PPT-L1 TMSY Telescope focal tuning results

Adam Mullavey Chris Guido 31 Oct 2013 LIGO G1400170 Source Parameters MM results EXTERNAL RESULTS Min Max Mean Std Dev Dim. . An appeal by IUA and UNESCO: . “… the citizens of the world rediscover their place in the Universe through the day- and night-time sky observation, and thereby engage a personal sense of wonder and discovery… . Presented . by:. . Rastislav Vajdák. . Senior Test Engineer. . . Oxymat. -Slovakia, s.r.o.. Fine tuning and setting PSA. OC input / output parameters. Tools. Start . o. f system to test . Astronomical Instruments. The Formation of Images. Suppose we want to apply some of the properties of light discussed in the last session?. Recall the refraction of light through a prism?. Forming Images. Integrated Energy. Low/No Cost Solutions through Building Automation System Control Technologies. James Goddard and Danny Taasevigen. Pacific Northwest National Laboratory. August 13, 2015. A . systematic process to identify and correct building operational problems that lead to energy waste. So, if you are not sure, do your best to guess.. Please bring pencil(s) so that you can fill out. the scantrons.. No other accessories (calculators, cell phones, …) are allowed.. Important: Anything in the posted slides that I did not cover in class could be on the exam.. Kadin Tseng. Boston University. Scientific Computing and Visualization. Serial Performance gain. Due to memory access. Due to caching. Due to vector . representations. Due to compiler. Due to other . RED. for Web Traffic. Mikkel Christiansen, Kevin Jeffay,. David Ott, Donelson Smith. UNC, Chapel Hill. SIGCOMM 2000, Stockholm. subsequently. IEEE/ACM Transactions on Networking. Vol. 9 ,  No. 3  (June 2001) pp 249 – 264.. By Hilary . Janysek. What’s the difference?. Intonation: . . (noun) The correct or accurate pitching (placement) of intervals; the capacity to play or sing in tune.. Tuning: . . (verb) to adjust to the correct or given standard of pitch. . Adapted from presentation by Chuck Patterson, Cheyenne, WY, HS teacher. Essential . Questions - . You should be able to answer these questions by the end of the PowerPoint.. What is the purpose of a telescope?. + . Also Affiliated with NSF Center for High-Performance Reconfigurable Computing . Tosiron Adegbija. 1. , Ann Gordon-Ross. 1+. ,. . and . Arslan. Munir. 2. 1. Department . of Electrical and Computer . power. of a lens. Tracing rays to find images from thin convex and concave lenses. . Compound lenses and using intermediate images to find final images. Eyeglasses and prescriptions. Optics Physics 4510. How It Works. Every 97 minutes, Hubble completes a spin around . Earth. .. . As it travels, Hubble's mirror captures light and directs it into its several science . instruments. The Hubble is . a type of telescope known as a . Telescope Specs.. Aperture X f-ratio = f or . fl. 98 x 6.3 = 617 . Eyepiece Focal Length in mm. AFOV - Apparent Field of View. Note: Not present on all Eyepieces. Eyepiece Formulas. Magnification = Telescope focal length ÷ Eyepiece focal length. Bram, Matt and Keita. 20 Oct. 2011. LIGO-G1101254. TMS Telescope. Folded off-axis parabolic telescope. Primary – 9” diameter (228.6 mm). Front telescope aperture 8.5”. Secondary – 1.5” diameter (38.1 mm).