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"Identification of High Energy Cosmic Ray Electrons using Advanced Techniques in Fermi LAT and CALET"
"Identification of High Energy Cosmic Ray Electrons using Advanced Techniques in Fermi LAT and CALET"

... University of Denver Department of Physics & Astronomy Measurements of the cosmic ray electron spectrum have received much attention over the last decade as anomalies in both electron and positron observations have been detected independently by several experiments. The profound possible implication ...
Adding TDI mode to PRISM - Harvard–Smithsonian Center
Adding TDI mode to PRISM - Harvard–Smithsonian Center

Telescopes & Electromagnetic Radiation
Telescopes & Electromagnetic Radiation

... As you stated, this galaxy is known for its edge-on view of the very bright core and broad ring of obscuring dust. It is one of the largest galaxies at the southern edge of the Virgo Galaxy Cluster. It was also the first galaxy found to have a large redshift in its spectrum, meaning it is moving awa ...
section 6 powerpoint
section 6 powerpoint

Astronomy: The Original Science
Astronomy: The Original Science

... 1 Describe two early ideas about the structure of the universe. 2. Describe the contributions of Brahe, Kepler, Galileo, Newton, and Hubble to modern astronomy ...
Microsoft PowerPoint - file [jen pro \350ten\355]
Microsoft PowerPoint - file [jen pro \350ten\355]

... aberration for refractor telescope by a lens design – kept secret • 1759 - it was uncovered and used commercially by John Dolland and his son • 1930 - Bernhard Schmidt – his telescope serves astronomy as a wide angle camera ...
NIE10x301Sponsor Thank You (Page 1)
NIE10x301Sponsor Thank You (Page 1)

... Some of the most important things Galileo discovered during 1609 with his telescope were the rings of Saturn, the moons of Jupiter, and the phases of Venus and craters on the moon. These observations began the human exploration of the Universe with the aid of telescopes and the modern science of Ast ...
Reminiscing about Mt. Wilson 60
Reminiscing about Mt. Wilson 60

... same location several times in a minute. This happens with objects or details that are JUST at the limit of visibility. But there was also detail in the B-ring (note the shading at the ends), and the C-ring which was plainly visible. ...
Large Diameter Telescopes
Large Diameter Telescopes

... Save My Exams! – The Home of Revision For more awesome GCSE and A level resources, visit us at www.savemyexams.co.uk/ ...
186,000 miles per second
186,000 miles per second

... The larger the opening, the greater the light gathering ability A= ∏(r)2 So, if you double the size of the telescope, it increases its light gathering potential by ____? ...
04 Astronomical Tools
04 Astronomical Tools

... Computer-controlled mirror supports adjust the mirror surface (many times per second) to compensate for distortions by atmospheric turbulence ...
Telescopes
Telescopes

... if they are seen as two separate points. Smallest angle resolved is proportional to 1/D. ...
Telescopes
Telescopes

... Surface accuracy not so important, so easy to make large one. ...
Heritage-130P review July16 Astronomy Now
Heritage-130P review July16 Astronomy Now

... until the sharpest images are obtained. Although it takes a bit of getting used to, I found it worked perfectly well in field tests. Care must be made not to unscrew the eyepiece holder too far, lest it come loose from the instrument proper. Most any eyepiece and/or Barlow combinations will come to ...
24.1 The Study of Light - Buncombe County Schools System
24.1 The Study of Light - Buncombe County Schools System

Telesopes
Telesopes

60-inch Mirror Successfully Re-aluminized in August
60-inch Mirror Successfully Re-aluminized in August

... An exploding star is called a supernova. Astronomers have been systematically hunting them since Fritz Zwicky began his first survey for them with Palomar’s 18-inch Schmidt telescope in 1936. Dr. Zwicky found 120 of them in his lifetime. Modern astronomers have kicked supernova hunting into high gea ...
reflecting telescope
reflecting telescope

... – Adaptive optics: sensors monitor distortions due to atmosphere and correct the shape of the mirror 10 to 100 times per second ...
1. History of Telescopes
1. History of Telescopes

... An object placed at any one of these 5 points will stay in place relative to the other two. ...
Slide 1 - Teacherpage
Slide 1 - Teacherpage

... • Temperatures measure heat and cold. • The temperatures in July are hot. • What are the temperatures in December? ...
Webster, Using SDSS Images, Jan. 6, 2009
Webster, Using SDSS Images, Jan. 6, 2009

Presentation UE6
Presentation UE6

... If the change is periodical it can be assumed is due to an orbiting planet ...
Click here to get the file
Click here to get the file

... Characteristics of the Field Corrector at Prime Focus We have set the condition that image quality in the focal plane will not be limited by telescope optics, rather by seeing and mechanical effects. To meet this condition, a 3-element field corrector, will be used to focus a 15 cm diameter focal p ...
Proposal memo example - University of Portland
Proposal memo example - University of Portland

... is $200 for materials and 100 hours of design a construction time. See Attachments for schedule and figures. Introduction The current telescope designed, built and owned by the author occupies substantial room in a vehicle while transporting it to observing sites. It is desired to have a telescope t ...
prof.-j.hill
prof.-j.hill

... aperture. The two Gregorian telescope sides point at the same object, or groups of objects close together (1 arcmin) on the sky. A unique feature of LBT is that the light from the two primary mirrors can be combined in the center of the telescope to produce phased-array imaging of an extended field ...
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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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