robotic telescopes bremen, 03 22 2005 t. granzer, aip current earth-bound projects
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Robotic Telescopes
Bremen, 03 22 2005
T. Granzer, AIP
Current Earth-bound projects
Why?Costs
Efficiency/speed
Constant data quality
(Arbitrary) long programs
Network:full phase coverageweather independent
Why not?
Troubleshooting
Software demands
Costs
Largest telescopes (VLT, Keck): ~100 M$
Hubble Space Telescope: ~6000 M$
Robotic telescope (1.5m): ~1 M$
AI replaces astronomer
Protect the instrument
Judge weather
Select targets
Operate instruments in right sequence
Protect the instrument
Monitor all system failures
Monitor environment conditionweather(!), computer health, UPS
Emergency planrepair, use of partly defect system
Judge weatherImmediately react on critical conditions
•wind speed, humidity
Predict weather•…saves time
Seeing, clouds•optimize target selection
The scheduling problem
Traditionally: A few nights, few targets tailored to observing period
Robotic: Span entire seasons, lots of targets
An ad-hoc approach not feasible
Approaches:
Queue scheduling:
Prescribe a distinct timeline
Easy to implement
Needs lots of human interference
Cannot react to changing conditions
Approaches (cont‘d):
Optimal scheduling:
Optimize schedule for given time-base.
CPU-intense (N! - permutations).
Unpredicted changes of conditions break schedule.
Difficult with changing weather, but used in space.
Approaches (cont‘d):
Dispatch scheduling:
Picks target according to actual conditions.
Must run in real-time, but N
Allows easy reaction to weather changes.
Used on most current robotic systems.
Current projects
Hawaii
Australia
Texas
La Palma /Tenerife
South Africa
Chile
Arizona
Fairborn Observatory
Washington Camp, Arizona
Fairborn Observatory
14 robotic telescopes, 0.1-2m
First installation world-wide
Mainly Photometry
REM
Focuses on -ray bursts
SWIFT satellite triggers Earth-bound telescopes
Robotic telescopes can react within seconds.
Chile, fully robotic
Project Monet
• Alfred Krupp von Bohlen und Halbach Stiftung
2x1.2m telescopes
Univ. Göttingen, SAAO, McDonald Observatory
App. 50% of total time for 'Hands-On Universe' school-projects
Liverpool & Faulkes
3x 2m Telescopes in La Palma, Hawaii and Australia
Again emphazises acces for schools and students
Robotic & remote modi
Twin-telescope STELLA
Tenerife / Teide2400m Altitude2x 1,2m telescopesAIP/IAC
STELLA
Two 1.2m & 0.8m, f/8 Alt/Az telescopes
Project STELLA
STELLA-I
Echelle Spectrograph, R470002kx2k Marconi chip
STELLA-II
Wide-field imager, 22’ FoV, Strømgren filters4kx4k STA chip
11 26 04
What's next?
Antarctica, Dome C
Exceptional seeing (0".27)
Ideal for AO & IR (high isoplanatic angle of 7".9)
'Half step' to Moon/Space
see also Lawrence, Nature 431, 278L
Shackleton@Moon?
lower pic. Margot/Cornell U
Passive cooling to 50K
Stable platform
No Expendables, no gyros
Fixed telescope for ultra-deep fields
Data rate ~50Mbyt/s (64x64k@1/600 Hz)
see also Angel, SPIE 5487, p.1
…but start realistic
Start with a ~4m precursorExperience with 4m class robotic telescopes (~10 ys.)
Possible benefits from Antarctica telescopes (~10 ys.)