SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

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• SAI SN RESEARCH GROUP

Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Moscow 119992, Russia . ... 84/32, Moscow 117997, Russia . ... Our CCD observations compared to times of minima derived from the archival photographic plates and from the NSVS and ASAS-3 data clearly show that the orbital period of the system is variable. ... The phased light curve for the light elements . ... CCD, Moscow . ... and for the current linear light elements (in excellent agreement with the NSVS, ASAS, and our CCD observations): . ...

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. [ Go back to Comet WWW site ] . Andrew A. Martis . martis @ sai.msu.ru .

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• The Body Element and Related Elements
• Hot links of Comet Center of SAI

... Format of the orbital elements | Estimation of the extrapolation errors | Version 1" of the orbital elements collection, determined by KIAM during flight and used for operations planning . Version 2" of the of the orbital elements collection, modified by IKI during flight and recommended for the orbital calculations during scientific data processing . ... Three kinds of the INTERBALL Auroral probe (IB_AUR) orbital elements' collections are presented here. ... IKI RAN | SSC IKI RAN | ...

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• INTERBALL Auroral probe (INTERBALL 2) post-flight orbital elements collection
• About modification of the INTERBALL orbital elements
• Институт космических исследований РАН (ИКИ РАН)

... Plastic forming and welding of optical elements for laser technologies and optical telecommunications. A set of technological processes of manufacturing of optical elements with sophisticated profiles for laser technologies and optical telecommunications has been developed in the Institute of Solid State Physics . ... тАв€а to form optical surfaces with non-spherical and rather sophisticated profiles, improving essentially effectiveness of laser technologies and optical telecommunications; . ...

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• Institutes of Chernogolovka
• Astronomy: Olympiad of Scientific Centres: Institutes of Chernogolovka
• Crystalline scintillators for physics, medicine, safety, engineering

... Chapter 5: Visits, Exposures and Exposure Groups > 5.12 Spectral Element [Sp_Element] . ... Spectral Elements include filters ( F ), gratings and grisms ( G ), echelles ( E ), prisms ( PR ), polarizers ( POL ), linear ramps ( FR ), quadrant filters ( FQ ) and mirrors ( MIRROR ). ... A medium-band ( M ) WFC3 IR filter ( F ) with midpoint of coverage near 0.98 microns . ... A narrow-band ( N ) WFC3 UVIS quadrant filter ( FQ ) with midpoint of coverage near 2320 е . ... Text Proposal File (Sp_Element) ...

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• COS Spectral Elements and Central Wavelengths
• COS Spectral Elements and CentralWavelengths
• Mode = POSConfig = FGS

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• RadioAstron Mission Element Overview
• RSOG Pre-Observation Products
• Contingency Plans

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

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• (Untitled)
• Keywords_79
• EPHEMERIDIES OF MINOR PLANETS (EMP)

... The binary nature was remarked by Deutsch, approximate orbital elements were at first derived in Potsdam. Recently, 53 Cam was directly resolved by speckle-interferometric measurements of McAlister et al. and Balega. Combining with the spectroscopic elements the determination of the absolute values of the system parameters should be possible. In the present paper a revision of the spectroscopic orbital elements and a comparison of spectroscopic and speckle data have been carried out. ...

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• http://jet.sao.ru/jet/~goray/kv2005fl.htm
• harak_e
• NES Stellar Spectroscopy Laboratory

A. Singh Institute of Mathematical Sciences, C.I.T. Chennai, India anupamk18@gmail.com Real elements in algebraic groups Let G be an algebraic group defined over a field k . ... Let G be a connected semisimple algebraic group of adjoint type defined over a perfect field k . ... It follows that if G is connected semisimple of adjoint type, with -1 in its Weyl group, then every semisimple element in G(k ) is strongly real in G(k ). This also shows that any regular element in such a group is real. ...

