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161. http://hea-www.harvard.edu/AstroStat/Stat310_1314/dj_20131112.pdf
... Computation: RJMCMC Similar to Richardson Green 1997 Knowledge of the PSF makes things easier Insensitive to the prior on k e.g. posterior when k = 10 and = 3: Posterior of number of sources (k) 8 9 10 11 12 0.058 0.141 0.222 0.220 0.157 0.019 0.022 0.029 0.027 0.021 Mean SD 7 0.029 0.018 13 0.082 0.014 Used posterior probabilities given by 10 chains 6 / 30 Example Region occupied by the three ... 28 / 30 XMM data spectral distribution 29 / 30 Four models 30 / 30 ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1314/dj_20131112.pdf -- 506.2 Кб -- 12.11.2013
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162. http://scan.sai.msu.ru/~kirx/ATel/BL_Lac/
... We thank the Swift team for their rapid scheduling of this observation. ... 2455705.20851 V 14.15 0.03 2455707.83079 V 14.10 0.03 2455710.84028 V 13.53 0.02 2455713.64631 V 13.66 0.02 2455714.65479 V 14.11 0.03 2455714.71823 V 14.12 0.02 2455714.78596 V 14.20 0.02 2455717.39593 V 14.37 0.03 2455726.62861 V 14.83 0.04 2455727.16343 V 14.57 0.04 2455730.50586 V 14.57 0.03 2455730.57329 V 14.56 0.03 2455730.70360 V 14.66 0.04 2455738.32865 V 14.00 0.02 2455742.86146 V 14.21 ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/~kirx/ATel/BL_Lac/ -- 11.7 Кб -- 12.07.2011
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163. SAI OCL Catalog NGC 136
. Home . Structure of Data . Description . Catalog . Publications . VO . ЮБ 2000 . 00:31:32.6 . ЮД 2000 . +61:30:30 . l . 120.561 . b . -1.272 . diameter . 4.0' . (m - M) 0 . 13.59 0.14 . distance . 5220 350 pc . E(B - V) . 0.7 0.09 . log(t) . 8.4 0.05 . SAO 1-m, BVRI observations (874 measurements) VOTable . 2MASS data VOTable . IPHAS IDR data VOTable . Developed by the Team . Send us your questions or feedback
[ Сохраненная копия ]  Ссылки http://ocl.sai.msu.ru/catalog/ngc_136/ -- 9.4 Кб -- 09.04.2016
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164. G14.3+0.1
... Flux density at 1 GHz (/Jy): 0.6 . Spectral Index: 0.4 . Notes: Has been called G14.30+0.14. ... 2006, ApJ, 639, L25. VLA at 330 MHz (42": S=1.2?0.1 Jy), plus other observations. ... Last updated: 2006 March 29 . ... detailed listings | summary listings . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2006/snrs.G14.3+0.1.html -- 2.6 Кб -- 10.04.2016
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165. http://zebu.uoregon.edu/~uochep/docs/docs01/0009035.pdf
‚ є є ¦± ·· ЅЅ · јЄ·¦ ё јјє ¦ № Ѕ Є·· ј № Ѕ Є·Ѕ ·¦ Љ ѓ ¬ѓ ¦ ­® ¦ ѓ®¦ ­­Ў · јЄ· …ј ® ЅЄ·¦№ Ѕ Є·Ѕ ·  · ‚ ¤Ѕ јЋ¦ Ї Ќ „ ‚ ·¦ ‰  » ё Entries / 5Іm 200 SLD 175 150 125 100 75 50 25 0 0 20 40 60 80 100 120 140 160 180 200 2-D impact parameter (Іm) ‰ Ў ­Ў ± Є¤ ј ј ІЎ ЋЄ г Ѕј¤ …јЄ· Є ј § ®§ ¬µ ¶© ј © ¤ ¶ ј ¤ Є ј § ® ¶Є¶ ·ј…¶ ‚ јЄ¤ јЄ ј Њ© ¤¶ ·ј є І¦ ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/docs/docs01/0009035.pdf -- 345.9 Кб -- 14.09.2001
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166. http://site2010.sai.msu.ru/static/doc/VOrlov_site2010.pdf
Dynamic Shack-Hartmann System RAPID V. G. Orlov, V. V. Voitsekhovich Instituto de AstronomМa, UNAM, MИxico CONACYT project E9507-1020P UNAM PAPIIT IN104910 Telescopes OAN OAN- SPM 2.1m telescope 1.5m telescope 0.84m telescope 2.1m telescope OAN-Tonanzintla 1m telescope Astronomical site SPM Observing statistics 1982-2002 (Tapia+ 2007 ) Photometric nights : 64.1% Spectroscopic ... Rapid - Dynamic Shack-Hartmann All modern telescopes demand installation of adaptive system. ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/VOrlov_site2010.pdf -- 1652.8 Кб -- 18.10.2010
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167. 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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168. http://www.accuracy.puldb.ru/200707/C094.HTM
... July , 2007 . ... 0.12 0.23 +/- 0.10 +/- 0.06 Internal error of single observation 0.18 0.11 ----------------------Compressed Ephemeris DE200/LE200 -------------- MP Obs Dynamical Time RA (O-C)cosDEC DEC (O-C) h m s " ' " " 78756 094 2007 7 22.891513 20 04 27.767 -0.12 - 9 55 57.80 0.32 78756 094 2007 7 22.899703 20 04 27.348 -0.34 - 9 55 58.00 0.30 78756 094 2007 7 22.907823 20 04 26.959 -0.18 - 9 55 58.20 0.28 78756 094 2007 7 22.914753 20 04 26.618 -0.17 - 9 55 58.30 0.33 Mean of last 4 obs. ...
