489 citations · 3.7k across the 55 of their papers we have counts for
50 papers · 1 filter
Ciii] emission as an alternative to Ly in the reionization era: the dependence of Ciii] and Ly at from the VANDELS survey
Mark H Cunningham, Aayush Saxena, Richard S Ellis +1
The velocity offset of Ly emission from a galaxy's systemic redshift is an excellent tracer of conditions that enable the escape of Ly photons from the galaxy, and potentiall…
GA-NIFS: JWST/NIRSpec IFU observations of HFLS3 reveal a dense galaxy group at z~6.3
G. C. Jones, H. Ubler, M. Perna +19
Massive, starbursting galaxies in the early Universe represent some of the most extreme objects in the study of galaxy evolution. One such source is HFLS3 (z~6.34), which was origi…
The Star-forming and Ionizing Properties of Dwarf z~6-9 Galaxies in JADES: Insights on Bursty Star Formation and Ionized Bubble Growth
Ryan Endsley, Daniel P. Stark, Lily Whitler +37
Reionization is thought to be driven by faint star-forming galaxies, but characterizing this population has long remained very challenging. Here we utilize deep nine-band NIRCam im…
Inside the bubble: exploring the environments of reionisation-era Lyman- emitting galaxies with JADES and FRESCO
Joris Witstok, Renske Smit, Aayush Saxena +35
We present a study of the environments of 17 Lyman- (Ly) emitting galaxies (LAEs) in the reionisation era () identified by JWST/NIRSpec as part of the JWST Advan…
JADES: The production and escape of ionizing photons from faint Lyman-alpha emitters in the epoch of reionization
Aayush Saxena, Andrew J. Bunker, Gareth C. Jones +32
We present the properties of 17 faint Ly emitting galaxies (LAEs) at from the JWST Advanced Deep Extragalactic Survey (JADES) in the Hubble Ultra Deep Field/GOODS-S. The…
JADES: The emergence and evolution of Ly emission and constraints on the IGM neutral fraction
Gareth C. Jones, Andrew J. Bunker, Aayush Saxena +32
The rest-frame UV recombination emission line Ly can be powered by ionising photons from young massive stars in star forming galaxies, but its ability to be resonantly scattered…