... Maidanak Observatory by AZT-22 1.5m telescope observations Alexander S. Gusev and Boris P. Artamonov Sternberg Astronomical Institute, Moscow, Russia gusev@sai.msu.ru INTRODUCTION Mount Maidanak Observatory at Ulugh Beg Astronomical Institute (UBAI) of Uzbek Academ y of Sciences located in the South Uzbekistan, on the slopes of the Baisun range, at an altitude of 2600 m. Brief history. ... Here we are presenting the study of the realistic seeing of CCD images obtained on the AZT-22 telescope. ......

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• General information
• Methods and instruments to measure/monitor major site properties

... About meteorites . Collections . ... About laboratory . Meteorite encyclopedia . ... Meteorite collection . ... Session of dissertational council Д 002.109.02 has taken place on the 16th of February, 2011, in Vernadsky Institute conference hall. ... 39 new meteorites were stoked the laboratory in 2010: one meteorite from Russia (Romashki), 8 meteorites from Morocco, 7 meteorites from Egypt, 2 meteorites from Qatar and 11 meteorites from Oman. ... 27 July, 2004 . ... Meteorite Encyclopedia: . ...

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• The Laboratory of Meteoritics, Vernadsky Institute, RAS

... GIANT Magellan Telescope . Dr. Dan Fabricant . ... The Giant Magellan Telescope (GMT) is a 25 meter diameter optical-infrared telescope that will be sited in Chile. ... Dr. Fabricant, a leader in the design of new instruments for optical astrophysics, led the development of the optical and instrument design for the Multiple Mirror Telescope (MMT) in Arizona. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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... OH, = 18 cm Nancay Radio Telescope, OH 18-cm line observations , since 1969 F, Jy 6 4 2 0 0 -1 -2 0 -1 -2 0 -2 -4 -6 30 40 50 1612 MHz I HU Pup August 5, 2009 1665 MHz 4 2 0 0.5 0.0 - 0.5 -1.0 -1.5 1.0 0.5 0.0 - 0.5 4 3 2 1 0 -1 1667 MHz I I 1.0 0.5 0.0 0.5 0.0 22-meter telescope, Pushchino Radio Astronomy Observatory H2O F, Jy 1.0 0.5 0.0 0.4 0.2 0.0 -0.2 -0.4 0.4 0.2 0.0 -0.2 -0.4 -0.6 0.6 0.4 0.2 0.0 -0.2 -0.4 -70 -60 -50 -40 -30 -20 -10 0 Mira-type star R Leo. ...

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• Multiwavelength Study of Mira Ceti-Type Variable Stars
• Rudnitskij Georgij M. Home Page
• RadioAstronomy Dept of SAI Home Page

... к почтовому серверу ГАИШ lnfm1.sai.msu.ru . ... WEB-страницы отделов ГАИШ . ... на LNFM1 . HERITAGE - АСТРОНОМИЧЕСКОЕ НАСЛЕДИЕ . астрономическое образование с сохранением традиций) . Лаборатория Новых Фотометрических Методов . ... Леонтьев Сергей Ефимович . ... Копаев Александр А. Отдел Радиоастрономии . Татарников Андрей М. Пахомов Юрий . ... Гусев Александр Сергеевич . ... Кононович Эдвард В. Купряков Юрий А. Горшков Алексей Б. Отдел Звездной астрофизики . ... Моисеев Алексей . ...

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• Maidanak Lab page
• Solar Optical spectroscopy -Links
• Y.Kupryakov, SAI, MSU

... R-band images obtained at 0.8 arcsec seeing conditions have allowed us to separate foreground star from point-like extragalactic source and estimate their brightness separately. ... To study the nature and properties of the source, we observed it under high spatial resolution. ... CONCLUSION RTT150 optical observations with sub-arcsecond seeing and low resolution spectra confirm the hypothesis of superposition of a radio source onto a `normal' F/G galactic star proposed by [1]. ...

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• http://hea.iki.rssi.ru/integral06/papers/D31_Bikmaev01-05Feb07_11:12:42.pdf
• Spectrum-Roentgen-Gamma - The astrophysical Project at IKI RAN
• The 6th INTEGRAL Workshop "The Obscured Universe"

... for Cosmic Ray Observation is situated in Irkutsk (Russia). ... Real-time (preliminary) cosmic ray data in Irkutsk . ... Online Cosmic Ray and Atmospheric Pressure Data Base . ... Real-time data Uncorrected for pressure (Resolution 1 hour - 1 year) -- since 05.2001 . Real-time data Corrected for pressure (Resolution 1 min - 1 year) --- since 09.2001 . Resolution 1 hour - 1 year) --- since 06.2001 . Final data Corrected for pressure (Resolution 1 hour - 1 year) --- From 01.1975 To 07.2004 . ...

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... Parameter Spec Measurement Technique: Wavelength = 355nm (Visual confirmation) Energy = 30 uJ, 160-180 mJ (4025 pulses), 40 uJ (micropulse) Pulse Duration = 10 ms (Measured at 10 ms on an oscilloscope) Micropulse Width = 70ps IR, = 50 ps UV (Autocorrelator to measure IR pulse waveform Temporal Profile - flat envelope) Measured at 10 ms on an oscilloscope. ... Burn Paper measurement) Repetition Rate = 10 Hz/402.5 MHz Oscilloscope Shot to Shot Stability = 3% RMS for pulse envelope. ...

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M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

51. APEX/Equipment

52. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFC3D3F92-EA91-4A57-B5C2-05DF8F838181%7D

53. op020202cloudcam

54. Matyushkin Evgeny, Space Research Institute (SRI)

55. Chief Designers Council for Russian piloted programs Resolution No. 285-01/06...

56. Куртка утепленная Z Generation - Z Generation - Z Generation Журнальный столик

57. http://www.scientific.ru/doska/russia.pdf

58. Astronaut Bio: Harrison Schmitt

59. Image: IMG 0153

60. http://www.atnf.csiro.au/research/masermeeting/web_papers/523_Rudnitskij.pdf