ASTRODEBATA / Victoria Strait: A low-mass galaxy in a star forming lull at z ∼ 5
A low-mass galaxy in a star forming lull at z ∼ 5
Dr. Victoria Strait
Cosmic Dawn Center, Copenhagen
While the cessation of star formation in high-redshift galaxies has been extensively studied, its underlying mechanisms remain elusive. Most research to date has concentrated on the most massive galaxies (log(M∗/M⊙) > 11) at redshifts below z ∼ 4, leaving a gap in our understanding of lower-mass systems in earlier epochs. I will report findings of an investigation on the nature of a low mass, high redshift galaxy: MACS0417-z5BBG. This intriguing galaxy, situated behind cluster MACS0417 at z = 5.201 ± 0.003 with a stellar mass of log(M∗/M⊙) ∼ 8, offers a unique glimpse into the early stages of galactic evolution. I will also discuss some updates from the Cosmic Dawn Center and the CAnadian NIRISS Unbiased Cluster Survey (CANUCS) team.