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Mic Bagley

Publications and source records attributed to Mic Bagley.

2 recordsLinked to original sources

Why a Multi-Cycle Treasury Program is Essential to Maximize JWST's Scientific Contributions to Galaxy Formation

The Genesis Initiative is an extragalactic community-wide effort to coordinate white papers in response to the STScI Multi-Cycle Treasury (MCT) concept call. Two of JWST's primary science goals are to discover and characterize the first stars and galaxies, and to understand how they evolved into the galaxies we see today - questions whose fundamental importance has been affirmed by the past three decadal surveys. JWST's first five years have surpassed expectations, revealing a bounty of unexpected discoveries about the early universe. Yet these discoveries have raised as many questions as they have answered, and key mission goals remain unmet. Transforming this excitement into a quantitative physical understanding of early galaxy formation requires a uniform, statistically controlled legacy dataset that the current portfolio of smaller, heterogeneous programs cannot provide. The history of the Hubble Space Telescope offers a clear precedent. Its most transformative extragalactic results came from large, coordinated surveys far exceeding what the standard time-allocation process typically approves, and these uniform datasets remain scientifically productive decades later. We argue that JWST is now poised for the same leap. Answering the field's central open questions demands coordinated, community-led surveys of ~1000-2000 hr, with uniform and well-characterized selection functions that are structurally impossible within single-cycle programs. Such an investment is time-critical while JWST's instruments remain at peak performance, and would maximize synergy with ALMA, Euclid, Roman, Rubin, and future facilities. We therefore urge STScI to open a MCT channel, enabling the bold, ambitious surveys needed to understand how galaxies evolve from first light to the present day.

astro-ph.IM↗

THRILS -- The High-(Redshift+Ionization) Line Search: Program Description & Redshift Catalog

To date, many spectroscopic confirmations of z>7 galaxies have been obtained using JWST/NIRSpec prism observations, with most of their physical properties inferred from these observations and corresponding imaging. What is needed are higher-resolution spectra at deeper depths to study these sources in detail. We present The High-(Redshift+Ionization) Line Search (THRILS) program: deep (>8 hr) observations in two pointings of JWST/NIRSpec G395M spectroscopy to 1) probe high ionization spectral features in z>8 galaxies that are indicative of top-heavy initial mass functions or growing massive black holes, 2) search for accreting supermassive black holes in typical galaxies at z~4-9 through broad Balmer line emission, and 3) probe the stellar-mass growth histories of massive galaxies. We include spectroscopic redshift measurements for 89 sources from the THRILS data, as well as a detection threshold for the full and half depth integration times of the program.

astro-ph.GA↗