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Polar Winter Differential image motion monitor (PWD)
Polar Winter Differential image motion monitor (PWD)

... • We should operate the day-time DIMM observation next campaign, because this follow up checks the seeing variation of the year exist or not. • We should put the new ultrasonic anemometer at same level of the DIMM. New ultrasonic anemometer brings us CT2 which we couldn’t get previous campaign. • If ...
Connecting The World`s Tallest Mountain The Evolution Of
Connecting The World`s Tallest Mountain The Evolution Of

... ear/nose/sinus congestion can be serious ...
- River Bend Astronomy Club
- River Bend Astronomy Club

... to “send processed images to Holvorcem at high speed via the Internet. The image processing software also has automatic object detection capability, but we visually confirm objects before reporting them.” “Our primary goal,” notes Juels, “is to find a large bright NEO (near-Earth object) moving seve ...
Operations of the Keck AO
Operations of the Keck AO

... Ok, watch PO and/or use pixel location Reliable, yet not optimized for IF and survey mode Automation needed Auto-recovery and automation needed ...


... is a member of our Local Group, the Sculptor dwarf, but before you go peering down your nearest large aperture telescope, this galaxy can only be seen in long exposure photographs on very large telescopes. The stars that make up sculptor are relatively faint, with Alpha Sculptor is shining at magnit ...
Support Astronomer Position - Gran Telescopio CANARIAS
Support Astronomer Position - Gran Telescopio CANARIAS

... attending scientific meetings and for publication fees, computing infrastructure, etc. Applicants must be able to communicate effectively in both English and Spanish, be self-motivated and lively team players with effective problem-solving and inter-personal skills. The ability to work without direc ...
orion® starBlast™ 4.5 EQ
orion® starBlast™ 4.5 EQ

... The EZ Finder II works by projecting a tiny red dot (it’s not a laser beam) onto a lens mounted in the front of the unit. When you look through the EZ Finder II, the red dot will appear to float in space, helping you locate even the faintest of deepsky objects. The red dot is produced by a light-emi ...
a history of the mcmath-pierce solar telescope - NSO
a history of the mcmath-pierce solar telescope - NSO

... the past four decades. Only now are plans being formed for a solar telescope to surpass its 1.6-meter aperture. An unusual all-reflecting optical system was chosen for the McM-P. A 2-meter heliostat feeds a beam to an open-air, unobstructed mirror system that produces an image of the Sun that’s roug ...
Te lescopes - Astromedia AB
Te lescopes - Astromedia AB

... of when we hear the word “telescope.” Refractors have a long, thin tube in which light passes in a straight line from the front objective lens directly to the eyepiece, at the opposite end of the tube. Refractor telescopes have many advantages, including: • Simplicity of design, which translates int ...
doc - IRAM
doc - IRAM

... Short answer/summary: Measurements of electromagnetic interferences and vibrations are under way at the 30m, this should help the instrumental design. Key points of the discussion:  Different detector technologies in 1 cryostat are not compatible.  The 30m cabin is equipped with an optical table m ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

... the place becoming more authentic in my mind for when next I review what Thoreau’s experience has to teach us. If we can work together through the ASP to make the universe in general more authentic to the people we touch by offering direct experience with it, and by providing greater understanding o ...


... must ...
The future of gamma-ray astronomy
The future of gamma-ray astronomy

... This activity was revived after a hiatus of 5 years with more number of mirrors and improved detection methods. For 10 years, an array of Cherenkov telescopes with a total mirror area of about was operated in and around Ooty (Now called Udhagamandalam) in southern India ( ...
IR Universe
IR Universe

...  IRAS also discovered bands of infrared emission that girdle our solar system.  Called the zodiacal dust bands, these are likely to be debris from colliding asteroids.  Two bands appear 9 degrees above and 9 degrees below the ecliptic, which result from debris in an orbit about the sun that is in ...
Introduction to Adaptive Optics
Introduction to Adaptive Optics

... • How is it supposed to work? • How does it really work? • Astronomy with adaptive optics. ...
MS word document
MS word document

... Prof Rebolo opened the meeting by welcoming the attendees and inviting modifications to the agenda. The agenda was adopted and is attached for reference. Prof Gilmore presented an overview of OPTICON, stressing its role of bringing together groups with common problems to develop solutions/opportunit ...
June 2010 - Denver Astronomical Society
June 2010 - Denver Astronomical Society

