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497 Autostar Manual for DS-2090AT-TC and DS-2102AT-TC
497 Autostar Manual for DS-2090AT-TC and DS-2102AT-TC

... entered. The alignment stars may change from night to night. All that is required is for the observer to center the selected stars in the eyepiece when prompted. NOTE: The GO TO key also allows you to perform a "spiral search." A spiral search is useful when the telescope slews to an object, but tha ...
01 DS-114AT manual final.qxd
01 DS-114AT manual final.qxd

... Often, club members are excellent astrophotographers. Not only will you be able to study examples of their art, but you may even be able to pick up some “tricks of the trade” to try out on your DS-114AT telescope. Many groups hold regularly scheduled star parties at which you can observe with many d ...
OBSERVATIONS OF PHYSICAL PROCESSES IN
OBSERVATIONS OF PHYSICAL PROCESSES IN

... joint project of the Ministério da Ciência, Tecnologia, e Inovação (MCTI) da República Federativa do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU). Support for this thesis was provided b ...
Untitled - Cambridge University Library
Untitled - Cambridge University Library

... Huygens had sent on 21 June. Newton’s reply was composed at Stoke on 8 July. He acknowledged Huygens’ remarks and asked about the progress of Christopher Cock, a London instrument maker, who was building a four-foot reflecting telescope with metal mirrors and also making trials of much shorter telesc ...
Astronomical imaging using ground
Astronomical imaging using ground

... the dynamic focus optics and a single electronically shuttered CCD. A prism array divides the pupil into 60 subapertures of equal area arranged in a hexapolar geometry. Substantial improvements to the optics have been made, increasing throughput and SNR, allowing the LGS WFS to run at a faster 460+ ...
optics7
optics7

... should be able to read 1M print (standard size reading material) with a add power of (100/20 = 5) +5.00 sphere.  Test circumstances such as illumination, contrast, and target type must be kept precisely the same……………..this is most of the time unable to be performed ...
instruction manual - NexStar Resource Site
instruction manual - NexStar Resource Site

... should keep this manual handy until you have fully mastered your telescope’s operation. The StarSeeker hand control has built-in instructions to guide you through all the alignment procedures needed to have the telescope up and running in minutes. Use this manual in conjunction with the on-screen in ...
T1000311-v7 TMS Hazards Analysis - DCC
T1000311-v7 TMS Hazards Analysis - DCC

... approximately ¼ in above the assembly table by raise the leveling pad feet of the Balance Bridge iteratively until the TMS Telescope Frame Assembly/ISC Table Assembly is supported by the TMS Tele-Opt Table Balance Bridge Pin that is mounted to the TMS Tele Alignment Support Bridge Assembly. The asse ...
Orion SkyView Pro™ 127 EQ Telescope Instruction Manual
Orion SkyView Pro™ 127 EQ Telescope Instruction Manual

... Assembling the telescope for the first time should take about 30 minutes. No tools are needed other than the ones provided. All screws should be tightened securely, but be careful not to over-tighten or the threads may strip. Refer to Figure 1 during the assembly process. ...
NS2-M3C12S2_-_The_Radiotelescope
NS2-M3C12S2_-_The_Radiotelescope

... Eifel Mountain near Bonn, Germany ...
PDF - WM Keck Observatory
PDF - WM Keck Observatory

... coordinates  and  organizes  the  outreach  efforts  of  the  Maunakea  Observatories,  and  acts   as  a  community  forum  for  the  observatories,  related  organizations  and  the  Maunakea   Visitor  Information  Station  (MKVIS).    MKA ...
p of the Sky
p of the Sky

... • Center for Theoretical Physics PAS, Warsaw • Warsaw University • Warsaw University of Technology ...
Chandra Telescope Optical Axis and Aimpoint Ping Zhao Chandra X-ray Center
Chandra Telescope Optical Axis and Aimpoint Ping Zhao Chandra X-ray Center

Lecture Notes and Essays in Astrophysics VOLUME III
Lecture Notes and Essays in Astrophysics VOLUME III

