|
gptkbp:instanceOf
|
gptkb:photographer
scientific instrument
|
|
gptkbp:completionExpected
|
2024
|
|
gptkbp:dataRate
|
20 terabytes per night
|
|
gptkbp:designedFor
|
gptkb:Legacy_Survey_of_Space_and_Time
|
|
gptkbp:diameter
|
1.65 meters
|
|
gptkbp:exposureModes
|
15 seconds
|
|
gptkbp:fieldOfView
|
9.6 square degrees
|
|
gptkbp:filterCount
|
6
|
|
gptkbp:filterTypes
|
i
y
z
r
u
g
|
|
gptkbp:firstLight
|
2025
|
|
gptkbp:fundedBy
|
gptkb:Department_of_Energy
gptkb:National_Science_Foundation
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
LSST Camera
|
|
gptkbp:length
|
3 meters
|
|
gptkbp:location
|
Cerro Pachón, Chile
|
|
gptkbp:manufacturer
|
gptkb:SLAC_National_Accelerator_Laboratory
|
|
gptkbp:partOf
|
gptkb:Vera_C._Rubin_Observatory
|
|
gptkbp:purpose
|
astronomer
cataloging asteroids
detecting transient astronomical events
mapping the night sky
studying dark matter and dark energy
studying the structure of the Milky Way
|
|
gptkbp:resolution
|
3.2 gigapixels
|
|
gptkbp:sensorCount
|
189
|
|
gptkbp:sensorType
|
CCD
|
|
gptkbp:size
|
10 microns
|
|
gptkbp:startYear
|
2014
|
|
gptkbp:website
|
https://www.lsst.org/camera
|
|
gptkbp:weight
|
approximately 3,000 kg
|
|
gptkbp:bfsParent
|
gptkb:Vera_C._Rubin_Observatory
|
|
gptkbp:bfsLayer
|
5
|