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Where to Put the Telescope
Where to Put the Telescope

... Post-9.2: The NASA Infrared Telescope Facility and the United Kingdom Infrared Telescope operate on the top of Mauna Kea, Hawai’i. If the atmosphere absorbs infrared radiation, how is it that these telescopes can observe at these wavelengths? ...
Electromagnetic Spectrum Ppt
Electromagnetic Spectrum Ppt

... • HOWEVER, TELESCOPES IN SPACE CAN COLLECT ENERGY AT ALL WAVELENGTHS! ...
CSOF3 - CSIRO
CSOF3 - CSIRO

... Delivering on Commitments Health, Safety & Sustainability ...
The Imaging Chain for Optical Astronomy
The Imaging Chain for Optical Astronomy

... – fast processing turnaround (CCD readout speeds ~1 sec) • NO development of emulsion! ...
XMM - advanced X-ray Astronomy school - X
XMM - advanced X-ray Astronomy school - X

... (this is the light from a point source will be spread in (almost) a Gaussian with the above dimensions). Although the spatial resolution in all telescopes is dictated by Airy’s law which says that for a given telescope diameter, the resolution (decreases) gets better with decreasing wavelength. Howe ...
The Catalina Sky Survey NEO Follow-up
The Catalina Sky Survey NEO Follow-up

... • 100% dedicated to NEO survey + follow-up • Assets: 3 survey telescopes + 1 follow up telescope • Cadence: 4 x 30 s images, deltaT ~10 min. ...
THE LAS CAMPANAS INFRARED SURVEY CAMERA S. E. Persson
THE LAS CAMPANAS INFRARED SURVEY CAMERA S. E. Persson

... Recent rapid improvement in the quality and size of nearinfrared imaging array detectors has led to great advances in many areas of astronomy, and the time is opportune to apply them to ambitious surveys. The camera described in this paper has been developed for the purpose of conducting deep (Ks  ...
telescopes I
telescopes I

... instrument, c.f. a spectrograph, spectropolarimeter, magnetograph, Fabry-Pérot interferometer....) ...
Transparencies - Rencontres de Moriond
Transparencies - Rencontres de Moriond

... Two experiments: two decades Multiwavelength campaigns Correlation studies Change hardness during flares (Krennrich et al, ICRC 2003) Light curves, look for fast flares ...
Introduction - WordPress.com
Introduction - WordPress.com

... Potentially the highest bandwidth (>100kHz) ...
G-CLEF Summary
G-CLEF Summary

Slide 1
Slide 1

The Revolution in Telescope Aperture
The Revolution in Telescope Aperture

... f/1.2 8-m mirror is measured in millimetres (1.19 mm) rather than micrometres. In addition, the active support systems used in the telescope can correct any large-scale errors, and polishers can now concentrate on local smoothness. The result is 8-m diameter mirrors that can perform near the diffrac ...
FIRSTSCOPE 60 - MODELS #21055 and #21055-DX
FIRSTSCOPE 60 - MODELS #21055 and #21055-DX

... sharpest possible focus. If you have astigmatism, corrective lenses must be worn at all times. ...
22-Laser
22-Laser

... lower 2p53p state resulting in 632.8 nm visible light and 1.15 μm infrared radiation respectively. The gas mixture is contained in a glass tube with highly reflective mirrors at each end which cause standing waves of wavelength 632.8 nm to be set up, but also permit a small fraction of the radiation ...
Figure 33.1: The 1m-Reflector of Hamburg Observatory
Figure 33.1: The 1m-Reflector of Hamburg Observatory

... Within the scope of my diploma thesis, supervised by Prof. Dr. Keller-Kempas on behalf of the FHTW/University of Applied Sciences Berlin and Prof. Dr. Gudrun Wolfschmidt on behalf of the University of Hamburg, I have developed a concept of preservation for the 1 m-reflector (see Fig. 33.2A) of the H ...
GRIS: The GREGOR Infrared Spectrograph
GRIS: The GREGOR Infrared Spectrograph

... of the support of all optical elements to avoid any stresses that may distort image quality. This is a delicate issue in the case of the grating, because of its weight. Since it is located at a pupil plane, any deformation will have an impact on the reflected wavefront quality. The grating lies over ...
LHDC High-Performance Fine-Steering Mirror Family
LHDC High-Performance Fine-Steering Mirror Family

Hubble Space Telescope - University of Southern California
Hubble Space Telescope - University of Southern California

... • Instruments: The Wide Field Planetary Camera (JPL) consists of four cameras that are used for general astronomical observations from far-UV to near-IR. The Faint Object Camera (ESA) uses cumulative exposures to study faint objects. The Faint Object Spectrograph (FOS) is used to analyze the propert ...
The Night Sky - Forest Holidays
The Night Sky - Forest Holidays

... drawing of a house, complete with roof • Orion (the hunter), with belt and sword, is perhaps the most famous constellation – and one of the few that actually bears some slight resemblance to its namesake ...
23.1 Telescopes - Ms. Billings Website
23.1 Telescopes - Ms. Billings Website

... telescopes are called? Radio telescopes look a lot like satellite dishes because both are designed to do the same thing —to collect and focus radio waves or microwaves (the shortest wavelength waves) from space. The largest single telescope in the world is at the Arecibo Observatory in Puerto Rico ( ...
scope buyer`s guide - Astronomy Magazine
scope buyer`s guide - Astronomy Magazine

... 152ED is Meade’s 6-inch f/9 model. Other telescopes in this line (all f/9) are the 102ED (4-inch), 127ED (5-inch), and 178ED (7-inch). In each case, ED stands for “extra-low dispersion,” which refers to the type of glass used in the second element of the objective lens. Using a twoelement lens syste ...
globular clusters - Jeremiah Horrocks Institute
globular clusters - Jeremiah Horrocks Institute

... The Moses Holden Telescope at Alston Observatory is still in the process of being commissioned, but it has already been used to image some deep-sky objects, such as nebulae, globular clusters and distant galaxies. The telescope has a very large collecting area, which allows it to detect these faint ...
Chapter 6 Telescopes: Portals of Discovery How does your eye form
Chapter 6 Telescopes: Portals of Discovery How does your eye form

... –! It uses refraction to bend parallel light rays so that they form an image. –! The image is in focus if the focal plane is at the retina. •! How do we record images? –! Cameras focus light like your eye and record the image with a detector. –! The detectors (CCDs) in digital cameras are like those ...
Observatory project to see first light in holiday season
Observatory project to see first light in holiday season

... According to Mr. Janover, the facility will be extremely beneficial to the Wall Township community. Students will explore and investigate a wide range of cosmological objects and events while gaining hands-on experience in the use and maintenance of astronomical equipment. The observatory is meant ...
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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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