High Voltage CMOS Control Interface for Astronomy - Grade Charged Coupled Devices
| dc.creator | Martin, Elena | |
| dc.creator | Varner, Gary | |
| dc.creator | Koga, Aaron | |
| dc.creator | Ruckman, Larry | |
| dc.creator | Onaka, Peter | |
| dc.creator | Tonry, John | |
| dc.creator | Lee, Aaron | |
| dc.date | 2008-06-02 | |
| dc.date | 2008-08-12 | |
| dc.date.accessioned | 2026-07-07T11:51:19Z | |
| dc.date.available | 2026-07-07T11:51:19Z | |
| dc.description | The Pan-STARRS telescope consists of an array of smaller mirrors viewed by a Gigapixel arrays of CCDs. These focal planes employ Orthogonal Transfer CCDs (OTCCDs) to allow on-chip image stabilization. Each OTCCD has advanced logic features that are controlled externally. A CMOS Interface Device for High Voltage has been developed to provide the appropiate voltage signal levels from a readout and control system designated STARGRASP. OTCCD chip output levels range from -3.3V to 16.7V, with two different output drive strenghts required depending on load capacitance (50pF and 1000pF), with 24mA of drive and a rise time on the order of 100ns. Additional testing ADC structures have been included in this chip to evaluate future functional additions for a next version of the chip. | |
| dc.description | 13 pages, 17 gigures | |
| dc.identifier | https://arxiv.org/abs/0806.0223 | |
| dc.identifier | http://arxiv.org/abs/0806.0223 | |
| dc.identifier | JINST3:P08004,2008 | |
| dc.identifier | doi:10.1088/1748-0221/3/08/P08004 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/203857 | |
| dc.subject | Instrumentation and Detectors | |
| dc.subject | Space Physics | |
| dc.title | High Voltage CMOS Control Interface for Astronomy - Grade Charged Coupled Devices | |
| dc.type | text |