Search Publications

Adding value to JWST spectra and photometry: stellar population and star formation properties of spectroscopically confirmed JADES and CEERS galaxies at z > 7
DOI: 10.1093/mnras/stae872 Bibcode: 2024MNRAS.529.4728D

Conselice, Christopher J.; Li, Qiong; Adams, Nathan +5 more

In this paper, we discuss measurements of the stellar population and star-forming properties for 43 spectroscopically confirmed publicly available high-redshift z > 7 JWST galaxies in the JADES and CEERS observational programs. We carry out a thorough study investigating the relationship between spectroscopic features and photometrically derive…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 13
Strong outflows and inefficient star formation in the reionization-era ultrafaint dwarf galaxy Eridanus II
DOI: 10.1093/mnras/stae1010 Bibcode: 2024MNRAS.530.2315S

Weisz, Daniel R.; Weinberg, David H.; Fu, Sal Wanying +1 more

We present novel constraints on the underlying galaxy formation physics (e.g. mass-loading factor, star formation history, and metal retention) at z ≳ 7 for the low-mass (M* ~ 105 M) Local Group ultrafaint dwarf galaxy (UFD) Eridanus II (Eri II). Using a hierarchical Bayesian framework, we apply a one-zone chemica…

2024 Monthly Notices of the Royal Astronomical Society
eHST 13
CARMENES input catalog of M dwarfs. VII. New rotation periods for the survey stars and their correlations with stellar activity
DOI: 10.1051/0004-6361/202346794 Bibcode: 2024A&A...684A...9S

Nagel, E.; Amado, P. J.; Caballero, J. A. +40 more


Aims: Knowledge of rotation periods (Prot) is important for understanding the magnetic activity and angular momentum evolution of late-type stars, as well as for evaluating radial velocity signals of potential exoplanets and identifying false positives. We measured photometric and spectroscopic Prot for a large sample of…

2024 Astronomy and Astrophysics
Gaia 13
EPOCHS IX. When cosmic dawn breaks: evidence for evolved stellar populations in 7 < z < 12 galaxies from PEARLS GTO and public NIRCam imaging
DOI: 10.1093/mnras/stad3877 Bibcode: 2024MNRAS.52711627T

Grogin, Norman A.; Pirzkal, Nor; Wilkins, Stephen M. +28 more

The presence of evolved stars in high-redshift galaxies can place valuable indirect constraints on the onset of star formation in the Universe. Thus, we use PEARLS GTO (Prime Extragalactic Areas for Reionization and Lensing Science Guaranteed Time Observations) and public NIRCam (Near Infrared Camera) photometric data to search for Balmer-break ca…

2024 Monthly Notices of the Royal Astronomical Society
JWST 13
The Next Generation Deep Extragalactic Exploratory Public Near-infrared Slitless Survey Epoch 1 (NGDEEP-NISS1): Extragalactic Star-formation and Active Galactic Nuclei at 0.5 < z < 3.6
DOI: 10.3847/1538-4357/ad429c Bibcode: 2024ApJ...969...90P

Papovich, Casey; Finkelstein, Steven L.; Pérez-González, Pablo G. +48 more

The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) survey program was designed specifically to include Near Infrared Slitless Spectroscopic observations (NGDEEP-NISS) to detect multiple emission lines in as many galaxies as possible and across a wide redshift range using the Near Infrared Imager and Slitless Spectrograph. We presen…

2024 The Astrophysical Journal
eHST JWST 13
NICER Discovery that SRGA J144459.2–604207 Is an Accreting Millisecond X-Ray Pulsar
DOI: 10.3847/2041-8213/ad4edb Bibcode: 2024ApJ...968L...7N

Chakrabarty, Deepto; Ray, Paul S.; Wolff, Michael T. +17 more

We present the discovery, with the Neutron Star Interior Composition Explorer (NICER), that SRGA J144459.2‑604207 is a 447.9 Hz accreting millisecond X-ray pulsar (AMXP), which underwent a 4 week long outburst starting on 2024 February 15. The AMXP resides in a 5.22 hr binary, orbiting a low-mass companion donor with M d > 0.1 M

2024 The Astrophysical Journal
INTEGRAL 13
Spectral Calculations of 3D Radiation Magnetohydrodynamic Simulations of Super-Eddington Accretion onto a Stellar-mass Black Hole
DOI: 10.3847/1538-4357/ad6b21 Bibcode: 2024ApJ...974..166M

Middleton, Matthew J.; Mills, Brianna S.; Davis, Shane W. +1 more

We use the Athena++ Monte Carlo (MC) radiation transfer module to postprocess simulation snapshots from nonrelativistic Athena++ radiation magnetohydrodynamic (RMHD) simulations. These simulations were run using a gray (frequency-integrated) approach but were also restarted and ran with a multigroup approach that accounts for Compton scattering wi…

2024 The Astrophysical Journal
XMM-Newton 13
First asteroseismic analysis of the globular cluster M80: multiple populations and stellar mass-loss
DOI: 10.1093/mnras/stad3565 Bibcode: 2024MNRAS.527.7974H

Stello, Dennis; De Silva, Gayandhi M.; Howell, Madeline +1 more

Asteroseismology provides a new avenue for accurately measuring the masses of evolved globular cluster (GC) stars. We present the first detections of solar-like oscillations in 47 red giant branch (RGB) and early asymptotic giant branch (EAGB) stars in the metal-poor GC M80; only the second with measured seismic masses. We investigate two areas of…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 13
Correlation between accretion rate and free-free emission in protoplanetary disks. A multiwavelength analysis of central mm/cm emission in transition disks
DOI: 10.1051/0004-6361/202348387 Bibcode: 2024A&A...684A.134R

van der Marel, N.; van der Tak, F. F. S.; Francis, L. +3 more

Context. The inner regions of protoplanetary disks are believed to be the primary locations of planet formation and the processes that influence the global evolution of the disk, such as magnetohydrodynamic winds and photoevaporation. Transition disks with large inner dust cavities are ideal targets for studying the inner regions (of tens of au) o…

2024 Astronomy and Astrophysics
Gaia 13
Imaging dark matter at the smallest scales with z ≈ 1 lensed stars
DOI: 10.1051/0004-6361/202450474 Bibcode: 2024A&A...689A.167D

Koekemoer, Anton M.; Treu, Tommaso; Filippenko, Alexei V. +19 more

Recent observations of caustic-crossing galaxies at redshift 0.7 ≲ z ≲ 1 show a wealth of transient events. Most of them are believed to be microlensing events of highly magnified stars. Earlier work predicts such events should be common near the critical curves (CCs) of galaxy clusters ("near region"), but some are found relatively far away from …

2024 Astronomy and Astrophysics
eHST 13