1.730 ± 0.025 R , LHS 1140 b falls within the radius valley separating H2-rich mini-Neptunes from rocky super-Earths. Recent mass and radius revisions indicate a bulk density si…

2024 The Astrophysical Journal
Gaia JWST 22
Gaia DR3 data consistent with a short bar connected to a spiral arm
DOI: 10.1093/mnras/stae083 Bibcode: 2024MNRAS.528.3576V

Steinmetz, M.; Khoperskov, S.; Minchev, I. +8 more

We use numerical simulations to model Gaia DR3 data with the aim of constraining the Milky Way (MW) bar and spiral structure parameters. We show that both the morphology and the velocity field in MW-like galactic disc models are strong functions of time, changing dramatically over a few tens of Myr. This suggests that by finding a good match to th…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 22
Evidence for inflows and outflows in the nearby black hole transient Swift J1727.8−162
DOI: 10.1051/0004-6361/202348754 Bibcode: 2024A&A...682L...1M

Armas Padilla, M.; Mata Sánchez, D.; Muñoz-Darias, T. +2 more

We present 20 epochs of optical spectroscopy obtained with the GTC-10.4m telescope across the bright discovery outburst of the black hole candidate Swift J1727.8−162. The spectra cover the main accretion states and are characterised by the presence of hydrogen and helium emission lines, commonly observed in these objects. They show complex profile…

2024 Astronomy and Astrophysics
Gaia 22
THEMIS 2.0: A self-consistent model for dust extinction, emission, and polarisation
DOI: 10.1051/0004-6361/202348391 Bibcode: 2024A&A...684A..34Y

Miville-Deschênes, M. -A.; Ysard, N.; Guillet, V. +6 more

Context. Recent observational constraints in emission, extinction, and polarisation have at least partially invalidated most of the astronomical standard grain models for the diffuse interstellar medium. Moreover, laboratory measurements on interstellar silicate analogues have shown quite significant differences with the optical properties used in…

2024 Astronomy and Astrophysics
Herschel 21
The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z = 4–6
DOI: 10.1051/0004-6361/202348782 Bibcode: 2024A&A...690A.197M

Übler, Hannah; Ferrara, Andrea; Fisher, Deanne B. +29 more

We present the morphological parameters and global properties of dust-obscured star formation in typical star-forming galaxies at z = 4–6. Among 26 galaxies composed of 20 galaxies observed by the Cycle-8 ALMA Large Program, CRISTAL, and 6 galaxies from archival data, we individually detect rest-frame 158 µm dust continuum emission from 19 g…

2024 Astronomy and Astrophysics
eHST 21