DESCRIPTION |
The Near Earth Asteroid Tracking (NEAT) survey began
observations with the U. S. Air Force 1.0m Ground-based
Electro-Optical Deep Space Surveillance (GEODSS)
telescope on Mt. Haleakala, Maui, HI (Pravdo 1999). In
2000, NEAT transitioned to the Maui Space Surveillance
Site (MSSS) 1.2m telescope located at the same facility.
The NEAT camera at the Maui site was a single 4096 x 4096
camera with 15 micron pixels. The pixel scale is 1.43
arc-sec/pixel with the 1.0m GEODSS telescope and 1.36
arc-sec/pixel with the MSSS 1.2m. No filters were used
and the bandpass is 0.4 - 0.8 microns, however the peak
response matches closely with the Bessel-type R filter
at 0.6 microns. A thermoelectric cooler (TEC) maintained
an approximate operating temperature of -5 and -20 degrees
C for the GEODSS and MSSS cameras, respectively. Four
amplifiers readout the CCD in four quadrants.
The table below provides a comparison of the instrument
and telescope characteristics used by NEAT on Maui, HI.
----------------------------------------------------------
| Site Maui/GEODSS Maui/MSSS |
| Dates of Operation: 12/95 - 2/99 2/00 - 4/07 |
| Telescope Diameter: 1.0m 1.2m |
| f/ratio: 2.15 3.14 |
| Camera: 4096 x 4096 4096 x 4096 |
| Pixel Size: 15 x 15 u 15 x 15 u |
| Pixel Scale: 1.43"/pix 1.36"/pix |
| Cooling: TEC @ ~-5C TEC @ ~-20C |
| Filter: None None |
| IAU Site Code: 566 608 |
| Latitude / Longitude: +20deg 42.5' 156deg 15.5'W |
| Elevation / Timezone: 3040.35m UTC - 10 |
|________________________________________________________|
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.
|