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JWST MIRI Detections of Hα and [O III] and a Direct Metallicity Measurement of the z = 10.17 Lensed Galaxy MACS0647‑JD
DOI: 10.3847/1538-4357/ad6562 Bibcode: 2024ApJ...973...81H

Costantin, Luca; Hutchison, Taylor A.; Larson, Rebecca L. +30 more

JWST spectroscopy has revolutionized our understanding of galaxies in the early Universe. Covering wavelengths up to 5.3 µm, NIRSpec can detect rest-frame optical Hα emission lines out to z = 7 and [O III] to z = 9.5. Observing these lines in more distant galaxies requires longer wavelength spectroscopy with MIRI. Here we present MIRI Medium…

2024 The Astrophysical Journal
eHST JWST 22
The Star-forming Main Sequence in JADES and CEERS at z > 1.4: Investigating the Burstiness of Star Formation
DOI: 10.3847/1538-4357/ad8ba4 Bibcode: 2024ApJ...977..133C

Shapley, Alice E.; Reddy, Naveen A.; Sanders, Ryan L. +5 more

We have used public JWST/NIRSpec and JWST/NIRCam observations from the CEERS and JADES surveys in order to analyze the star-forming main sequence (SFMS) over the redshift range 1.4 ≤ z < 7. We calculate the star formation rates (SFRs) of the galaxy sample using three approaches: Balmer line luminosity, spectral energy distribution (SED) fitting…

2024 The Astrophysical Journal
eHST JWST 22
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
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
Sulfur Dioxide and Other Molecular Species in the Atmosphere of the Sub-Neptune GJ 3470 b
DOI: 10.3847/2041-8213/ad55e9 Bibcode: 2024ApJ...970L..10B

Fortney, Jonathan J.; Henry, Gregory W.; Bell, Taylor J. +13 more

We report observations of the atmospheric transmission spectrum of the sub-Neptune exoplanet GJ 3470 b taken using the Near-Infrared Camera on JWST. Combined with two archival Hubble Space Telescope/Wide-Field Camera 3 transit observations and 15 archival Spitzer transit observations, we detect water, methane, sulfur dioxide, and carbon dioxide in…

2024 The Astrophysical Journal
Gaia eHST JWST 21
Uncovering a Massive z 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
DOI: 10.3847/2041-8213/ad11ee Bibcode: 2024ApJ...961L..25L

Casey, Caitlin M.; Chworowsky, Katherine; Hutchison, Taylor A. +47 more

In this Letter, we report the discovery of the highest redshift, heavily obscured, radio-loud (RL) active galactic nucleus (AGN) candidate selected using JWST NIRCam/MIRI, mid-IR, submillimeter, and radio imaging in the COSMOS-Web field. Using multifrequency radio observations and mid-IR photometry, we identify a powerful, RL, growing supermassive…

2024 The Astrophysical Journal
eHST JWST 21
The On-axis Jetted Tidal Disruption Event AT2022cmc: X-Ray Observations and Broadband Spectral Modeling
DOI: 10.3847/1538-4357/ad2b6b Bibcode: 2024ApJ...965...39Y

Kulkarni, S. R.; Cenko, S. Bradley; Gezari, Suvi +5 more

AT2022cmc was recently reported as the first on-axis jetted tidal disruption event (TDE) discovered in the last decade, and the fourth on-axis jetted TDE candidate known so far. In this work, we present NuSTAR hard X-ray (3–30 keV) observations of AT2022cmc, as well as soft X-ray (0.3–6 keV) observations obtained by NICER, Swift, and XMM-Newton. O…

2024 The Astrophysical Journal
XMM-Newton 21
Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data
DOI: 10.3847/1538-4357/ad062f Bibcode: 2024ApJ...961..189N

Hamaguchi, Kenji; Notsu, Yuta; Kowalski, Adam F. +12 more

We conducted the time-resolved simultaneous optical spectroscopic and photometric observations of mid-M-dwarf flare stars YZ CMi, EV Lac, and AD Leo. Spectroscopic observations were obtained using Apache Point Observatory 3.5 m and Small and Moderate Aperture Research Telescope System 1.5 m telescopes during 31 nights. Among the 41 detected flares…

2024 The Astrophysical Journal
Gaia 21