activity
20242026
collaborators

8 papers

astro-ph.GA2026

MOSDEF-3D: Keck/OSIRIS Maps of the Ionized ISM in Galaxies

Natalie Lam, Alice E. Shapley, Ryan L. Sanders +8

We present spatially-resolved rest-frame optical emission line maps of four galaxies at observed with Keck/OSIRIS to study the physical conditions of the ISM at Cosmic N…

astro-ph.GA2026

The Far-Ultraviolet Extragalactic Legacy (FUEL) Survey: Hubble Far-UV Images and Catalogs of the Extragalactic Legacy Fields

Aliakbar Kavei, Brian Siana, Harry I. Teplitz +7

We present far-ultraviolet (FUV) images and catalogs from the Hubble Space Telescope (HST) Advanced Camera for Surveys/Solar Blind Channel (ACS/SBC) F150LP (about 1600 Angstrom) of…

astro-ph.GA2026

FRESCO: Constraining Dust Attenuation and Star-Formation Rates of Star-Forming Galaxies with JWST Paschen and Ground-Based Balmer Emission Line Observations

Michael A. Wozniak, Naveen A. Reddy, Pascal A. Oesch +7

We present new constraints on dust attenuation and star-formation rates (SFRs) for 77 galaxies at redshifts , using Paschen emission line detections from the JWST FRES…

astro-ph.GA2026

The faint end of the UV luminosity function at from the Hubble Frontier Fields

Lei Sun, Xiao-Lei Meng, Xin Wang +7

By extending the Hubble Frontier Fields (HFF) observations to the F225W band using HST WFC3/UVIS, we measure the rest-frame UV luminosity function (LF) of galaxies at $0.4 < z < 0.…

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

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…