Speaker
Blas Irigoyen Gimenez
(Fermi National Accelerator Laboratory)
Description
This work reports results aimed at enhancing the signal-to-noise ratio (SNR) of Skipper-CCD for astronomical applications. Results on the implementation of a backside processing for fully depleted Skipper CCDs using arsenic ion implantation and microwave annealing for back contact formation and activation are presented. Simulations and experimental progress to date will be presented. This represents a promising step toward a highly sensitive and optically efficient instrument for astronomy.
Author
Blas Irigoyen Gimenez
(Fermi National Accelerator Laboratory)