collaborators

8 papers

astro-ph.GA2026

Spatially Resolved Nebular-Stellar Reddening with JWST/NIRISS

Peter J. Watson, Benedetta Vulcani, Tommaso Treu +7

An accurate determination of the dust attenuation within galaxies is essential to derive key physical properties such as the star formation rate (SFR). We present an analysis using…

astro-ph.GA2026

The NIRISS PASSAGE Spectroscopic Redshift Catalog in COSMOS

Mason S. Huberty, Kalina V. Nedkova, Zahra Sattari +34

We present the Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution (PASSAGE) spectroscopic redshift catalog in the COSMOS field. PASSAGE is a JWST Cycle 1 Nea…

astro-ph.GA2026

MAMMOTH-LyC: Investigating the Role of Galaxy Mergers in a Strong Lyman Continuum Leaker at

Shengzhe Wang, Xin Wang, Matthew A. Malkan +16

The MAMMOTH-LyC survey is a cycle 30 Hubble Space Telescope (HST) medium program obtaining 18-orbit-deep WFC3/UVIS F225W imaging in two massive galaxy protocluster fields at $z\sim…

astro-ph.GA2025

Compact Size, High SFR: Defining Morphological Features of Ly-Emitters

Keunho Kim, Anahita Alavi, Christopher Snapp-Kolas +7

The mechanisms of Ly photon escape are key to understanding galaxy evolution and cosmic reionization, yet remain poorly understood. We investigate the UV-continuum sizes of 23…

astro-ph.GA2025

The Parallel Ionizing Emissivity Survey (PIE). I. Survey design and selection of candidate Lyman Continuum leakers at 3.1<z<3.5

Alexander Beckett, Marc Rafelski, Claudia Scarlata +18

We present the survey design and initial results from the Parallel Ionizing Emissivity (PIE) survey. PIE is a large HST survey designed to detect Lyman continuum (LyC) emitting gal…

astro-ph.GA2025

UV Spectral Slope and Nebular Dust Attenuation in Dwarf Galaxies at

Anahita Alavi, Brian Siana, Harry I. Teplitz +7

We analyze nebular dust attenuation and its correlation with stellar mass () and UV spectral slope () in 33 lensed, low-mass star-forming galaxies at $1.4\leq z \leq 2.6…