The information on this page provides the characteristics for the various CCDs and IR detectors in use on Kitt Peak.
The CCD characteristics are also available in the CCD Characteristics Manual, and some of the individual Instrument Manuals kept at each telescope.
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Currently Available KPNO - Detectors |
KPNO - Available Detectors
- Only the Dark Energy Survey Instrument (DESI)
will be in use at the Mayall 4 Meter telescope. No CCD information available at this time.
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IR Instruments
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Currently Available WIYN - Detectors |
WIYN - Available Detectors
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IR Instruments
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Retired KPNO - Detectors |
KPNO - Retired Detectors
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Retired IR Instruments
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WIYN - Detectors |
WIYN - Retired Detectors
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Retired IR Instruments
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KPNO CCD Instruments
LB1A
Specifications |
Quantum Efficiency Curve |
CCD: (LB1A 1980x800)
Format
: 1980 x 800
Gain
: 2.5 e-/adu
Read Noise :
7 e-
Dark Current : 20-80 electrons/(20 minutes)
Pixel size :
15 micro
Pixel scale : Instrument/Telescope dependent
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Images |
Ave. Dark (100s)
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Ave. Zero
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MARS CAM (LBNL)
Specifications |
Quantum Efficiency Curve |
CCD: (LBNL 1980x800)
Format
: 1980 x 800
Gain
: 2.0 e-/adu
Read Noise :
8.0 e-
Dark Current : 10-25 electrons/hour
Pixel size :
15 microns
Pixel scale : 0.8618"/pix
(determined from 700 stars in M15
imaged through an I-band filter)
(quadratic term in solution) |
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No Images Available |
WIYN CCD Instruments
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