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Profile Documents Logout
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Slides
Slides

... Grazing angle reflection only! Nested metallic mirrors Paraboloid+Hyperboloid surfaces ...
Astronomy - SAVE MY EXAMS!
Astronomy - SAVE MY EXAMS!

... For more awesome GCSE and A level resources, visit us at www.savemyexams.co.uk/ ...
ch6
ch6

... • Why do we put telescopes into space? – Forms of light other than radio and visible do not pass through Earth's atmosphere. – Also, much sharper images are possible because there is no turbulence. © 2014 Pearson Education, Inc. ...
Wolf 94.. - Centre for Astrophysics Research (CAR)
Wolf 94.. - Centre for Astrophysics Research (CAR)

... The object is thought to have formed like a star, but has ended up looking more like Jupiter. It is roughly the same size, despite being between 20 and 30 times as heavy, and when the infrared spectral "fingerprints" of the two objects are compared, their resemblance is striking. The new object orbi ...
OSA6Challenges and opportunities - DU Portfolio
OSA6Challenges and opportunities - DU Portfolio

... transportation make Mt. Evans an appropriate site for a significant astronomical facility. An unusual dual-aperture 28.5-inch, f/21 Ritchey-Chretien telescope has been completed and installed in the high altitude observatory facility, with first light August 1997. It was designed by Eric T. Meyer to ...
Buying A Telescope
Buying A Telescope

... objects because of its larger aperture. Whatever you decide, don’t forget to add in the cost of extra eyepieces if desired, a sky map or planisphere, subscription, and any other accessories that might be needed. If you have $400-$700 to spend - You’ll find tons of telescopes in this price range. For ...
How Telescopes Work.
How Telescopes Work.

... What does it mean to have a diffraction limit? If two astronomical sources are closer together than this, they will appear as one blurred source. In principle it may still be possible to deblend them, by looking for marginal elongations of the image, but it’s hard and requires very high quality data ...
Word - NASA Infrared Telescope Facility
Word - NASA Infrared Telescope Facility

... This document will attempt to present the potential hazards connected with operating the IRTF as it relates to the TCS and how the TCS3 and associated systems negate these hazards to put the telescope in a safe condition for operation, maintenance, and facility protection. This document will mainly ...
Lenses - singhscience
Lenses - singhscience

... creates a real image within a telescope of a distant object. Eyepiece lens – magnifies the image of a distant object. ...
TELESKOOPPI / KAUKOPUTKI
TELESKOOPPI / KAUKOPUTKI

... MIKA HANHILA OPTICS AND SPETROSCOPY ...
A modern physics laboratory activity: Radio astronomical observations of recombination lines
A modern physics laboratory activity: Radio astronomical observations of recombination lines

... measured in the modern physics laboratory if they were not measured in general physics. Perhaps the visible spectrum of deuterium is calculated and measured to show the effect of changing M. Observations of recombination lines provide another example of the quantum mechanical model of atoms. Using t ...
Large Astronomical Telescope Development in China
Large Astronomical Telescope Development in China

... large field of view. Needed in such kind of observations are large-aperture optical/infrared telescopes of general type, which unfortunately are missing in China and even Asia. Considering the reflective area of its main mirrors, the effective illumination diameter of LAMOST is 7.8m, with a 6.67m×6. ...
For teachers who attended without students
For teachers who attended without students

... [teacher name] a [grade] teacher at [insert school here] recently completed scientific training at the National Radio Astronomy Observatory (NRAO) in Green Bank, West Virginia. In the coming school year, s/he will recruit and train students to join an international team of astronomers in searching f ...
Light Source Test at the Telescope Array Site
Light Source Test at the Telescope Array Site

... 20 flights in TA site on Oct. 14, 15, and 16 in last year. We had analyzed the four calibration operation data to the center PMT 77 in camera 07 which the distance between the octocopter and the mirror is about 1.0 km. The standard deviation of the octocopter position for the flights are less than a ...
Internet URLs
Internet URLs

... This site is an absolute must if you plan to chase any solar eclipses. It is maintained by NASA scientist, Fred Espenak, who often writes eclipse articles for S&T and Astronomy. ...
Buying Your First Telescope - Naples Free-Net
Buying Your First Telescope - Naples Free-Net