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• IUM10 conference: V.Buchstaber
• Elements of the representation theory (Spring 2000)
• Elements of the theory of modular forms (Spring 2000)

... Variation of systematic errors for USNO A2 (in mas per year) 23 .914 0.082 0.250 0.418 0.586 0.753 0.921 1.089 1.257 1.425 1.593 4 4. 3. 3. 3. 3. 3. 3. 3. 3. 3. 15 ± 7± 1± 3± 3± 10 ± 10 ± 11 ± 6± 10 ± 12 ± and their errors USNO UCAC USNO UCAC A2.0 2 3 B1.0 4 (1998) (2006) (2003) (2012) 37 27 11 4 732 529 778 501 050 078 775 387 (34 610 829) (17 209 447) (9 744 401) () Distribution of observations ( ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/girdiuk.pdf
• Pulkovo NEO Page: Ephemeris Support

... В четверг, 14 апреля 2016 г., состоится семинар кафедры астрофизики. Повестка дня . ... Начало в 11 час.15 мин. Ауд. ... В четверг, 31 марта 2016 г., состоится семинар кафедры астрофизики . ... В четверг, 24 марта 2016 г. , состоится семинар кафедры. ... В четверг, 17 марта 2016 г. , состоится заседание кафедры. ... ОСП НИИ ПММ Национального исследовательского Томского государственного университета) . ... Copyright 2016 Астрономия в Санкт-Петербургском университете . ...

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• Statist.htm: Add elements
• AddElem.htm: Add elements
• ArrElem.htm: Elements of Array

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) . ...

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This Directory contains mean daily values of geomagnetic field components at the Tbilisi Observatory (1880 - 1991). ... Information on the DUSHETI (TBILISI, GEORGIA) magnetic observatory Geograpic Geomagnetic Latitude 42 05' 36 31' longitude 44 42' 122 12' The long history of magnetic observations of Dusheti observatory is recor- ded on the PC-Disquette. On the floppy disk in the directory DUSHETI are written the elements of the Earth's magnetic field from 1880 to 1991. ...

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Main News Phones Research area Brief history Institute Structure Experimental Base Observational data English/Russian . research on the site(Google) . ... 7(4112)390400 . Fax: . 7(4112)390450 . ... Phone: +7(4112) 390-441 . Fax: +7(4112) 390-450 . Field of investigations: . ... drift of the ionospheric plasma at auroral and subauroral latitudes . ... Research assistant Elena Bondar . Research assistant Sargylana Kobyakova . Post-graduate Kiril Borisov . ...

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Subject of Celestial Mechanics. ... Differential Absolute Coordinates Equations of the Problem. ... General Integral of Non-Perturbed Motion. ... General Equation of Non-Perturbed Orbit. ... Other Integration Methods of Non-Perturbed Motion Differential Equations; Bine Equation for Case of Non-Perturbed Motion. ... Ellipsical Motion, Kepler Equation. ... Motion Differential Equations in Absolute Coordinates. ... Equation of System of Bodies Motion in Barycentric Coordinates, in Relative Coordinates. ...

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• Elements of osculating planetary orbits. Explanation for Computer Ephemeris.
• Eclipse elements for Computer Ephemeris for 2015 (DE200/LE200).
• Eclipse elements for Computer Ephemeris for 2014 (DE200/LE200).

Proposal Identification No.: P2678 Date Received: 2011-Oct-03 23:44:10 Technical Page Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: Regular Pulsars Galactic 33 Hours 1.00 hr Refined Relativistic Orbital Elements and Mass Measurements for Two Neutron Stars ABSTRACT: Arecibo observations of the pulsar­white-dwarf binaries J0621+ 1002 and J0751 + 1807 have yielded measured relativistic precession (J0621+ ...

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• http://www.naic.edu/vscience/schedule/tpfiles/NicetagP2678tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/OlmitagA1966tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/GiovanellitagA2010tp.pdf

DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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• International workshop “Europa lander: science goals and experiments”
• Elements of Algebra
• Space Research Institute (IKI) Seminar

From XEphem running the Soft03Cmt database of 20121002, for the date and time of the observation: RA: 08:16:04.25 Dec: 27:48:13 2012-09-30 UT 09:45 UTC Measured: RA: 08:16:04.4 Dec: 27:48:12.9 Header listing for HDU #1: SIMPLE = T / This is a FITS file BITPIX = -32 / NAXIS = 2 / NAXIS1 = 4341 / NUMBER OF ELEMENTS ALONG THIS AXIS NAXIS2 = 4355 / NUMBER OF ELEMENTS ALONG THIS AXIS EXTEND = T / This file may contain ...

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• http://www.astro.louisville.edu/shared_skies/archive/select/supernovae/sn1572/20121130/hst/log.txt

... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

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• Observation Interval Determination for the Chandra X-ray Observatory
• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
• ISDC Data Access Layer