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The last gasps of VY CMa: Aperture synthesis and adaptive optics
The last gasps of VY CMa: Aperture synthesis and adaptive optics

... 1992). Assuming the polarization arises from Rayleigh scattering, these observations suggest an asymmetric near-IR brightness distribution extending toward PA 170◦ (or PA -10◦ ). This is in close agreement with the new high resolution results presented in Figure 2. The 10-m baselines afforded by the ...
transparencies - Rencontres de Moriond
transparencies - Rencontres de Moriond

... Milagro can provide sorely needed alerts for Cherenkov telescopes. Pointing instruments (e.g. air Cherenkov) generally have better sensitivity than survey instruments. Counter example: Glast. Narrow field-of-view problems: i) you necessarily have an a priori discovery goal - serendipity almost rule ...
SOFIA Engineering Meeting 12-May-2011
SOFIA Engineering Meeting 12-May-2011

... – SOFIA is an observatory, not a mission – Given constraints of airplane, flight plans, etc., need to observe multiple p targets g each flight g to maximize relativelyy small observingg time (only 1000 hours per year in full opertations) Al working on sensitivity calculator for SOFIA with 1000K and ...
chapter9-Section2
chapter9-Section2

... • Since the 1980s, several telescopes have been ...
Skyscraper How to Color the Universe by Kim Arcand the
Skyscraper How to Color the Universe by Kim Arcand the

G030033-00 - DCC
G030033-00 - DCC

...  Sensor/actuators (OSEMs) for the all the suspended optics were assembled, cleaned and baked, tested, and prepared for installation. Three core optics (Beamsplitter, ITMx, and ITMy) were suspended and damped in February 2003. Four remain to be suspended by the summer 2003. Remaining optical sensi ...
LaPalma_telescopes_2008
LaPalma_telescopes_2008

... Gregorians may be easier to make and can be better baffled in some cases. 23rd June 2008 ...
4. Overview of combined internal and external NGAO interface
4. Overview of combined internal and external NGAO interface

... A preliminary NGAO overall N-squared diagram is given in Figure 3. The reader should also look at the associated spread sheet, as it maybe easier to read the figures in it than this word document. For the purposes of Figure 3, the telescope, observatory facilities, and the instrument are considered ...
Article PDF - IOPscience
Article PDF - IOPscience

... than the two-point correlation length, then the likelihood can be calculated as ...
Telescopes
Telescopes

... 1. Can observe 24 hours a day 2. Clouds, rain, and snow don’t interfere 3. Observations at an entirely different frequency; get totally different information ...
Lecture #1 Basic Concepts and Principles of Adaptive Optics
Lecture #1 Basic Concepts and Principles of Adaptive Optics

Spectral Line VLBI
Spectral Line VLBI

Origami Sunshield Concepts for Space Telescopes Lee Wilson and Sergio Pellegrino Rolf Danner
Origami Sunshield Concepts for Space Telescopes Lee Wilson and Sergio Pellegrino Rolf Danner

... instead of using two Type 2 corners as in the original scheme, the best solution identified utilizes two Type 1 corners and six Type 2 to obtain a hexagonal prism in the fully deployed configuration, as shown in Figure 13. The Type 2 corners provide the basic hexagonal prism shape and the Type 1 cor ...
ISNS3371_040507_bw - The University of Texas at Dallas
ISNS3371_040507_bw - The University of Texas at Dallas

... The eye consists of pupil that allows light into the eye - it controls the amount of light allowed in through the lens - acts like a simple glass lens which focuses the light on the retina - which consists of light sensitive cells that send signals to the brain via the optic nerve. An eye with perfe ...
T1000700-v2 Transmon Telescope Mirror Test Procedure
T1000700-v2 Transmon Telescope Mirror Test Procedure

... Firmly attach the base of the autocollimator mounting post to the Newport table at the desired location that defines the position of the Primary mirror beam line. Move the autocollimator vertically on the post to approximately 5.13 in above the granite table. Place the corner cube at the output of t ...
Optical Fabrication and Testing - National Optical Astronomy
Optical Fabrication and Testing - National Optical Astronomy

... Cost-effective segment fabrication Characterization of wind loading Hierarchical control systems ...
SCA Laser Collimator for SCT
SCA Laser Collimator for SCT

... even though star testing would indicate perfect collimation. In addition, the secondary mirror, convex shape, magnifies any error by about 5 times. The error of deviation for a typical well collimated SCT will return laser beam at around 0.125" to 0.250" off center. In order to compensate the mechan ...
Lecture ppt - UCO/Lick Observatory
Lecture ppt - UCO/Lick Observatory

apt/astap/rept-09 - Asia
apt/astap/rept-09 - Asia

... FOV(field of view): The acceptance angle (of an FSO receiver) is the angle between the lines at which the power detected by the receiver falls to 1/e2 in this report. There is some other definitions whose power levels fall to 1/e or 1/2. The angle is always referred in full width. Optical antenna: O ...


... the periphery of the observable electromagnetic spectrum, the VHE band must now be considered a legitimate astronomical discipline with established sources, both steady and variable, both galactic and extragalactic, a growing number of observatories, and the promise of significant advances in detect ...
Introduction to SkyMaker and the STEP 1 simulations
Introduction to SkyMaker and the STEP 1 simulations

... What is skymaker? Skymaker makes realistic sky simulations with the main emphasis on reproducing observational effects: - telescope aperture - Optical defects (e.g. astigmatism, coma, tracking errors) - detector and sky characteristics (gain, sky brightness, saturation effects) - halos around bright ...
Slides in ppt
Slides in ppt

... Proofs of Earth's motion ...
Table C5. Vertical Wind and Temperature
Table C5. Vertical Wind and Temperature

... resolution, sensitivity and range of many systems are still limited by signal levels. Experiments conducted during the past fifteen years using the 3-meter class telescopes at the Starfire Optical Range, NM and Haleakala, Maui (Maui/MALT Program) demonstrated clearly the substantial scientific advan ...
The effect of the Fluorescence Yield selection on
The effect of the Fluorescence Yield selection on

... (absolute value, wavelength spectrum and atmospheric dependency). The comparison of the energy spectra of Auger and HiRes/TA indicates a possible disagreement in the energy scale [1], which could be partly due to using different fluorescence yield data. In this work we evaluate the effect of the flu ...
Astrometry: Revealing the Other Two Dimensions of
Astrometry: Revealing the Other Two Dimensions of

... Galileo was interested in double stars as a means for proving the heliocentric theory. He assumed systems were optical in nature. ...
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CfA 1.2 m Millimeter-Wave Telescope

The 1.2 meter Millimeter-Wave Telescope at the Harvard-Smithsonian Center for Astrophysics and its twin instrument at CTIO in Chile have been studying the distribution and properties of molecular clouds in our Galaxy and its nearest neighbours since the 1970s. The telescope is nicknamed ""The Mini"" because of its unusually small size. At the time it was built, it was the smallest radio telescope in the world. Together, ""The Mini"" and its twin in Chile have obtained what is by far the most extensive, uniform, and widely used Galactic survey of interstellar carbon monoxide (CO). ""The Mini"" is currently in operation from October to May each year.
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