This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

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Sternberg Astronomical Institute, Moscow University, . Moscow, Russia . Supernovae make us brighter .. Search russian astronomical resources . Mirror of International Supernovae Network ( Original site ) . Catalogue of Supernovae Stars . HTTP access to SAI Catalogue of Supernovae Stars . SAI SN Light Curves Online . ... Sternberg Astronomical Institute ( in Russian ) . ... Astronet - Russian Astronomical Network . ... Russian Foundation for Basic Research . ...

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• Отдел Изучения Галактики и переменных звезд
• Index of /groups/cluster/CEP/RADVEL

B?rbel Koribalski ( ATNF ) . ... The Grus-Quartet consists of four large spiral galaxies which are so close to each other that they should be interacting. The high starburst activity of two of the members, namely NGC 7552 and NGC 7582, is also thought to arise from tidal galaxy-galaxy interactions and subsequent formation of a bar in the disk. ... The colour gradient is in units of Jansky/beam km/s.) . The colour gradient is in units of km/s.) . ... Baerbel.Koribalski @ csiro.au ...

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• Pulsar Group Main/Psrfits
• Pulsar Group PmWiki/Markup Master Index
• Pulsar Group PmWiki/Page File Format

... Astrophysics Group . ... VSA . ... CAT . ... The Very Small Array is a custom-built radio telescope (operating between 26-36 GHz), designed expressly to make high resolution observations of the cosmic microwave background (CMB) radiation on angular scales around and below one degree. ... The VSA has been operated in ?compact array? and ?extended array? configurations (see the technical description below) and data collected to achieve high sensitivity in both regimes have been analysed. ... 1.75 GHz)...

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• OptInt PmWiki : PmWiki / Wiki Group
• Astrophysics Group AMI
• Astrophysics Group VLSS

... HST . ... Missions . ... Data . ... Hubble Heritage Project . Future Missions and . ... Missions Office . ... Journal Clubs and Research Groups . ... HST Peer Review Process . Hubble Fellowships . ... HST Overview . Overview . ... Servicing Missions . ... Cycle 24 Announcement . Cycle 23 Results . ... Mid Cycle Submission . ... Phase II Cycle 23 . ... Retrieving HST Data . Hubble Legacy Archive . Data Analysis . ... HST Science Year in Review . ...

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• Spectral Energy Distributions for Massive-star Populations
• ramp_fixsectors.pro (JWST Pipeline routines in IDL)
• The Astronomy Thesaurus and UDC - Present and Future (Group Discussion for

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

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• System Interfaces to the STIS Calibration Pipeline
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
• Automatic Detection of Linear Features in Astronomical Images

Next: Non-standard keywords Up: FITS keywords Previous: FITS keywords . ... The first group is translated into special MIDAS descriptors for the data structure in question. The conversion for image files is given in Table . The START descriptor of a MIDAS image refers to the first pixel and is computed from the values CRVAL and CRPIX for the reference pixel as given in the FITS header. ... Table: Name translation between standard FITS keywords and MIDAS descriptors. ...

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• Nearby Galaxies Catalogue (NBG)
• Some statistical trends and distributions
• Group IAG

... Velocity allipcoid parameters as functions of heigt above the Galactic disk for the complete sample of F -stars (left) and a young ( t 3 Gyr) metal-rich ( [Fe/H] -0.13 ) group (reght). ... next figure | previous figure . ...

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• Vladimir Marsakov Publication List
• Vladimir Marsakov Abstracts

N. A. Vavilov Department of Mathematics and Mechanics, State University of Saint-Petersburg St. Petersburg, Russia nikolai-vavilov@yandex.ru Calculations in exceptional groups Let be a reduced irreducible root system, R be a commutative ring with 1. ... The Steinberg group St(, R). ... 2] R. Hazrat, N. Vavilov, K1 of Cheval ley groups are nilpotent, J. Pure Appl. ... 6] N. Vavilov, An A3 -proof of structure theorems for Cheval ley groups of types E6 and E7 , Int. J. Algebra Comput. 17 (2007), no. ...

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• Young researchers' seminar in statistical physics
• Transformation Groups 2007
• Dubna-2015: M. Triestino

... Kopylov, A.I., Kopylova, F.G. "Structure of galaxy groups and clusters and measurement of their masses", . ... Kopylova, F.G., Kopylov, A.I. "Peculiar motions of galaxy clusters and groups in the Hercules and Leo supercluster regions", . ... Kopylova, F.G., Kopylov, A.I. "Analysis of the properties of clusters of galaxies in the region of the Leo supercluster", . ... Kopylova, F.G., Kopylov, A.I. "Analysis of the properties of clusters of galaxies in the region of the Ursa Major supercluster", . ...

