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CEERS Key Paper. IX. Identifying Galaxy Mergers in CEERS NIRCam Images Using Random Forests and Convolutional Neural Networks
DOI: 10.3847/2041-8213/ad8dd4 Bibcode: 2024ApJ...976L...8R

Papovich, Casey; Yang, Guang; Finkelstein, Steven L. +32 more

A crucial yet challenging task in galaxy evolution studies is the identification of distant merging galaxies, a task that suffers from a variety of issues ranging from telescope sensitivities and limitations to the inherently chaotic morphologies of young galaxies. In this paper, we use random forests and convolutional neural networks to identify …

2024 The Astrophysical Journal
JWST 5
Optical- and UV-continuum Morphologies of Compact Radio Source Hosts
DOI: 10.3847/1538-4357/ad2513 Bibcode: 2024ApJ...965...17D

Worrall, D. M.; Morganti, R.; O'Dea, C. P. +6 more

We present the first systematic search for UV signatures from radio source-driven active galactic nuclei (AGN) feedback in Compact Steep Spectrum (CSS) radio galaxies. Owing to their characteristic sub-galactic jets (1–20 kpc projected linear sizes), CSS hosts are excellent laboratories for probing galaxy scale feedback via jet-triggered star form…

2024 The Astrophysical Journal
eHST 5
The Impact of Cometary "Impacts" on the Chemistry, Climate, and Spectra of Hot Jupiter Atmospheres
DOI: 10.3847/1538-4357/ad28b3 Bibcode: 2024ApJ...966...39S

Walsh, C.; Sainsbury-Martinez, F.

Impacts from icy and rocky bodies have helped shape the composition of Solar System objects; for example, the Earth–Moon system, or the recent impact of comet Shoemaker–Levy 9 with Jupiter. It is likely that such impacts also shape the composition of exoplanetary systems. Here, we investigate how cometary impacts might affect the atmospheric compo…

2024 The Astrophysical Journal
JWST 5
AGN STORM 2. X. The Origin of the Interband Continuum Delays in Mrk 817
DOI: 10.3847/1538-4357/ad8160 Bibcode: 2024ApJ...976...59N

Kaspi, Shai; Barth, Aaron J.; Horne, Keith +26 more

The local (z = 0.0315) active galactic nucleus (AGN) Mrk 817 was monitored over more than 500 days with space-borne and ground-based instruments as part of a large international campaign, AGN STORM 2. Here, we present a comprehensive analysis of the broadband continuum variations using detailed modeling of the broad line region (BLR), several type…

2024 The Astrophysical Journal
eHST 4
DIISC-III. Signatures of Stellar Disk Growth in Nearby Galaxies
DOI: 10.3847/1538-4357/ad029b Bibcode: 2024ApJ...960...24P

Heckman, Timothy; Kennicutt, Robert C.; Thilker, David +8 more

We explore the growth of the stellar disks in 14 nearby spiral galaxies as part of the Deciphering the Interplay between the Interstellar medium, Stars, and the Circumgalactic medium (DIISC) survey. We study the radial distribution of specific star formation rates (sSFRs) and investigate the ratio of the difference in the outer and inner sSFRs (Δ<…

2024 The Astrophysical Journal
eHST 4
Contemporaneous X-Ray Observations of 30 Bright Radio Bursts from the Prolific Fast Radio Burst Source FRB 20220912A
DOI: 10.3847/1538-4357/ad6a13 Bibcode: 2024ApJ...974..170C

Kaspi, Victoria M.; Bhardwaj, Mohit; Scholz, Paul +21 more

We present an extensive contemporaneous X-ray and radio campaign performed on the repeating fast radio burst (FRB) source FRB 20220912A for 8 weeks immediately following the source's detection by CHIME/FRB. This includes X-ray data from XMM-Newton, NICER, and Swift, and radio detections of FRB 20220912A from CHIME/Pulsar and Effelsberg. We detect …

2024 The Astrophysical Journal
XMM-Newton 4
A Comprehensive Study of Open Cluster Chemical Homogeneity Using APOGEE and Milky Way Mapper Abundances
DOI: 10.3847/1538-4357/ad78e1 Bibcode: 2024ApJ...975...89S

Cunha, Katia; Souto, Diogo; Tayar, Jamie +4 more

Stars in an open cluster are assumed to have formed from a broadly homogeneous distribution of gas, implying that they should be chemically homogeneous. Quantifying the level to which open clusters are chemically homogeneous can therefore tell us about interstellar medium pollution and gas mixing in progenitor molecular clouds. Using Sloan Digital…

2024 The Astrophysical Journal
Gaia 4
Spatial Variations of Dust Opacity and Grain Growth in Dark Clouds: L1689, L1709, and L1712
DOI: 10.3847/1538-4357/ad2a59 Bibcode: 2024ApJ...965...29L

Chen, Xi; Jiang, Biwei; Zhao, He +2 more

The far-infrared (FIR) opacity of dust in dark clouds within the Ophiuchus molecular cloud is investigated through multiwavelength infrared observations from UKIDSS, Spitzer, and Herschel. Employing the infrared color excess technique with both near-infrared and mid-infrared photometric data, a high-resolution extinction map in the K band (A

2024 The Astrophysical Journal
Herschel 4
ALMA-LEGUS. II. The Influence of Subgalactic Environments on Molecular Cloud Properties
DOI: 10.3847/1538-4357/ad198a Bibcode: 2024ApJ...964...13F

Grebel, Eva K.; Smith, Linda J.; Aloisi, Alessandra +24 more

We compare the molecular cloud properties in subgalactic regions of two galaxies, barred spiral NGC 1313, which is forming many massive clusters, and flocculent spiral NGC 7793, which is forming significantly fewer massive clusters despite having a similar star formation rate to NGC 1313. We find that there are larger variations in cloud propertie…

2024 The Astrophysical Journal
eHST 4
Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
DOI: 10.3847/1538-4357/ad64d2 Bibcode: 2024ApJ...974...22Z

Choi, Yumi; Olsen, Knut; Roman-Duval, Julia +11 more

The Large Magellanic Cloud (LMC) is home to many H II regions, which may lead to significant outflows. We examine the LMC's multiphase gas (T∼104-5 K) in H I, S II, Si IV, and C IV using 110 stellar sight lines from the Hubble Space Telescope's Ultraviolet Legacy Library of Young Stars as Essential Standards program. We develop a contin…

2024 The Astrophysical Journal
eHST 4