collaborators

15 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.IM2026

Revealing Cosmic Ecosystems with the Hubble Space Telescope in 2030s and Beyond

Sanchayeeta Borthakur, Tanmay Singh, David French +22

Ultraviolet spectroscopy with the Hubble Space Telescope (HST) provides the most direct and sensitive probe of the disk-circumgalactic medium (CGM) interface at radii of 20 kpc, wh…

astro-ph.IM2026

Astronomical Advantages of a Boost Mission to Facilitate HST Science into the 2030s: Imaging the Circumgalactic Medium of Galaxies

Matthew J. Hayes, Kate H. R. Rubin, Michelle A. Berg +20

We present the case for imaging ultraviolet line emission from highly ionized metals and HI Lya in the circumgalactic medium of galaxies, should the Hubble Space Telescope receive…

astro-ph.IM2026

Extending Hubble into the 2030s to Resolve the Physics of LyC Escape

Cody Carr, Stephan McCandliss, Michelle Berg +6

Current observations with the James Webb Space Telescope (JWST) suggest that star-forming galaxies produce enough ionizing (LyC; nm) photons to drive cosmic reionization…

astro-ph.GA2026

Witnessing the onset of stellar winds in Super-Luminous Supernova Hosts: implications for star-formation-driven outflows in low and high-redshift galaxies

A. Saldana-Lopez, A. Gkini, M. J. Hayes +6

Direct observational constraints on the earliest, stellar-wind-dominated phases of galactic outflows remain scarce. We present medium-resolution VLT/X-shooter spectroscopy of six T…

astro-ph.GA2026

Modeling Emission-Line Surface Brightness in a Multiphase Galactic Wind: An O VI Case Study

Zirui Chen, Zixuan Peng, Kate H. R. Rubin +6

We present a fast and robust analytic framework for predicting surface brightness (SB) of emission lines in galactic winds as a function of radius up to kpc out in the c…