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Characterization and Optimization of Skipper CCDs for the SOAR Integral Field Spectrograph (2311.00813v1)

Published 1 Nov 2023 in astro-ph.IM

Abstract: We present results from the characterization and optimization of six Skipper CCDs for use in a prototype focal plane for the SOAR Integral Field Spectrograph (SIFS). We tested eight Skipper CCDs and selected six for SIFS based on performance results. The Skipper CCDs are 6k $\times$ 1k, 15 $\mu$m pixels, thick, fully-depleted, $p$-channel devices that have been thinned to $\sim 250 \mu$m, backside processed, and treated with an antireflective coating. We optimize readout time to achieve $<4.3$ e$-$ rms/pixel in a single non-destructive readout and $0.5$ e$-$ rms/pixel in $5 \%$ of the detector. We demonstrate single-photon counting with $N_{\rm samp}$ = 400 ($\sigma_{\rm 0e-} \sim$ 0.18 e$-$ rms/pixel) for all 24 amplifiers (four amplifiers per detector). We also perform conventional CCD characterization measurements such as cosmetic defects ($ <0.45 \%$ ``bad" pixels), dark current ($\sim 2 \times 10{-4}$ e$-$/pixel/sec.), charge transfer inefficiency ($3.44 \times 10{-7}$ on average), and charge diffusion (PSF $< 7.5 \mu$m). We report on characterization and optimization measurements that are only enabled by photon-counting. Such results include voltage optimization to achieve full-well capacities $\sim 40,000-63,000$ e$-$ while maintaining photon-counting capabilities, clock induced charge optimization, non-linearity measurements at low signals (few tens of electrons). Furthermore, we perform measurements of the brighter-fatter effect and absolute quantum efficiency ($\gtrsim\, 80 \%$ between 450 nm and 980 nm; $\gtrsim\,90 \%$ between 600 nm and 900 nm) using Skipper CCDs.

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