Search Publications

MIDIS: JWST/MIRI Reveals the Stellar Structure of ALMA-selected Galaxies in the Hubble Ultra Deep Field at Cosmic Noon
DOI: 10.3847/1538-4357/ad43e5 Bibcode: 2024ApJ...969...27B

Henning, Thomas; Costantin, Luca; Boogaard, Leindert A. +30 more

We present deep James Webb Space Telescope (JWST)/Mid-Infrared Instrument (MIRI) F560W observations of a flux-limited, Atacama Large Millimeter/submillimeter Array (ALMA)-selected sample of 28 galaxies at z = 0.5–3.7 in the Hubble Ultra Deep Field (HUDF). The data from the MIRI Deep Imaging Survey (MIDIS) reveal the stellar structure of the HUDF g…

2024 The Astrophysical Journal
eHST JWST 19
Large-scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
DOI: 10.3847/1538-4357/ad32c5 Bibcode: 2024ApJ...966...18T

Casey, Caitlin M.; Kartaltepe, Jeyhan S.; Mobasher, Bahram +15 more

To study the role of environment in galaxy evolution, we reconstruct the underlying density field of galaxies based on COSMOS2020 (The Farmer catalog) and provide the density catalog for a magnitude-limited (K s < 24.5) sample of ∼210,000 galaxies at 0.4 < z < 5 within the COSMOS field. The environmental densities are calcula…

2024 The Astrophysical Journal
eHST 18
A Galactic Eclipse: The Small Magellanic Cloud Is Forming Stars in Two Superimposed Systems
DOI: 10.3847/1538-4357/ad1591 Bibcode: 2024ApJ...962..120M

Murray, Claire E.; Choi, Yumi; Lee, Min-Young +22 more

The structure and dynamics of the star-forming disk of the Small Magellanic Cloud (SMC) have long confounded us. The SMC is widely used as a prototype for galactic physics at low metallicity, and yet we fundamentally lack an understanding of the structure of its interstellar medium (ISM). In this work, we present a new model for the SMC by compari…

2024 The Astrophysical Journal
Gaia 18
Are These Planets or Brown Dwarfs? Broadly Solar Compositions from High-resolution Atmospheric Retrievals of ∼10–30 M Jup Companions
DOI: 10.3847/1538-4357/ad4796 Bibcode: 2024ApJ...970...71X

Zhang, Yapeng; Fitzgerald, Michael P.; López, Ronald A. +32 more

Using Keck Planet Imager and Characterizer high-resolution (R ∼ 35,000) spectroscopy from 2.29 to 2.49 µm, we present uniform atmospheric retrievals for eight young substellar companions with masses of ∼10–30 M Jup, orbital separations spanning ∼50–360 au, and T eff between ∼1500 and 2600 K. We find that all companions …

2024 The Astrophysical Journal
JWST 18
The One-hundred-deg2 DECam Imaging in Narrowbands (ODIN): Survey Design and Science Goals
DOI: 10.3847/1538-4357/ad165e Bibcode: 2024ApJ...962...36L

Dey, Arjun; Gronwall, Caryl; Jeong, Woong-Seob +40 more

We describe the survey design and science goals for One-hundred-deg2 DECam Imaging in Narrowbands (ODIN), a NOIRLab survey using the Dark Energy Camera (DECam) to obtain deep (AB ∼ 25.7) narrowband images over an unprecedented area of sky. The three custom-built narrowband filters, N419, N501, and N673, have central wavelengths of 419, …

2024 The Astrophysical Journal
Gaia 18
Two Distinct Classes of Quiescent Galaxies at Cosmic Noon Revealed by JWST PRIMER and UNCOVER
DOI: 10.3847/2041-8213/ad464c Bibcode: 2024ApJ...967L..23C

Dickinson, Mark; Giavalisco, Mauro; Grogin, Norman A. +31 more

We present a measurement of the low-mass quiescent size–mass relation at cosmic noon (1 < z < 3) from the JWST PRIMER and UNCOVER treasury surveys, which highlights two distinct classes of quiescent galaxies. While the massive population is well studied at these redshifts, the low-mass end has been previously underexplored due to a lack of o…

2024 The Astrophysical Journal
eHST JWST 18
MIDIS: JWST NIRCam and MIRI Unveil the Stellar Population Properties of Lyα Emitters and Lyman-break Galaxies at z ≃ 3–7
DOI: 10.3847/1538-4357/ad15f6 Bibcode: 2024ApJ...963...97I

Pérez-González, Pablo G.; Costantin, Luca; Boogaard, Leindert A. +29 more

We study the stellar population properties of 182 spectroscopically confirmed (MUSE/VLT) Lyα emitters (LAEs) and 450 photometrically selected Lyman-break galaxies (LBGs) at z = 2.8–6.7 in the Hubble Extreme Deep Field. Leveraging the combined power of Hubble Space Telescope and JWST NIRCam and MIRI observations, we analyze their rest-frame UV-thro…

2024 The Astrophysical Journal
eHST JWST 18
JWST MIRI MRS Images of Disk Winds, Water, and CO in an Edge-on Protoplanetary Disk
DOI: 10.3847/2041-8213/ad35c9 Bibcode: 2024ApJ...965L..13A

van Dishoeck, E. F.; Melnick, G. J.; Boogert, A. C. A. +14 more

We present JWST MIRI MRS observations of the edge-on protoplanetary disk around the young subsolar-mass star Tau 042021, acquired as part of the Cycle 1 GO program "Mapping Inclined Disk Astrochemical Signatures." These data resolve the mid-IR spatial distributions of H2, revealing X-shaped emission extending to ∼200 au above the disk m…

2024 The Astrophysical Journal
JWST 18
NGDEEP Epoch 1: Spatially Resolved Hα Observations of Disk and Bulge Growth in Star-forming Galaxies at z ∼ 0.6–2.2 from JWST NIRISS Slitless Spectroscopy
DOI: 10.3847/2041-8213/ad28bd Bibcode: 2024ApJ...963L..49S

Papovich, Casey; Finkelstein, Steven L.; Pérez-González, Pablo G. +21 more

We study the Hα equivalent width (EW(Hα)) maps of 19 galaxies at 0.6 < z < 2.2 in the Hubble Ultra Deep Field using NIRISS slitless spectroscopy as part of the Next Generation Deep Extragalactic Exploratory Public Survey. Our galaxies mostly lie on the star formation main sequence with stellar masses between 109 and 1011

2024 The Astrophysical Journal
Herschel eHST JWST 18
Discrepancies in the Properties of a Coronal Mass Ejection on Scales of 0.03 au as Revealed by Simultaneous Measurements at Solar Orbiter and Wind: The 2021 November 3–5 Event
DOI: 10.3847/1538-4357/ad1883 Bibcode: 2024ApJ...962..190R

Farrugia, C. J.; Davies, E. E.; Yu, W. +4 more

Simultaneous in situ measurements of coronal mass ejections (CMEs), including both plasma and magnetic field, by two spacecraft in radial alignment have been extremely rare. Here, we report on one such CME measured by Solar Orbiter (SolO) and Wind on 2021 November 3–5, while the spacecraft were radially separated by a heliocentric distance of 0.13…

2024 The Astrophysical Journal
SolarOrbiter 18