User's Guide to the Prime Focus Camera


Table of Contents


Introduction
Description
Hardware Overview
Software Overview
Detector Characteristics
Plate Scale and FOV
Filters
Count Rates
PFCam User Interfaces
Dashboard
Top-end Interface
CCD Interface
Soundserver
Observing with PFCam
Starting the Software
Observing Hints
Illustrations
3-D representation
2-D representation
CCD diagrams
PFCam layout

Mt. Hamilton Homepage

CCD Characteristics (see also Plate Scale and Field of View)

PFCam's detector is a back-illuminated, Fairchild 4096 x 4096 CCD with 15-micron square pixels.

Quantum Efficiency Plot (measured in the lab, Jamuary 2006; opens in a new window).

Readnoise (measured on the telescope, June 2006 by E.G.)

binning readout
speed
gain readnoise
(e-)
readout time
(m:ss)
approx. bias (DN)
(left amp, right amp)
x1slow1.43.92:40 1750, 1750
x1fast1.35.40:50 1950, 1950
x2slow1.54.10:45 1800, 1800
x2fast1.35.00:15 1800, 1800
x4slow1.54.40:15 1900, 1900
x4fast1.35.20:05 1800, 1800

The CCD is linear over the full 64K DN dynamic range of the A-to-D converters (as measured on the telescope, January 2006 by E.G.). Full well is reached at 118K e-, well beyond the 64K DN A-to-D saturation.

The default setup reads out the CCD using two of the chip's four amplifiers. The overscan regions occupy the far right (highest numbered) columns and correspond to the amplifiers as shown below (overscan regions not to scale).

More PFCam CCD specs and characeristics can be found on our detector pages.