The James Webb Space Telescope has discovered a surprising population of bright galaxies in the very early Universe (≲500 Myr after the Big Bang) that is hard to explain with conventional galaxy-formation models and whose physical properties are not fully understood. Insight into their internal physics is best captured through nebular lines, but at these early epochs, the brightest of these spectral features are redshifted into the mid-infrared and remain elusive. Using the mid-infrared instrument onboard the James Webb Space Telescope, here we present a detection of Hα and doubly ionized oxygen ([O iii] 4959,5007 Å) from the bright, ultra-high-redshift galaxy candidate GHZ2/GLASS-z12.
View Article and Find Full Text PDFAtmos Environ (1994)
June 2024
Purpose: Surgery is the definitive treatment for pterygium; therefore, reliable animal models are required for translational research. The goal of this investigation was to establish a standardized preclinical model of pterygium-like lesion.
Methods: A subconjunctival injection of fibroblasts (NIH3T3) and extracellular matrix was administered to 22 New Zealand rabbits.