... zonal winds in the Southern hemisphere at altitudes ranging from 47 to 66 km are nearly constant with latitude with westward velocities of 105 m/s at cloud-tops and 60-70 m/s at the cloud-base. At high latitudes, zonal wind speeds decrease linearly with virtually no vertical wind shear, indicating a ...
History - Astrophysical Research Consortium
History - Astrophysical Research Consortium

... project), and they needed a partnership with other astronomy departments because their small, but growing faculty would underutilize and have difficulty managing a large facility (Wallerstein 2004). As early as October 1965 the UW Regents authorized construction of a large telescope using external ...
Leica Nova MS50 - White Paper
Leica Nova MS50 - White Paper

... measurements. The possibility to capture images of each measured point improves the documentation of the field work. Furthermore, sketching functionality allows making notations directly in the images for better understanding of what has been measured. The high resolution images from both cameras ca ...
Orion StarMax 127 EQ Manual
Orion StarMax 127 EQ Manual

... WARNING: Never look directly at the Sun through your telescope or its finder scope— even for an instant—without a professionally made solar filter that completely covers the front of the instrument, or permanent eye damage could result. Young children should use this telescope only with adult superv ...
PATBNTED OCT. 29. 1907. TELESCOPE.
PATBNTED OCT. 29. 1907. TELESCOPE.

View
View

... fully mastered your telescope’s operation. The LCM hand control has built-in instructions to guide you through all the alignment procedures needed to have the telescope up and running in minutes. Use this manual in conjunction with the on-screen instructions provided by the hand control. The manual ...
Correcting Systematic Poalrization Effects in Keck LRISp
Correcting Systematic Poalrization Effects in Keck LRISp

... environments when signal to noise ratios (SNRs) above 2000 can be achieved. The LRISp spectropolarimeter is capable of achieving these SNRs on faint targets with the 10m aperture of the Keck telescope, provided several instrumental artifacts can be suppressed. We describe here several methods to ove ...
Catchers Introduction - Astrophotography for Astrophotographers
Catchers Introduction - Astrophotography for Astrophotographers

... During the course of the six years it has taken me to research and write the ‘Catchers of the Light’, I have been helped by many individuals and organizations. In the main this assistance has been confined to the provision of information, documents and photographs; and for this I am especially grate ...
DOBSONIAN TELESCOPE - Raleigh Astronomy Club
DOBSONIAN TELESCOPE - Raleigh Astronomy Club

... mastered the basics and ready for new, more challenging observations. The final part of this manual contains a list of objects that can be observed through your Celestar telescope. Included are the coordinates for each object, its brightness, and a code which indicates what type of an object it is. ...
Outline Thesis – so far
Outline Thesis – so far

... strong aberrations caused by the large off-axis distance. To match the wavefront of the beacons‟ images to the desired precision of 50 nanometres rms, I designed a custom objective, incorporating a computer generated hologram to shape the wavefronts of three optical fibres forming the light sources. ...
LCM SerieS
LCM SerieS

... Congratulations on your purchase of the Celestron LCM telescope! The LCM ushers in a whole new generation of computer automated technology. Simple and friendly to use, the LCM telescope is up and running after locating just three bright celestial objects. It’s the perfect combination of power and po ...
The following is a supplemental addendum to the included
The following is a supplemental addendum to the included

... Once centered, press the UNDO button until you are at the main menu. With CGE Ready displayed, press the ALIGN key on the hand control. Use the Up/Down buttons and select the Alignment Stars option and press ENTER. The display will then ask you which alignment star you want to replace. Use the UP an ...
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XMM-Newton



The XMM-Newton, also known as the X-ray Multi-Mirror Mission and the High Throughput X-ray Spectroscopy Mission, is an orbiting X-ray observatory launched by ESA in December 1999 on an Ariane 5 rocket. It is named in honor of Sir Isaac Newton. The telescope was placed in a very eccentric 48 hour elliptical orbit at 40°; at its apogee it is nearly 114,000 kilometres (71,000 mi) from Earth, while the perigee is only 7,000 kilometres (4,300 mi).
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