Gas-rich, star-forming, low-mass galaxies in the nearby Universe are powerful laboratories for studying baryonic physics in detail, including: stellar mass assembly, stellar feedback, chemical enrichment, and the interplay of the interstellar medium with star formation. Investigating these disparate yet interconnected...
Kristen B. W. McQuinn, O. Telford, Roger E. Cohen et al.· Astrophysical Journal Supple...· 2 citations
We present an experimental JWST/NIRSpec observational method to obtain $R\gtrsim1000$ G140M/F100LP slitless spectroscopic observations. This"Multi-Object Coronagraphy for Slitless Spectroscopy"(MOCSS) technique involves opening essentially all microshutters on NIRSpec simultaneously while closing shutters corresponding...
M. Huberty, C. Scarlata, Matthew J. Hayes et al.· 0 citations
We report the detection of a previously unknown object with a single emission line within the Hubble Ultra Deep Field, using a new JWST NIRSpec technique called Multiobject Coronagraphy for Slitless Spectroscopy (MOCSS) with the G140M/F100LP observing mode. The MOCSS technique involves opening almost all the shutters o...
M. Huberty, C. Scarlata, Matthew J. Hayes et al.· Astrophysical Journal· 0 citations
JWST has revealed rapid nitrogen enrichment in high redshift galaxies, renewing the need for stellar yields that follow metal free stars beyond the main sequence and across their final fates. We present Geneva stellar evolution models of rapidly rotating Pop~III stars with $5 \leq M_{\rm ini}/M_\odot \leq 200$ and $\up...
D. Nandal, Konstantinos Topalakis, V. Sergienko et al.· 0 citations
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