Characterization of the SPARC4 CCDs
D. V. Bernardes (1), E. Martioli (1), C. V. Rodrigues (2) ((1), Laborat\'orio Nacional de Astrof\'isica, (2) Instituto Nacional de Pesquisas, Espaciais)

TL;DR
This paper systematically characterizes four SPARC4 CCD cameras, measuring key parameters like read noise, gain, dark current, and quantum efficiency to assess performance and monitor aging.
Contribution
It provides a comprehensive experimental methodology for CCD characterization, including spectral quantum efficiency measurements and analysis of spatial and temporal noise variations.
Findings
Average read noise of 6.33 electrons
Quantum efficiency up to 95.8%
Dark current of 0.00014 e-/pix/s at -70°C
Abstract
We present the photometric characterization of the four iXon Ultra 888 CCD cameras of the SPARC4 instrument, which will be installed on the 1.6 m telescope of the Pico dos Dias Observatory in Brazil. We applied experimental methodologies for a systematic characterization of the read noise, electronic gain, dark current, and quantum efficiency of the CCDs. We have analyzed the statistical distribution of the read noise, and also its spatial gradient and temporal variability, where we obtained an average value of the read noise of 6.33 electrons. We applied the Janesick method to determine the electronic gain, where we obtained an average value of 3.35 e-/ADU. We have also obtained an average dark current of 0.00014 e-/pix/s for CCD internal temperature of -70 oC. We have inspected the dependency of the dark current with temperature and the spatial distribution of the dark current, where…
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