... Paws for a great Mexican pig-out. Friday morning, and on to Camp Oakes. The schedule was sort of undecided; the camp was supposed to be open to us Wednesday, but with no meal service. It turns out the camp snack bar was open Thursday, but I felt it would be a mess to go, set up camp and then have to ...
The Quest for Object X - Department of Physics and Astronomy
The Quest for Object X - Department of Physics and Astronomy

... involved. The CLEA software provided with this exercise gives you access to a wide range of telescopes, instruments, and analysis software that you can use to analyze the light from an unknown celestial object. You can use these facilities to perform tests that will help you uncover the object’s mos ...
the search for object x
the search for object x

... involved. The CLEA software provided with this exercise gives you access to a wide range of telescopes, instruments, and analysis software that you can use to analyze the light from an unknown celestial object. You can use these facilities to perform tests that will help you uncover the object’s mos ...
Budinoff_3-14
Budinoff_3-14

... Dual pallets allows robot to continue building after it empties a single pallet; a support robot would exchange the empty pallet for a new one. This allows the “working” robot to continuously build independent of pallet count until translation to a new worksite is required ...
instruction manual - Optical Vision Ltd
instruction manual - Optical Vision Ltd

... swivel the telescope around on a plane parallel to your horizon and then tilt it up and down from there (Fig.c). You can think of it as turning your telescope in azimuth until it is facing the horizon below a celestial object and then tilting it up to the object's altitude. However, the Earth rotate ...
OBJXlab
OBJXlab

... involved. The CLEA software provided with this exercise gives you access to a wide range of telescopes, instruments, and analysis software that you can use to analyze the light from an unknown celestial object. You can use these facilities to perform tests that will help you uncover the object’s mos ...
Ay 105 Lab Experiment #2: Geometric optics
Ay 105 Lab Experiment #2: Geometric optics

... you can determine the effective focal length (EFL) for the 6-inch telescope. Make all of your micrometer measurements at a single focus setting. Now move the (micrometer or other, e.g. the Celestron) eyepiece out of the way and perhaps the eyepiece holder which may be threaded into the telescope tub ...
Bioptic telescopes - The College of Optometrists
Bioptic telescopes - The College of Optometrists

... can offer an aid that provides a magnified distance image, thereby improving resolution and reducing associated visual disabilities. Differing from hand-held monocular or binocular telescopes, a bioptic telescope provides a spectacle-mounted hands-free method for magnification at a distance that can ...
Estimating the Cost of Extremely Large Telescopes
Estimating the Cost of Extremely Large Telescopes

... “wish list” fashion. The collection of science modes is then scrutinized to find the tightest requirement on each design parameter, and the science requirements document is then the collection of the tightest requirements. If design studies show that some of the requirements can’t be met, formal app ...
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James Webb Space Telescope



The James Webb Space Telescope (JWST), previously known as Next Generation Space Telescope (NGST), is a space observatory under construction and scheduled to launch in October 2018. The JWST will offer unprecedented resolution and sensitivity from long-wavelength visible to the mid-infrared, and is a successor instrument to the Hubble Space Telescope and the Spitzer Space Telescope. The telescope features a segmented 6.5-meter (21 ft) diameter primary mirror and will be located near the Earth–Sun L2 point. A large sunshield will keep its mirror and four science instruments below 50 K (−220 °C; −370 °F).JWST's capabilities will enable a broad range of investigations across the fields of astronomy and cosmology. One particular goal involves observing some of the most distant objects in the Universe, beyond the reach of current ground and space based instruments. This includes the very first stars, the epoch of reionization, and the formation of the first galaxies. Another goal is understanding the formation of stars and planets. This will include imaging molecular clouds and star-forming clusters, studying the debris disks around stars, direct imaging of planets, and spectroscopic examination of planetary transits.In gestation since 1996, the project represents an international collaboration of about 17 countries led by NASA, and with significant contributions from the European Space Agency and the Canadian Space Agency. It is named after James E. Webb, the second administrator of NASA, who played an integral role in the Apollo program.The JWST has a history of major cost overruns and delays. The first realistic budget estimates were that the observatory would cost $1.6 billion and launch in 2011. NASA has now scheduled the telescope for a 2018 launch. In 2011, the United States House of Representatives voted to terminate funding, after about $3 billion had been spent and 75 percent of its hardware was in production. Funding was restored in compromise legislation with the US Senate, and spending on the program was capped at $8 billion. As of December 2014, the telescope remained on schedule and within budget, but at risk of further delays.
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