... First of all, you can obtain a map of the final coordinates of your objects and guide stars by using the command: PLOT/OPTOPUS [table] [label] [EW_flag] , . where [table] is the table output by REFRACTION/OPTOPUS . ... In order to avoid object misidentifications at a later stage, and for a cross identification between object identifiers and hole numbers, it is recommended to bring a printout of the table output created by the command REFRACTION/OPTOPUS to the telescope. ...

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• Encapsulated PostScript Files
• Handling of Plotfiles
• Discriminant Analysis

... This document and the attached postscript figure document an analysis that I did to determine the optimum midpoint and required ranges for both the rotator and azimuth for the 2.5 M telescope. ... I simulate a series of drift scans on the sky for tracks that cover the northern survey area. These tracks cover the range in survey latitude of -60 to +60 degrees, spaced by 10 degrees. ... Along each track the azimuth, elevation, and position angle of the CCD is computed at 1 minute intervals. ...

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• Astigmatism II
• Primary mirror support
• Observers Instructions for filling out the ARCSAT nightlog

. This mosaic of WFPC-2 images shows the evolution of the G impact site on Jupiter (the 21 comet fragments of Shoemaker-Levy 9 were each assigned a corresponding letter to identify the impact site; G represents the 7th fragment to strike the planet. It was also the largest impact.) // R. Evans/J. Trauger/H. Hammel/and the HST Comet Science Team

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA6149A58-A920-49AF-96EE-0FAD66E4F93D%7D

Next: Flagging data Up: Interferometry Previous: The plot selection widget Contents . A data selection widget is opened for a stream when the selected axis item requires further user input. ... In the data selection widget, input beam, output beam, and triple have to be specified, depending on the selected axis item. ... N EXT and P REVIOUS return a selection of the next or previous index values, where is the number of selected index values in the selection line. ...

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• EVM and ETRM specification for ESO instruments
• Procedure to handle Waiver Requests
• Help for Night Report / Progress Pages

nearneighbor - A Nearest neighbor gridding algorithm nearneighbor [ xyzfile ( s ) ] -G out _ grdfile -I x _ inc [ m|c ][/ y _ inc [ m|c ]] -N sectors -R west / east / south / north [ r ] -S search _ radius [ m|c|k|K ] [ -E empty ] [ -F ] [ -H [ nrec ] ] [ -L flag ] [ -V ] [ -W ] [ -: ] [ -bi [ s ][ n ] ] nearneighbor reads arbitrarily located (x,y,z[,w]) triples [quadruplets] from standard ... Default is quadrant search, i.e., sectors = 4]. ... H Input file(s) has Header record(s). ...

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• Calculation of binary NS coalescence rates
• The Model
• Results of calculations

Fast algorithm of reconstruction of absolute conductivity distribution in a cross-section of human body by measurements of electrodes' potentials on the skin surface is described. ... This paper describes fast algorithm for absolute conductivity reconstruction and results of its application. ... The main problem under the absolute image reconstruction is obtaining of reference data, corresponding to the object with uniform conductivity and the same electrode positions. ...

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• Getting Started in Actor Prolog. Analyzing Web Sites.

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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... Inside the Eagle Nebula . ... A closer look at the Eagle Nebula, however, shows the bright region is actually a window into the center of a larger dark shell of dust. ... The telescope mirror, about the size of the Hubble Space Telescope mirror, is protected by a red covering. ... In fact, early last week RS Oph suddenly became visible to the naked eye for the first time since 1985. ... An Unusually Smooth Surface on Saturns Telesto . ... M51: The Whirlpool Galaxy in Dust and Stars . ...

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. Number . Task . Pri . Author . Created By Tool . Created On . Modified On . Completed . Modified By . Assigned To . Link To . Magic . Description

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• To Do List History

... public class EDM . ... Euclidean Distance Map: The value of each pixel is the distance to the nearest background pixel (for background pixels, the EDM is 0) - Ultimate Eroded Points (UEPs) are maxima of the EDM. ... static int . ... Unit in old make16bitEDM: this pixel value corresponds to a distance of one pixel. static int . ... int . ... For compatibility with previous versions of ImageJ only. public FloatProcessor makeFloatEDM ( ImageProcessor ip, int backgroundValue, boolean edgesAreBackground)...

