JWST observations of Terzan 5 reveal multiple stellar populations with ages of 12.5 and 4.7 Gyr, plus hints of a 3.8 Gyr component, suggesting a multi-epoch formation history.
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5 Pith papers cite this work. Polarity classification is still indexing.
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JWST difference imaging from COSMOS-Web and PRIMER has yielded 68 high-redshift supernovae including a core-collapse event at z>3 and a Type Ia at z>2, demonstrating the feasibility of wide-area time-domain searches in the early universe.
Over 100 caustic-crossing stellar events identified in the Dragon galaxy at z≈0.725 with JWST data yield a stellar luminosity function slope β=2.18 and confirm parity asymmetry.
New optical identifications and precise astrometry are reported for four quiescent black hole X-ray transients, with 3-sigma magnitude limits for five additional candidates.
Kinematically selected red clump stars give A_K/E_{H-K} = 1.259 ± 0.074, A_H/A_K = 1.794 ± 0.046, and a Nuclear Bulge stellar mass of 12.2 ± 2.6 × 10^8 solar masses.
citing papers explorer
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The multi-age stellar populations of Terzan 5 as revealed by JWST
JWST observations of Terzan 5 reveal multiple stellar populations with ages of 12.5 and 4.7 Gyr, plus hints of a 3.8 Gyr component, suggesting a multi-epoch formation history.
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Expanding the High-z Supernova Frontier: "Wide-Area" JWST Discoveries from the First Two Years of COSMOS-Web
JWST difference imaging from COSMOS-Web and PRIMER has yielded 68 high-redshift supernovae including a core-collapse event at z>3 and a Type Ia at z>2, demonstrating the feasibility of wide-area time-domain searches in the early universe.
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First Statistical Study of Over 100 Magnified Stellar Events at Redshift $z \approx 0.725$ with JWST
Over 100 caustic-crossing stellar events identified in the Dragon galaxy at z≈0.725 with JWST data yield a stellar luminosity function slope β=2.18 and confirm parity asymmetry.
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A search for optical counterparts in quiescent black hole X-ray transients
New optical identifications and precise astrometry are reported for four quiescent black hole X-ray transients, with 3-sigma magnitude limits for five additional candidates.
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Extinction law and stellar mass in the Nuclear Bulge from kinematically-selected red clump stars
Kinematically selected red clump stars give A_K/E_{H-K} = 1.259 ± 0.074, A_H/A_K = 1.794 ± 0.046, and a Nuclear Bulge stellar mass of 12.2 ± 2.6 × 10^8 solar masses.