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141. spectrographic optical design
... Optical Prescription . ... Radius=625. 000 Source at infinity s c s n a2 a4 a6 k 1 -8.889e-005 0.00 -1.00028 0.000e + 000 0.000e + 000 3.81e-022 -1.285e+ 000 2 -1.390e-004 -3644.44 1.00028 0.000e + 000 0.000e + 000 1.79e-019 -1.197e+001 3 0.000e + 000 3619.89 1.46080 2.321e-005 -1.173e-010 -7.87e-017 0.000e + 000 4 0.000e + 000 12.00 1.00028 0.000e + 000 0.000e + 000 0.00e+ 000 0.000e + ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19961022_SpecOpticalDesign/19961022.html -- 11.3 Кб -- 18.05.1999
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142. http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer3.pdf
... Data It is now clear that fuzzballs are actually galaxies. ... Using the automatic telescope, we measured the redshifts and brightnesses of a large number of fuzzballs in all regions of the sky. ... Correlation between brightness and redshift Redshifts and Brightnesses 0.005 0.004 0.003 0.002 0.001 0 -0.001 0 -0.002 -0.003 -0.004 -0.005 Redshift of Fuzzball 500 1000 1500 2000 Brightness of Fuzzball The brightnesses and redshifts of all the fuzzballs measured are shown in this graph. ...
[ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer3.pdf -- 63.3 Кб -- 27.06.2002
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143. VLT First Light
... Image Quality of the VLT . Total Optical Control . First light for the ESO VLT unit telescope 1 occurred during the workshop. ... The image shown (Figure 1 ) here was obtained with the VLT on May 16, 1998, in red light (R band), i.e. while the mirror was still uncoated. ... In this diagram (FIgure 2), the measured image quality of the VLT UT1 astronomical images is plotted versus the ``seeing", as measured by the Seeing Monitor, a small telescope also located on top of the Paranal Mountain. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node5.html -- 11.0 Кб -- 12.06.2006
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144. http://www.astro.louisville.edu/shared_skies/archive/select/moon/20101017/log.txt
October 17, 2010 ================ CDK125 and Nikon D3s Exposure of 0.001 seconds at ISO 1600 nikon_1287376892_moon_0p001s_1600iso.jpg was taken at Wed, 30 Jan 1974 00:28:09 GMT You can convert any unix time stamp to GMT (UTC) at this website: http://www.onlineconversion.com/unix_time.htm
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/shared_skies/archive/select/moon/20101017/log.txt -- 1.3 Кб -- 16.11.2011
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145. Integral challenges physics beyond Einstein | Astronomy.com
... Tonight's Sky . ... space flight . ... space physics . ... Integral challenges physics beyond Einstein . The gamma-ray observatory has placed stringent new limits on the size of quantum т??grainsт?? in space, ruling out some quantum loop gravity theories. ... The European Space Agencyт??s (ESA) Integral gamma-ray observatory has provided results that will dramatically affect the search for physics beyond Einstein. ... Only registered members of Astronomy.com are allowed to comment on this article. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2011/07/integral-challenges-physics-beyond-einstein -- 70.2 Кб -- 10.04.2016
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146. Apache Content Negotiation
Apache's support for content negotiation has been updated to meet the HTTP/1.1 specification. It can choose the best representation of a resource based on the browser-supplied preferences for media type, languages, character set and encoding. ... Content-Language: . ... The reason for setting this language quality factor for variant with no language to a very low value is to allow for a default variant which can be supplied if none of the other variants match the browser's language preferences. ...
[ Сохраненная копия ]  Ссылки http://neptun.sai.msu.su/manual/content-negotiation.html -- 27.5 Кб -- 05.11.2004
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147. Robust Estimation and Image Combining
... A task GCOMBINE in the STSDAS package, for combining images, is briefly reviewed. With a stack of input images, one can identify bad pixels by comparing the deviation of a pixel from the mean with a user-specified threshold times the clipping sigma. It is crucial that estimation of the mean and sigma be robust against unidentified outliers, in order to reject cosmic ray events effectively. ... By uniform weighting, we mean that the weight is a constant for all pixels in an input image. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/zhangc.html -- 15.8 Кб -- 03.11.2000
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148. Astronomy articles, forums, listings, and other resources about Astronomy.
The Astronomy Net . Articles | ... Forums . ... Planets | ... The list below is a live snapshot of where the planets and moon are located right now. ... The links in the left hand column take you to a mirror of the excellent NinePlanets web site where you can read about each planet and much much more. The latest news includes the fact that Pluto is no longer classified as a planet. ... Pluto is now classified as a 'dwarf planet' which includes Ceres and soon to be many others. ... 100 . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/planets/ -- 21.1 Кб -- 09.04.2016
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149. ASP: The Nearest Stars: A Guided Tour
... That star is called Sirius, and it is the brightest star in Earth's nighttime sky. ... But the other reason Sirius is so brilliant in our nighttime sky is that it is so close; Sirius is the nearest neighbor star to the Sun that can be seen with the unaided eye from the Northern Hemisphere. ... and even the nearest other star (alpha Centauri, visible from the Southern Hemisphere) would be 6,000 miles away. ... Sun . ... For example, alpha Centauri is the brightest star in the constellation Centaurus....
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/05/05.html -- 25.4 Кб -- 02.10.2012
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150. Accuracy of World positional CCD observations of the numbered minor planets
... For reliable estimation of the accuracy of asteroid CCD observations we usually consider from ten or more various NUMBERED MINOR PLANETS (NMPs) observed during several nigths per month (more then 50 positions). ... They can be considered as an indicator of accuracy of the CCD positional observations with given MPC code. ... For any NUMBERED minor planet the (O-C) values must be zero if the errors of observations and the errors of its theory are absent. ...