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Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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... SHORT TERM PREDICTION OF POWER SOLAR FLARES FROM SSRT DATA . The algorithm for short term prediction of powerful solar flares, based on SSRT data, includes microwave emission characteristics in total and polarized flux, the structure of active region (AR) magnetic field at the photospheric level, and H a patrol data. ... During this period, 7 AR's crossed the solar disk, in which 20 flares of importance ? ... Data on AR's and magnetic fields were received from the Sayan observatory by teletype. ...

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Dynamic Routing; Configuration of Overloaded Interacting Servers N.D. Vvedenskaya, Moscow, I ITP We consider a symmetrical network with k servers and l Poisson input flows. The proto col uses dynamic routing: each flow is assigned to a subgroup of m servers, up on its arrival a message is directed to the least busy of these servers. ... 6 One server. ... Therefore it is sufficient to consider the equal overload of m , k m m servers caused by the equal overheat of several flows. ...

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• Riemann surfaces, Lie algebras, and mathematical physics (Spring 2008)

Mercury Autumn 2011 Table of Contents . by Douglas Duncan . ... More than one million clickers are in use nationwide, and more than 17,000 of them are at Colorado University. ... find out if students have done assigned reading before class; . ... Of course, none of these outcomes are magically achieved by the clicker itself. ... If you enjoyed this excerpt from a feature article and would like to receive our quarterly Mercury magazine, we invite you to join the ASP and receive 4 issues a year. ...

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International Q-Days and D-Days ---------------------------------------------------------------------------- Classification of Days (deduced from Kp indices) The selection of the quietest days (Q-days) and most disturbed days (D-days) of each month is deduced from the Kp indices on the basis of three criteria for each day: 1. ... In order to indicate such a situation, selected days which do not satisfy certain absolute criteria are marked as follows. ...

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• http://www.wdcb.ru/stp/data/sudden.com/storm_rev.txt
• http://www.wdcb.ru/stp/data/cosmic.ray/Neutron_Monitors(minute_values)/C/1990C/1990KIEL/F1.PAS

... The term Plug-and-Play (PnP) has various meanings. ... In the sense used in this HOWTO, the configuration is only that of configuring PnP bus-resources and letting the device drivers know about it. ... For the case of Linux, it is often just a driver giving a command to set the bus-resources in it's device or determining how the BIOS has set them. ... Linux still is not really a PnP operating system and seems to mainly rely on and device drivers and the PnP BIOS to configure bus-resources for...

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• Plug-and-Play-HOWTO : Introduction
• Comedi Reference
• Pointers

Institute of Applied Astronomy Russian Academy of Sciences Method of Determining the Orbits of the Small Bodies in the Solar System Based on an Exhaustive Search of Orbital Planes Dmitrii Vavilov, Yurii Medvedev Introduction to the problem: Let we have n 3 positional observations of a body: points in time ( = 1, ) , right ascensions , and declinations . ... Determination of the orbit using the Gauss method of determining orbital elements based on two heliocentric positions and points in time. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/bezmenov.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm08d.pdf
• Pulkovo VLBI Analysis Center

MAGNETIC FIELDS IN STARS John Landstreet, Leverhulme Visiting Professor at Armagh Observatory Eight one-hour lectures supplemented by approximately eight hours of supplementary reading and eight hours of short problems and exercises. ... Lecture 1 An overview of the place of magnetic fields in stellar evolution, from star formation to final collapse -- where fields are found, what phenomena they are associated with, what importance they may have. ... Final review of the course. ...

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• Armagh Observatory
• sfit_genetic.html
• sfit help file

AUTOMATED CREATION OF THE LUNAR HYPSOMETRIC MAP: TECHNIQUES OF COMPILING. ... And the second one is the database, obtained from the raster images of the Lunar Subpolar regions (higher than latitude ±60°) where brightness of each pixel depends on its height [1]. ... Due to these reasons it was necessary to develop the special 10-stage methodology of data processing and map compiling. ... The height data were obtained and the lunar hypsometric map was created according to the 10-stage methodology. ...

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• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf
• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf

... title=' Золотое кольцо 01K613066Z - Ювелирное изделие - Ювелирное изделие' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> Кольцо. ... The aim of this book is to add certain new topics to the material of the famous textbook "Statistical physics" by L.D.Landau and E.M.Lifshitz. ... Артикул: PICT53_RED RED Цвет: красный Состав: 100% шелк Параметры изделия: длина 158 см, ширина 9 см Страна дизайна: Италия Страна производства: Италия . ...

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