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The top documents tagged [resolution elements]

What is Pan-STARRS? Telescopes –4 x 1.8m –7 square degree FOV –possible sites on Mauna Kea and Haleakala Operation mode: –simultaneous imaging of the same
What is Pan-STARRS? Telescopes –4 x 1.8m –7 square degree FOV –possible sites on Mauna Kea and Haleakala Operation mode: –simultaneous imaging of the same
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FTIR
FTIR
158 views
Multi-color adaptive optics imaging of asteroid 1 Ceres Christophe Dumas, JPL - USA ESO Bill Merline, SwRI - USA Thierry Fusco, ONERA - France
Multi-color adaptive optics imaging of asteroid 1 Ceres Christophe Dumas, JPL - USA ESO Bill Merline, SwRI - USA Thierry Fusco, ONERA - France
216 views
Jan Conrad (KTH, Sthlm) EPNT 06 20 September 2006 1 Upper Limits and Discovery in Search for Exotic Physics Jan Conrad Royal Institute of Technology (KTH)
Jan Conrad (KTH, Sthlm) EPNT 06 20 September 2006 1 Upper Limits and Discovery in Search for Exotic Physics Jan Conrad Royal Institute of Technology (KTH)
213 views
Light Source: Globar Silicon Carbide Rod (5mm diameter, 50 mm long) Heated electrically to 1300 – 1500 K Positive temperature coefficient of resistance
Light Source: Globar Silicon Carbide Rod (5mm diameter, 50 mm long) Heated electrically to 1300 – 1500 K Positive temperature coefficient of resistance
227 views
Possible spectrometers Bent Bragg (after P. Siddons-NSLS) Mosaic crystal Bent Laue –Zhong Zhong-NSLS X-ray Grating –P. Heimann-ALS, S. Hulbert-NSLS
Possible spectrometers Bent Bragg (after P. Siddons-NSLS) Mosaic crystal Bent Laue –Zhong Zhong-NSLS X-ray Grating –P. Heimann-ALS, S. Hulbert-NSLS
221 views
Lecture 3 By Tom Wilson. Summary of Lecture 1 Noise in a Receiver time on source Receiver itself, atmosphere,ground and source Analying bandwidth (for
Lecture 3 By Tom Wilson. Summary of Lecture 1 Noise in a Receiver time on source Receiver itself, atmosphere,ground and source Analying bandwidth (for
218 views
Extragalactic Science Case
Extragalactic Science Case
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Imaging Molecular Gas in a Nearby Starburst Galaxy NGC 3256, a nearby luminous infrared galaxy, as imaged by the SMA. (Left) Integrated CO(2-1) intensity
Imaging Molecular Gas in a Nearby Starburst Galaxy NGC 3256, a nearby luminous infrared galaxy, as imaged by the SMA. (Left) Integrated CO(2-1) intensity
219 views
Theoretical Basis for Public Relations. Theory In Public Relations There is no single theory that covers all public relations and communication. We
Theoretical Basis for Public Relations. Theory In Public Relations There is no single theory that covers all public relations and communication. We
238 views
J. Sánchez Almeida Instituto de Astrofísica de Canarias Magnetometry: set of techniques and procedures to determine the physical properties of a magnetized
J. Sánchez Almeida Instituto de Astrofísica de Canarias Magnetometry: set of techniques and procedures to determine the physical properties of a magnetized
218 views
Future modelling efforts Eelco van Kampen ESO evkampen@eso.org
Future modelling efforts Eelco van Kampen ESO [email protected]
220 views