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• articles_alex_01
• Observatory structure
• Metagalaxy sector, archive 2001

... The polarimetry group at the Arcetri Observatory has been working for several years, mainly from the theoretical-interpretative side, on the polarization of the radiation emitted by objects of astrophysical interest. ... E. Landi Degl'Innocenti "The physics of polarization" in "Astrophysical Spectropolarimetry", J. Trujillo Bueno, F. Moreno Insertis, F. Sanchez (eds.), Cambridge University Press, 1. ... E. Landi Degl'Innocenti "The Zeeman effect: applications to solar physics" Astron. ...

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• mod_unixd - Apache HTTP Server
• Arcetri Star-Formation Group Publications
• Arcetri Solar Physics Group: High Resolution Studies

Procedure to be followed by DMD secretary for DFS Group documentation . Initial email comes from author requesting document number. ... An email is then sent by the DMD secretary to the Technical Archive (tecarch@eso.org) with the same information, to request the last 4 digits of the document number (the 'chronological number'). ... Some time will pass and then the author, using the DFS Group tool 'WebCheck', will post a web readable version of the document on the DFS Group website. ...

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• AB structure
• pyQC: script structure
• Quality Control Group

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

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• Stellar Astronomy

This session will provide a forum for a discussion of variety of topics in Astrostatistics following the Special Session "Lectures on Astrostatistics" held on Wednesday morning. It will also anticipate the "Time-Domain and Applicable Methodologies" session scheduled for Thursday morning. ... 111.02 - Andreas Hans Wilhelm Kupper -- Exploding Satellites - The Tidal Debris of the Ultra-Faint Dwarf Galaxy Hercules . ... Moderators: Aneta Siemiginowska (CfA) and Vinay Kashyap (CfA) . ...

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• Comments on: tests of fit for the Poisson distribution By: hlee
• Statistics 310 2007-2008
• X--ray Quiet PMS Candidates

Last time we saw that flat rotation curves for galaxies, when measured in galaxies with extended gas distributions, provides unambiguous data that shows the mass distribution is dominated by an unseen, spherical halo. ... Perhaps only galaxies with extended dark matter halos are capable of retaining large gaseous extents? . ... Clusters of Galaxies: . ... The case of the Cancer cluster: . ... Below is the velocity distribution of galaxies in the Cancer cluster: . ... What's going on in Cancer? ...

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• Low Surface Brightness Galaxy Gallery
• Astrophysics Group in the Physics Department
• University of Oregon Center for High Energy Physics - Group Talks, Papers, and

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

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• Index of /~igor/images/group

... Credit Copyright: Local Group Galaxies Survey Team , NOAO , AURA , NSF Explanation: Nearby galaxy NGC 6822 is irregular in several ways. ... Pictured above , NGC 6822, also known as Barnard's Galaxy , is located only about 1.5 million light years away and so is a member of our Local Group of Galaxies . ... Publications with keywords: galaxies - Local Group of Galaxies - NGC 6822 . Publications with words: galaxies - Local Group of Galaxies - NGC 6822 . ... HCG 87: A Small Group of Galaxies . ...

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• Астронет > Local Group Galaxy NGC 6822
• Galaxy Group HCG 87
• Galaxy Group Hickson 44

... Working Group . ... Science justification, survey strategies, and requirements . ... possible survey strategies and data taking modes . ... Karen O'Neil , Riccardo Giovanelli, Martha Haynes . ... Jon Davies, Erwin de Blok, Martha Haynes, Robert Minchin, Sabina Sabatini and Steve Schneider . ... 4.4 Definition of Phase I data products to public access . ... 8.2 Definition/organization of the post-white paper activities of the group . 8.3 Recommendations for group structure post-white paper . ...

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• GALFA System Description
• Radio-astronomy group.
• pdev_birdies_25jun07

... rmfgen generates the o/p rmf in the format specified by OGIP. This format allows response data for a given energy range to be stored in the form of contiguous groups of elements whose values are above a particular threshold. ... The fitting package expands this format, replacing those elements in between groups with zero. ... The threshold value can be set by the user through the threshold parameter and allowed range is between 0 and 1 (the maximum possible response value). ...

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• Home Page

... Measurement of the MASS detectors parameters with mass program January 24, 2015 [112707] . MASS/DIMM electronics. ... Turbina-core(D): Dimm User Guide. ... N.Shatsky, V.Kornilov, The revision of the MASS/DIMM star catalogue. ... О.Возякова, В.Корнилов, Н.Шатский, Новое программное обеспечение прибора MASS/DIMM. ... V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site. ...

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