... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

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• Astronomical Catalogues
• Positions and Proper Motions
• Positions and Proper Motions - South

DSS Mirror Archive at SAI MSU Search Position in the form "ra,dec" where ra and dec are given in decimal degrees in the ICRS coordinate system. ... ALL GRAPHIC METADATA image/fits image/jpeg . Field name Survey Observation midpoint as Modifed Julian Date RA of image center Dec of image center Number of axes Image size Image scale for each axes Bandpass CD matrix Reference pixel Reference pixel Projection Coordinate system reference frame Image format Image URL ...

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• saivo:todo [SAI Virtual Observatory - Wiki]

... Астрософт (Модератор: tlgleonid ) > . Reference stars в программе MaxIm DL . ... Благодарностей: 0 . ... 21 Июнь 2009, 10:23:08 ? В программе MaxIm DL (Version 4.58) столкнулась с тем, что при фотометрировании не могу отметить больше чем 8 звезд сравнения (ref). ... Ответ #1 : 21 Июнь 2009, 13:10:42 ? ... А блеск исследуемых звезд вычисляется из среднего по всем звездам сравнения. ... Цитата: Protozvezda от 28 Июнь 2009, 02:44:42 Не хотели ли бы Вы подключиться к моей программе наблюдений? ...

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... 9) Oknyanskij V.L. 1994, "Optical-radio time delays in Q0957+561", Odessa Astronomical Publ., ... 11) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", in Proceedings of Int. Conf. ... 1994. 12) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", Astrophys. and Space Science, 222, p.157. ... 14) Oknyanskij V.L., van Groningen E., 1997, "Optical spectral variability of NGC4151 in 1990", Astronomical and Astrophys. ...

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... We have reference image without OT on 2015-05-20.80932 UT with unfiltered magnitude limit 20.6m. This OT is in 8.3W and 13.1S from the PGC663454 galaxy (S0). We have 8 pairs of images of this area. 2015-12-02 01:48:48 no OT 19.2 2015-12-02 01:52:21 no OT 19.0 2015-12-02 02:00:58 OT 19.0 2015-12-02 02:08:02 no OT 19.3 2015-12-02 02:13:28 no OT 19.0 2015-12-02 02:17:25 no OT 19.0 2015-12-02 02:22:53 no OT 18.5 2015-12-02 02:28:26 no OT 18.2 Spectral observations are required. ...

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• http://observ.pereplet.ru/MASTEROTJ035815.59+214117.9.html
• MASTER OT 054547.15+091200.3 discovery

... The areas between the contours were measured automatically. The results of the measurement are represented on fig.1 The graphic shows the distribution of the height levels against their areas. ... USGS, USA Fig.1 The dependence of the distribution of the heights levels versus the area occupied Fig.2 The distribution of the areas of heights levels in the northern and southern hemispheres Fig.3 The distributions of the areas heights levels in eastern and western hemispheres of Mars ...

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• http://selena.sai.msu.ru/Rod/Publications/ms40/78_Sitnikov_etal.pdf
• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
• http://selena.sai.msu.ru/Ber/Publications/ms40/88_Yamashita%20et_al.pdf

... Upper stage Block DM design is based on Block D, which was originally developed under lunar program N1-L3 and the first time it successfully operated in flight was as a part of L1 complex (with Proton launch vehicle) on March 10, 1967. Upper stage Block DM features high reliability proven by more than 30 years of its operational history, and capacity for multiple burns of the main engine, which allows it to perform the required orbital maneuvers. ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• S.P.Korolev RSC Energia - LAND LAUNCH SYSTEM
• RSC "Energia" - Land Launch
• S.P. Korolev RSC Energia - News

We present a catalogue of galaxies for which spatially resolved data on their internal kinematics have been published; there is no apriori restriction regarding their morphological type. The catalogue lists the references to the articles where the data are published, as well as a coded description of these data: observed emission (E) or absorption (A) data, optical (O) or radio (R) data, velocity (V) or velocity dispersion (D), radial profile (1) or 2D field (2). ...

70. Closing of conference

71. What is Redshift? (2dF QSO Redshift Survey - 2QZ)

72. Источники информации

73. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF50A52A4-0B23-4E0C-9FF7-6DA5BD8FA1F2%7D

74. Amateur Telescope Makers of Boston

75. NS EOS: contents

76. http://kcor.sai.msu.ru/2010/calc_kcor.pro

77. POWER SPECTRUM OF THE IRREGULARITIES AND IT'S FIXING

78. VISTA - Visible and Infrared Survey Telescope for Astronomy

79. СМ5 : Горячие клавиши графического редактора ACCEL Schematic

80. VaST homepage