[ Сохраненная копия ]  Ссылки http://www.accuracy.puldb.ru/200707/C094.HTM -- 7.4 Кб -- 05.12.2007
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169. ARC 3.5m | SPICAM
... ARC 3.5m | SPIcam . ... 2.3 Taking SPIcam Exposures . ... Data Reduction . ... SPIcam is operated within the Telescope User Interface (TUI) software written and maintained by Russell Owen at the University of Washington. ... The instrument is configured using the SPIcam window accessible under the Inst menu from the main TUI window. ... Be sure to turn off any calibration lamps you may have used, then hand over the instrument by simply quitting out of the SPIcam instrument control window in TUI. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/SPICAM/ -- 30.5 Кб -- 24.02.2016
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170. 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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171. 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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172. 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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173. 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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174. 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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175. Winer Weather Status
... 25.43 . ... 0.000 . ... 39321 . ... Omega-RC1500 DP ( C) . ... Message[0]="D,01/23,01:04:30, 68, 18,25.43,247, 8, 38, 0.00, 6.21, 64,!007 " at 2457488.319282 . Message[1]="D,01/23,01:03:23, 67, 18,25.43,270, 10, 38, 0.00, 6.21, 61,!009 " at 2457488.318507 . Message[2]="D,01/23,01:02:15, 68, 18,25.43,270, 13, 38, 0.00, 6.18, 61,!019 " at 2457488.317720 . Message[3]="D,01/23,01:01:07, 67, 19,25.43,225, 7, 38, 0.00, 6.15, 64,!006 " at 2457488.316933 . ... S-Message[0]="" at 2457488.318507 . ...
[ Сохраненная копия ]  Ссылки http://www.winer.org/engWeather.html -- 8.3 Кб -- 09.04.2016
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176. 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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177. Vulcan: ghost planet | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Sun . ... There could be an eighth planet to discover! ... The orbits of the planets could be predicted perfectly- apart from Mercuryт??s. Planetary orbits are not circles, but ellipses and Mercuryт??s orbit was the least circular (or most т??eccentricт??) known. ... Vulcan, according to Le Verrier, orbited the Sun every 19.7 days at an average distance of 21 million km (0.14 au), a little over a third of Mercury?s average distance from the Sun. ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/vulcan-the-solar-systems-ghost-planet.html -- 54.0 Кб -- 09.04.2016
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178. 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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179. http://curl.sai.msu.ru/mass/download/doc/pmt_param_eng.pdf
... 2 Measurement of PMTs counting characteristics and selection of op erating p oint To select the operating point of the PMT, that is the optimal values of the high voltage supply and pulse discrimination threshold, the command run counting=hv value is provided in the program mass. ... Starting with the minimum voltage (say 550 V) run command run counting=550 for the measurement execution. ... It is recommended to take measurements for the set of values of 0.4, 0.6, 0.8, 1.0. ...
[ Текст ]  Ссылки http://curl.sai.msu.ru/mass/download/doc/pmt_param_eng.pdf -- 111.1 Кб -- 12.09.2015
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180. http://www.vista.ac.uk/Files/docs/vdfs/Cal-Plan-draft_v1.4.pdf
Data Flow System Document Title: Document Number: Issue: Date: Document Prepared by: Document Approved by: Document Reviewed by: Document Released by: Peter Bunclark & Simon Hodgkin (CASU) Mike Irwin (CASU Manager) William Sutherland (VISTA Project Scientist) Jim Emerson (VDFS Project leader) VISTA Infra Red Camera Calibration Plan VIS-SPE-IOA-20000-0002 1.4 pre 1 2006-11-13 Signature And date: Signature And date: Signature And date: Signature And date: DATA FLOW Calibration Plan SYSTEM VISTA Document:
[ Текст ]  Ссылки http://www.vista.ac.uk/Files/docs/vdfs/Cal-Plan-draft_v1.4.pdf -- 648.5 Кб -- 20.04.2011
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