Mapper of the IGM Spin Temperature
MIST is a Cosmology Experiment trying to detect with high precision the Global Redshifted 21-cm Signal that encapsulates the large-scale physics of the Universe during its first billion years; specifically, during the Universe's Dark Ages, Cosmic Dawn, and Epoch of Reionization.
For this purpose, MIST conducts measurements of the sky-averaged radio spectrum at frequencies below 200 MHz from some of the most remote sites on Earth.
Team
Ricardo Bustos (PI) (UCSC) Ian Hendricksen (McGill)
Raúl Monsalve (Co-PI) (UC Berkeley)   (raul.monsalve AT berkeley.edu) Christian Bye (UC Berkeley)
Cynthia Chiang (McGill) Xinze 'Sunny' Guo (UC Berkeley)
Jonathan Sievers (McGill) Francis McGee (McGill)
Nithyanandan Thyagarajan (CSIRO) Cinthia Altamirano (UCSC)
Patricio Mena (NRAO) Lisa Nasu-Yu (McGill)
Silvia Restrepo (UCSC) Vadym Bidula (McGill)
Past Members
Benjamín Fernández
Mauricio Díaz
Felipe Lucero
Matheus Pessôa
Erika Hornecker
Garima Prabhakar
Oscar Restrepo