[ Сохраненная копия ]  Ссылки http://www.accuracy.puldb.ru/METHOD.HTM -- 21.2 Кб -- 05.12.2007
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151. INVERTOSCOPE
... The versatile and efficient INVERTOSCOPE? combines the highest optical performance with unsurpassed mechanical quality, and is backed by LOMO's unique lifetime warranty, the most comprehensive in the industry. ... A 15X focusing eyepiece with two interchangeable reticles (a 10mm/100div scale and a 10mm x 10mm/400sq grid) for convenient measuring and counting. ... A set of stage inserts and extension plates to accommodate a variety of sample vessels such as Petri dishes, flasks, microtest plates, etc...
[ Сохраненная копия ]  Ссылки http://www.lomoplc.com/invertoscopeDataPage.htm -- 25.3 Кб -- 09.04.2016
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152. Faster than light neutrinos at CERN? | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... By admin September 26, 2011 Posted in: Cosmology . ... Neutrinos emitted by this explosion did not travel faster than light. ... Albert Einstein (1879-1955) came up with the theory of relativity that established the speed of light as the cosmic speed limit. ... If you divide the distance between those two points by the time it takes for the neutrinos to travel, you get their speed. ... Reply . ... Posted September 26, 2011 at 3:41 PM . ... Astronotes . ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/are-neutrinos-faster-than-light.html -- 63.0 Кб -- 09.04.2016
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153. http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf
Using Site testing data for Adaptive Optics simulations Kislovodsk, October 2010 1Glen Herriot, 1David Andersen, 1Jean-Pierre VИran, 2Brent Ellerbroek, 2Luc Gilles, 2Lianqi Wang 1National Research Council Canada ­ Herzberg Institute of Astrophysics 2TMT Project Office, Pasadena TMT.AOS.PRE.10.074.REL01 1 Outline TMT / NFIRAOS Site Testing Parameters and their value for Adaptive Optics Simulations ... TMT.AOS.PRE.10.074.REL01 9 What is the interest of Adaptive Optics in r 0 Seeing ? ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf -- 1942.1 Кб -- 18.10.2010
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154. http://curl.sai.msu.ru/mass/download/doc/dimm_spec.pdf
DIMM . ... MASS/DIMM 2007 ­ 2009 MASS DIMM. ... D = 0.09 , B = 0.2 r0 = 0.1 . ... 5 , d, : + 2 dz Cn (z ) в 0.009687 - 2 = 0 dfx dfy (fx , fy )f -11/3 cos2 ( z f 2 ). (1 0 ) 1.0 2.0 0.9 1.9 2 / (0) 2 0.7 2 0.8 l / 2 t 1.8 1.7 0.6 0 5 10 15 20 25 1.6 0 5 10 15 20 25 H, km H, km . ... Wlgt (0) , 7 1.0 6в10 4в10 2в10 -13 0.8 -13 -13 P( l/ t) 0.6 -1/3 2 JGL,m 0 -2в10 -13 2 0.4 -4в10 0.2 -13 -6в10 -13 0.0 1.0 1.2 1.4 1.6 2 -8в10 1.8 2 t -13 2.0 2.2 2.4 -14 -13.5 -13 16 -12.5 l / log J 2 . ... dimm . ...
[ Текст ]  Ссылки http://curl.sai.msu.ru/mass/download/doc/dimm_spec.pdf -- 336.0 Кб -- 04.04.2010
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155. http://www.atmob.org/newsletters/200203.pdf
STAR FIELDS Newsletter of the Amateur Telescope Makers of Boston Including the Bond Astronomical Club Established in 1934 In the Interest of Telescope Making & Using Vol. ... We all hope to see your telescope at Stellafane this year, Bruce. ... George A. Wood, Jr., past-President and Secretary of ATMoB, and his wife Nancy Wood George A. Wood, Jr., club member from 1960-1985, Club Secretary 1963-1965, and Club President 1965-1967, passed away on February 18th. ... George was a former secretary as well. ...
[ Текст ]  Ссылки http://www.atmob.org/newsletters/200203.pdf -- 43.1 Кб -- 10.06.2006
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156. http://sn.sai.msu.ru/~sil/preprints/aspb121.pdf
... Properties of Stellar Populations in Isolated Lenticular Galaxies I. Yu. ... The resulting average ages of the stellar population in bulges and discs fill an entire range of possible values from 1.5 to 15 Gyr which indicates the absence in the isolated lenticular galaxies, unlike in the members of groups and clusters, of a certain epoch when the structural components are formed: they could have been formed at a redshift of z > 2 as well as only several billion years ago. ... 69 NGC 2350 No. ...
[ Текст ]  Ссылки http://sn.sai.msu.ru/~sil/preprints/aspb121.pdf -- 1591.8 Кб -- 11.07.2015
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157. http://www.aaa.org/EyepieceFiles/aaa/2010_09_September_Eyepiece.pdf
Journal of the Amateur Astrono mers Association of New York September 2010 Volume 58 Number 9, ISSN 0146-7662 EYEPIECE around other stars and transported to our solar system. ... Astronomers found several stars with surface temperatures mor e than 71,500 degr ees, mor e than seven times hotter than the Sun. ... Astronomers have found a disk of dust around a huge, massive star in its early stages of growth, indicating that stars big and small for m by the same mechanism. ...
[ Текст ]  Ссылки http://www.aaa.org/EyepieceFiles/aaa/2010_09_September_Eyepiece.pdf -- 712.2 Кб -- 22.02.2015
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