Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3873
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dc.contributor.authorRikame, Ketanen_US
dc.contributor.authorChattopadhyay, Sabyasachi et al.en_US
dc.date.accessioned2019-09-09T11:26:40Z
dc.date.available2019-09-09T11:26:40Z
dc.date.issued2018-07en_US
dc.identifier.citationJournal of Astronomical Telescopes, Instruments, and Systems, 4(3), 036002.en_US
dc.identifier.issn2329-4124en_US
dc.identifier.issn2329-4221en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3873
dc.identifier.urihttps://doi.org/10.1117/1.JATIS.4.3.036002en_US
dc.description.abstractThe IUCAA digital sampling array controller (IDSAC) is a flexible and generic yet powerful CCD controller that can handle a wide range of scientific detectors. Based on an easily scalable modular backplane architecture consisting of single board controllers (SBC), IDSAC can control large detector arrays and mosaics. Each of the SBCs offers the full functionality required to control a CCD independently. The SBCs can be cold swapped without the need to reconfigure them. IDSAC is also available in a backplane-less architecture. Each SBC can handle data from up to four video channels with or without dummy outputs at speeds up to 500-kilo pixels per second (kPPS) per channel with a resolution of 16 bits. Communication with a Linux-based host computer is through a USB3.0 interface, with the option of using copper or optical fibers. A field programmable gate array (FPGA) is used as the master controller in each SBC, which allows great flexibility in optimizing performance by adjusting gain, timing signals, bias levels, etc., using user-editable configuration files without altering the circuit topology. Elimination of thermal kTC noise is achieved via digital correlated double sampling (DCDS). The number of digital samples per pixel (for both reset and signal levels) is user configurable. We present the results of noise performance characterization of IDSAC through simulation, theoretical modeling, and actual measurements. The contribution of different types of noise sources is modeled using a tool to predict noise of a generic DCDS signal chain analytically. The analytical model predicts the net input referenced noise of the signal chain to be 5 electrons for 200-k pixels/s per channel readout rate with three samples per pixel. Using a cryogenic test setup in the lab, the noise is measured to be 5.4 e (24.3 μV), for the same readout configuration. With a better-optimized configuration of 500-kPPS readout rate, the measured noise is down to 3.8 electrons RMS (17 μV), with three samples per interval.en_US
dc.language.isoenen_US
dc.publisherSociety of Photo-Optical Instrumentation Engineersen_US
dc.subjectIUCAA digital sampling array controlleren_US
dc.subjectFlexible and generic yet powerfulen_US
dc.subjectCCD controlleren_US
dc.subjectDCDS signal chain analyticallyen_US
dc.subjectDCDS technique for processingen_US
dc.subject2018en_US
dc.titleNoise characterization of IUCAA digital sampling array controlleren_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitleJournal of Astronomical Telescopes, Instruments, and Systemsen_US
dc.publication.originofpublisherForeignen_US
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