Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...

... HST . ... Staff Directory . ... Missions . ... Data . ... Future Missions and . ... HST Overview . ... Cycle 24 Announcement . ... Retrieving HST Data . ... These parameters are used in the pipeline to combine and clean associated datasets with MultiDrizzle . ... These files can be downloaded directly from the jref directory. file_name camera delivery pedigree p3p1650tj_mdz.fits HRC Mar 25 2005 INFLIGHT p3p16510j_mdz.fits SBC Mar 25 2005 INFLIGHT p3p16511j_mdz.fits WFC Mar 25 2005 INFLIGHT Copyright...

Next: Three-dimensional Data Analysis in IRAF and ZODIAC+ . ... A data analysis system has been developed at SRON, which has been designed to allow rigorous control of the quality of its processed data products. ... This means recording all parameters of all steps which lead to the establishment of the final data products (Figure 1 ). ... Figure: A processing pipeline is a sequence of tasks with several input/output files and parameters, which pass data from one task to the next. ...

... Future seminars . P a s t seminars . Seminar council . The emission time of Gamma-Ray Bursts" . A. Sanin (IKI) . ... The three new parameters of cosmic gamma-ray bursts are introduced: the emission time, the peak energy of the emission time spectrum and the cosmological invariant parameter. ... Using this distribution the "collective estimation" of the best fitting redshifts for the group of long bright gamma-ray bursts detected by BATSE experiment was found. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Project History . ISS Russian Segment . ... ISS 45/46 . ... Study of OOA compound manifold action on operational characteristics of separate orbital station systems which affect reliability and efficient operation of object as a whole (solar arrays, windows, attitude control systems). ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

Our completed projects . Russian Foundation for Basic Research . ... P.I. - V.Klochkova . ... P.I. - Panchuk V.E. The team: Panchuk V., Aliev A., Tavolganskaya N., Yushkin M. Russian Foundation for Basic Research (RFBR) + GFEN . ... The team: Chentsov E., Panchuk V., Tavolganskaya N., Yushkin M. Russian Foundation for Basic Research (RFBR) . ... P.I. - Panchuk V.E. The team: Panchuk V., Ermakov M.V., Najdenov I.D., Tavolganskaya N., Yushkin M. Russian Foundation for Basic Research (RFBR) . ...

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... yes . ... none . name of input events file . ... boolean . ... Create output events file (no for overwriting input) . ... events.out' . ... name of output events file. ... WEIGHT' . ... name of output (weight) column . ... factor the mirror's effective area (and gratings absorption for MOS) into vignetting weight . ... factor the filter's transmission into vignetting weight . ...

Fortran 90 properties already in CF77 . ... Only the old form (fix form) of the source code is available. ... LOGICAL Default KIND number = 8 INTEGER Default int7 int15 KIND number = 6 1 2 digits = 46 7 15 radix = 2 2 2 range = 13 2 4 huge = 70368744177663 127 32767 bit_size = 46 8 16 INTEGER int31 int46 int64 KIND number = 4 6 8 digits = 31 46 63 radix = 2 2 2 range = 9 13 18 huge = 2147483647 70368744177663 9223372036854775807 bit_size = 32 46 46 REAL half Default,single double KIND ...

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 . ...

An early version of the database was used by Garcia ( Garcia et al. 1993 ; Garcia 1993 ) for a general study of group membership of all galaxies with a radial velocity less or equal to 5500 and an apparent magnitude brighter than bt=14. ... From the whole sample 485 groups were build. They are identified by the acronym LGG (for Lyons Galaxy Group). For a galaxy, the LGG number lgg gives the group to which the galaxy belongs. The lgg number is available for 2702 galaxies. ...

The current set of keyword-value pairs of a task can be monitored by typing ESC K while the name of the task is present in the User Command Area. This causes (part of) the Common Output Area to be overlaid with a display containing the current user input parameters of the task. ... If there is currently a set of parameters displayed on the screen (as the result of typing ESC K ), these parameters will be edited; otherwise the name of the task is derived from the User Command Area contents. ...

Next: Post-AGB Stars Up: C.S. Jeffery Previous: Research Group Contents . Hot subluminous stars (or subdwarfs) are low-mass stars that are less luminous than massive main-sequence stars of a similar temperature. ... Chris Winter and Simon Jeffery worked towards completing a scheme for the automatic spectral classification and parameterization of hot subdwarfs. ... Simon Jeffery has embarked on a project to construct theoretical models for subluminous B stars. ...

Design Parameters and Efficiency of a Space System for Warning about Small Celestial Bodies Approaching the Earth along Collision Trajectories . ... tracking of an earlier detected hazardous celestial body (HCB) for synchronous-basic position measurements. The space telescopes (ST) would be placed at a long distance (such as 5 10 7 km) from the Earth to provide for detecting small (100 m) celestial bodies when they are moving to the Earth from the sunward direction. ...

THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

... SMIS : Space Monitoring Information Support laboratory . Russia's Weather : State Meteorological Center Weather Forecast . Space Weather service : ACE real time solar wind data and simple geomagnetic activity forecast. ... World Fire Web : Space Research Institute (IKI) node . Sputnik : Joint project of SRC Planeta, Rosgidromet and Space Research Institute (IKI) . ... Today's Space Weather : Presented by the Space Environment Center . ... Back to the Space Research Institute Home Page ...

... Using the Echelle with TUI . Using the Echelle with Remark . ... Configuring TUI to use the Echelle . Setting up the Echelle exposure parameters . ... Focusing the Echelle . ... Changing the echelle guider filters . ... Configuring Remark to use the Echelle . ... Echelle User's Manual . ... The Echelle home page is http://astro.uchicago.edu/echelle . ... Echelle Description . ... Enclosure . ... schematic CAD files . schematic PDF files . ... enclosure wiring schematic . ...

... I determine th as a time period (from some moment in the past till the present moment) during which papers responsible for 1/2 of the total citation index were published. Parameter Nt represents averaging of the citation index over this period: Nt = C.I./2th 1 Intro duction The problem of estimation of an impact of a scientist (or a group of them) is an actual one (see, for example, [1] and references therein). ... One published in 1965 a paper with C.I.=5000, and nothing after that. ...

... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...

... Together, this small group works mostly in the field of Active Galactic Nuclei, exploring their distribution in parameter space (black hole mass, black hole spin, accretion rate) and their evolution in cosmic time. Since the growth and activity of the central black hole, on the one side, and the assembly of the host galaxy, on the other, go very tightly in parallel, the AGN evolution is a convenient window on the more general problem of the formation of cosmic structures. ...