Collection Information
|
| IDENTIFIER |
urn:nasa:pds:gbo.ast.neat.survey:data_tricam::1.0
|
| NAME |
data_tricam collection for the "NEAR EARTH ASTEROID TRACKING" bundle
|
| TYPE |
Data
|
| DESCRIPTION |
This is the data_tricam collection for the gbo.ast.neat.survey bundle.
The Near-Earth Asteroid Tracking (NEAT)
project began as a collaborative effort with the United States Air
Force (USAF) in December 1995. It concentrated on the discovery and
observations of near-Earth asteroids and comets, collectively called
near-Earth objects (NEOs). NEAT ended its observations in April 2007.
Throughout its history, NEAT utilized three 1m class telescopes - two
on the Hawaiian island of Maui and the 1.2m Oschin Schmidt telescope
at Palomar Observatory near San Diego, CA. Three unique cameras were
developed and used throughout the program. These data are intended to
be usable for photometric analysis of the various objects within the
NEAT data. Most nights included calibration data, and the lists of
photometric standard calibration fields.
|
| SEARCH/ACCESS DATA |
NEAR EARTH ASTEROID TRACKING Online
|
| |
|
| Citation |
| DIGITAL OBJECT IDENTIFIER (DOI) |
10.26033/xkmy-me08 (from parent bundle)
|
| AUTHOR LIST |
|
| EDITOR LIST |
Bauer, J. M. and Lawrence, K. J.
|
| PUBLICATION YEAR |
2020
|
| DESCRIPTION |
This is the data_tricam collection for the gbo.ast.neat.survey bundle.
The Near-Earth Asteroid Tracking (NEAT)
project began as a collaborative effort with the United States Air
Force (USAF) in December 1995. It concentrated on the discovery and
observations of near-Earth asteroids and comets, collectively called
near-Earth objects (NEOs). NEAT ended its observations in April 2007.
Throughout its history, NEAT utilized three 1m class telescopes - two
on the Hawaiian island of Maui and the 1.2m Oschin Schmidt telescope
at Palomar Observatory near San Diego, CA. Three unique cameras were
developed and used throughout the program. These data are intended to
be usable for photometric analysis of the various objects within the
NEAT data. Most nights included calibration data, and the lists of
photometric standard calibration fields.
|
| |
|
| Context |
| START DATE TIME |
1996-04-17T12:00:00.000Z
|
| STOP DATE TIME |
2007-04-15T12:00:00.000Z
|
| LOCAL MEAN SOLAR TIME |
|
| LOCAL TRUE SOLAR TIME |
|
| SOLAR LONGITUDE |
|
| PRIMARY RESULT PURPOSE |
SCIENCE
|
| PRIMARY RESULT PROCESSING LEVEL |
Calibrated
|
| PRIMARY RESULT DESCRIPTION |
|
| PRIMARY RESULT WAVELENGTH RANGE |
Visible
|
| PRIMARY RESULT DOMAIN |
|
| PRIMARY RESULT DISCIPLINE NAME |
Imaging
|
| INVESTIGATION |
NO SPECIFIC INVESTIGATION
|
| OBSERVING SYSTEM |
|
| OBSERVING SYSTEM COMPONENT |
NEAT Tri-Cam
Palomar Observatory
1.24/1.83-m Oschin Schmidt photographic equat. telescope
NEAT-Maui Camera
Air Force Maui Optical and Supercomputing Site (AMOS)
Maui Space Surveillance Site (MSSS) 1.2m at Air Force Maui Optical and
Supercomputing Site (AMOS)
NEAT-Maui Camera
Air Force Maui Optical and Supercomputing Site (AMOS)
Ground-based Electro-Optical Deep Space Surveillance (GEODSS at Air Force Maui
Optical and Supercomputing Site (AMOS)
NEAT QUEST Camera
Palomar Observatory
1.24/1.83-m Oschin Schmidt photographic equat. telescope
|
| TARGET |
MULTIPLE ASTEROIDS
DARK
FLAT FIELD
|
| REFERENCES |
|
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