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.
FTIR
Multi-color adaptive optics imaging of asteroid 1 Ceres Christophe Dumas, JPL - USA ESO Bill Merline, SwRI - USA Thierry Fusco, ONERA - France.
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)
Light Source: Globar Silicon Carbide Rod (5mm diameter, 50 mm long) Heated electrically to 1300 – 1500 K Positive temperature coefficient of resistance.
Possible spectrometers Bent Bragg (after P. Siddons-NSLS) Mosaic crystal Bent Laue –Zhong Zhong-NSLS X-ray Grating –P. Heimann-ALS, S. Hulbert-NSLS.
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.
Extragalactic Science Case
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.
Theoretical Basis for Public Relations. Theory In Public Relations There is no single theory that covers all public relations and communication. We.
J. Sánchez Almeida Instituto de Astrofísica de Canarias Magnetometry: set of techniques and procedures to determine the physical properties of a magnetized.
Future modelling efforts Eelco van Kampen ESO [email protected].