... If you have gotten this far you must be fairly serious about buying a telescope. Above is a list of four considerations that must be taken into account before purchase – I also hinted some possible workarounds if one or more of these considerations is preventing you from owning your dream telescope ...
Notes on telescopes
Notes on telescopes

... A light curve represents a series of brightness measurements made over a period of time. ...
DTU 8e Chap 3 Light and Telescopes
DTU 8e Chap 3 Light and Telescopes

... resolving power comparable to the Hubble Space Telescope. ...
Loan-A-Scope Program FAQ
Loan-A-Scope Program FAQ

... If the telescope is a GEM mount with a simple tracking motor, make sure the motor is properly engaging and running. You should be able to hear a hum or whine from the motor. If not, check that it is getting power and if it has LED’s, that some are on. If not, check the power source/change the batter ...
Lecture 7
Lecture 7

... The  Hubble  Space  Telescope  overcame  the  limits  of  seeing  by  going  into  space.    In  recent  years,  it  has  become  possible  to  achieve diffraction­limited imaging from the ground. One  way  of  doing  this  is  called  lucky  imaging.    You  simply  take  a  huge  number  of  image ...
Telescopes
Telescopes

... Concave spherical primary Convex spherical secondary - Spherical corrector lens plate removes first order spherical aberration - Tend to have narrower field of view than Schmidt-Cassegrains due to longer focal length - Invented by Dmitri Maksutov (1896-1964) - Does not scale very well with large ape ...
Instruments
Instruments

... He explained two advantages, - Angular resolution - Different wavelength that is absorbed by Earth atmosphere ...
Portable Speckle Interferometry Camera Checkout at Kitt Peak
Portable Speckle Interferometry Camera Checkout at Kitt Peak

... The National Optical Astronomy Observatory (NOAO) Time Allocation Committee (TAC) awarded eight nights on the 2.1m telescope at Kitt Peak National Observatory for double star speckle interferometry using a portable camera. As described in the proposal, binary orbits, when combined with parallaxes, y ...
Inside… - College of San Mateo
Inside… - College of San Mateo

... With these instruments, our students have been graphing the light curve of intrinsic variable stars, as well as eclipsing binaries, in order to determine their period. They will be analyzing the spectrum of stars to determine their spectral type as part of their laboratory work. Our one of a kind ob ...
CSOF3 - CSIRO
CSOF3 - CSIRO

... CSIRO Astronomy and Space Science (CASS) is completing instrumentation of the Australian SKA Pathfinder (ASKAP) telescope at the Murchison Radio-astronomy Observatory (MRO) in mid-west WA and is seeking an experienced, qualified Optical Fibre & Cabling Technician to join a small dedicated team of te ...
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Allen Telescope Array



The Allen Telescope Array (ATA), formerly known as the One Hectare Telescope (1hT) is a radio telescope array dedicated to astronomical observations and a simultaneous Search for Extraterrestrial Intelligence (SETI). The array is situated at the Hat Creek Radio Observatory, 290 miles (470 km) northeast of San Francisco, California.Originally developed as a joint effort between the SETI Institute and the Radio Astronomy Laboratory (RAL) at the University of California, Berkeley (UC Berkley) with funds obtained from an initial US$11.5 million donation by the Paul G. Allen Family Foundation, the project completed the first phase of construction and become operational on 11 October 2007 with 42 antennas (ATA-42), after Paul Allen (co-founder of Microsoft) pledged an additional $13.5 million to support the construction of the first and second phases.Though overall Allen has contributed more than $30 million to the project, the project has not succeeded in building the 350 six metre (19.7 feet) dishes originally conceived, and suffered an operational hiatus due to funding shortfalls between April and August 2011. Subsequently, UC Berkeley exited the project, completing divestment in April 2012. The facility is now managed by SRI International (formerly Stanford Research Institute), an independent, nonprofit research institute.In August 2014 the installation was threatened by a forest fire in the area and was briefly forced to shut down, but ultimately emerged largely unscathed.
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