DESCRIPTION |
In 2001, the Palomar 1.2m Oschin Schmidt telescope located
in northern San Diego, CA was incorporated into the NEAT
inventory. The Palomar "Tri-camera" consists of three
separate 4096 x 4096 pixel CCDs. The CCDs are arranged
in a linear, north-south, orientation and denoted by "A,
B or C." An approximate one-degree gap is between each
CCD and each CCD covers nearly 1.0 square degree. The
15 micron pixels yield a pixel scale of 1.01 arc-sec/pixel.
No filters were used, but matches closely with a Bessel-
type R filter at 0.6 microns and TECs maintained an
operating temperature of -30 degrees C. Four amplifiers
readout the CCD in four quadrants. This camera, as well
as the Maui camera, used "CCD485" chips produced by
Fairchild Imaging. The central wavelength is 702 nm.
The table below provides a comparison of the QUEST and
tri-camera instruments used by NEAT at Palomar Observatory.
--------------------------------------------------------------
| Site Pal/Tri-cam Palomar/QUEST |
| Dates of Operation: 4/01 - 6/03 6/03 - 4/07 |
| Telescope Diameter: 1.2m 1.2m |
| f/ratio: 2.50 2.50 |
| Camera: 4096 x 4096 x 3 600 x 2400 x 112 |
| Pixel Size: 15 x 15 u 13 x 13 u |
| Pixel Scale: 1.01"/pix 0.87"/pix |
| Cooling: TEC @ ~-30C LN2 @ -120C |
| Filter: None 610 nm |
| IAU Site Code: 644 644 |
| |
| Latitude / Longitude: +33deg 21.4' 116deg 51.8'W |
| Elevation / Timezone: 1726.3m UTC - 8 |
|____________________________________________________________|
Regardless of the camera, each CCD chip read to a unique output
file. Filenames are based on the universal start time of the
exposure and, if appropriate, identify the specific chip used.
The Maui and tri-camera images contain the 4080 x 4080 imaging
area. The initial orientation of the Maui and Palomar tri-camera
images has East towards to left and North downward. Each
uncompressed, 4k x 4k, image (Palomar tri-camera and Maui) is
66.6 and 33.3 Mb in size, respectively.
|