Search Publications

High-precision Atmospheric Characterization of a Y Dwarf with JWST NIRSpec G395H Spectroscopy: Isotopologue, C/O Ratio, Metallicity, and the Abundances of Six Molecular Species
DOI: 10.3847/1538-3881/ad3425 Bibcode: 2024AJ....167..237L

Fortney, Jonathan J.; Batalha, Natasha E.; Johnstone, Doug +19 more

The launch of the James Webb Space Telescope (JWST) marks a pivotal moment for precise atmospheric characterization of Y dwarfs, the coldest brown dwarf spectral type. In this study, we leverage moderate spectral resolution observations (R ∼ 2700) with the G395H grating of the Near-Infrared Spectrograph (NIRSpec) on board JWST to characterize the …

2024 The Astronomical Journal
JWST 16
Dynamics of a Galaxy at z > 10 Explored by JWST Integral Field Spectroscopy: Hints of Rotating Disk Suggesting Weak Feedback
DOI: 10.3847/1538-4357/ad82dd Bibcode: 2024ApJ...976..142X

Ono, Yoshiaki; Ouchi, Masami; Harikane, Yuichi +9 more

We investigate the dynamics of GN-z11, a luminous galaxy at z = 10.60, carefully analyzing the public deep integral field spectroscopy (IFS) data taken with the JWST NIRSpec integral field unit. While the observations of the IFS data originally targeted an He II clump near GN-z11, we find that the C III] λ λ1907, 1909 emission from ionized gas at …

2024 The Astrophysical Journal
JWST 16
Precision MARS Mass Reconstruction of A2744: Synergizing the Largest Strong-lensing and Densest Weak-lensing Data Sets from JWST
DOI: 10.3847/1538-4357/ad0cbf Bibcode: 2024ApJ...961..186C

Jee, M. James; Cha, Sangjun; HyeongHan, Kim +2 more

We present a new high-resolution free-form mass model of A2744 that combines both weak-lensing (WL) and strong-lensing (SL) data sets from JWST. The SL data set comprises 286 multiple images, presenting the most extensive SL constraint to date for a single cluster. The WL data set, employing photo-z selection, yields a source density of $\sim 350\…

2024 The Astrophysical Journal
JWST 16
High-precision Astrometry and Photometry with the JWST/MIRI Imager
DOI: 10.1088/1538-3873/ad2551 Bibcode: 2024PASP..136c4502L

Law, David R.; Hines, Dean C.; Álvarez-Márquez, Javier +8 more

Astrometry is one of the main pillars of astronomy, and one of its oldest branches. Over the years, an increasing number of astrometric works by means of Hubble Space Telescope (HST) data have revolutionized our understanding of various phenomena. With the launch of JWST, it becomes almost instinctive to want to replicate or improve these results …

2024 Publications of the Astronomical Society of the Pacific
Gaia JWST 16
Setting the Stage for the Search for Life with the Habitable Worlds Observatory: Properties of 164 Promising Planet-survey Targets
DOI: 10.3847/1538-4365/ad3e81 Bibcode: 2024ApJS..272...30H

Kane, Stephen R.; Dressing, Courtney D.; Harada, Caleb K. +1 more

The Decadal Survey on Astronomy and Astrophysics 2020 has recommended that NASA realize a large IR/optical/UV space telescope optimized for high-contrast imaging and spectroscopy of ∼25 exo-Earths and transformative general astrophysics. The NASA Exoplanet Exploration Program (ExEP) has subsequently released a list of 164 nearby (d < 25 pc) tar…

2024 The Astrophysical Journal Supplement Series
Gaia Hipparcos XMM-Newton 16
The SRG/eROSITA all-sky survey. Identifying the coronal content with HamStar
DOI: 10.1051/0004-6361/202348278 Bibcode: 2024A&A...684A.121F

Schmitt, J. H. M. M.; Salvato, M.; Czesla, S. +6 more

Context. The first eROSITA all-sky survey (eRASS1) performed on board the Spectrum-Roentgen-Gamma mission (SRG) provides more than 900 000 X-ray sources in the 0.2-2.3 keV band located in the western hemisphere.
Aims: We present identifications of the eRASS1 sources obtained using our HamStar method, which was designed for the identification …

2024 Astronomy and Astrophysics
Gaia 16
On the formation of a 33 solar-mass black hole in a low-metallicity binary
DOI: 10.33232/001c.117652 Bibcode: 2024OJAp....7E..38E

El-Badry, Kareem

A 33M⊙ black hole (BH) was recently discovered in an 11.6-year binary only 590 pc from the Sun. The system, Gaia BH3, contains a 0.8M⊙ low-metallicity giant () that is a member of the ED-2 stellar stream. This paper investigates whether the system could have formed via isolated binary evolution. I construct evolutionary models for metal-poor massi…

2024 The Open Journal of Astrophysics
Gaia 16
Cloud-by-cloud multiphase investigation of the circumgalactic medium of low-redshift galaxies
DOI: 10.1093/mnras/stae962 Bibcode: 2024MNRAS.530.3827S

Richter, Philipp; Charlton, Jane C.; Kacprzak, Glenn G. +10 more

The pervasive presence of warm gas in galaxy haloes suggests that the circumgalactic medium (CGM) is multiphase in its ionization structure and complex in its kinematics. Some recent state-of-the-art cosmological galaxy simulations predict an azimuthal dependence of CGM metallicities. We investigate the presence of such a trend by analysing the di…

2024 Monthly Notices of the Royal Astronomical Society
eHST 16
The Type I superluminous supernova catalogue I: light-curve properties, models, and catalogue description
DOI: 10.1093/mnras/stae2270 Bibcode: 2024MNRAS.535..471G

Rest, Armin; Villar, V. Ashley; Eftekhari, Tarraneh +25 more

We present the most comprehensive catalogue to date of Type I superluminous supernovae (SLSNe), a class of stripped-envelope supernovae (SNe) characterized by exceptionally high luminosities. We have compiled a sample of 262 SLSNe reported through 2022 December 31. We verified the spectroscopic classification of each SLSN and collated an exhaustiv…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 16
Strong size evolution of disc galaxies since z = 1. Readdressing galaxy growth using a physically motivated size indicator
DOI: 10.1051/0004-6361/202346133 Bibcode: 2024A&A...682A.110B

Trujillo, Ignacio; Buitrago, Fernando

Our understanding of how the size of galaxies has evolved over cosmic time is based on the use of the half-light (effective) radius as a size indicator. Although the half-light radius has many advantages for structurally parameterising galaxies, it does not provide a measure of the global extent of the objects, but only an indication of the size o…

2024 Astronomy and Astrophysics
eHST JWST 16