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Program: TRACE Purpose: TRACE plots image values at user given positions as function of distance to a plot centre (in 2-d (sub)sets). Category: ANALYSIS, PLOTTING File: trace.c Author: M.G.R. Vogelaar Keywords: INSET= Give set (, subset): Only one subset is allowed. ... XYBOX= Give size of box around one pixel: [3,3] The resulting value at a selected position is an average of the pixels in the defined box around that position. ... POSITION= Give position x, y: Physical values are allowed. ...

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• http://www.atnf.csiro.au/vlbi/dokuwiki/lib/exe/fetch.php/difx/difxwsbonn.pdf
• Channel Selection, Averaging and Doppler Correction - UV Linetypes
• Widefield VLBI Calculator

ALFA - 'dishspot' (pre-cursor for 'leapfrog' mode - we've called it 'dishspot' because it observes a constant range of positions on the . ... length of time. ... Total observing time (mins): 55.4848 . ... Mean Slew time for between each step (sec)=32.9088 . observing efficiency for dishspot:90% . ... Total observing time=55.4848+Ntracks . observing efficiency for onoff:76% . ... total observing time=55.4848+Ntracks*0.6 . observing efficiency for leapfrog:81% . ... click here for pixel 1 . ...

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• Arecibo Galaxy Environment Survey (AGES)

National Research Institute for Physical-Technical and Radio Engineering Measurements IMPROVEMENT OF THE SOFTWARE BERNESE FOR CALCULATION OF THE EARTH ROTATION PARAMETERS ACCORDING TO THE DATA OF SATELLITE LASER RANGING (LAGEOS 1, LAGEOS 2) IN THE MAIN METROLOGICAL CENTRE OF THE STATE TIME AND FREQUENCY SERVICE Tsyba E. N., Kaufman M. B. 141570, Mendeleevo, Moscow region, Russia tel. +7-903-194-7575; tsyba_e_n@mail.ru ABSTRACT Preparatory ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/bezmenov.pdf

... The plot widgets as shown below are created using Calibrate|Visibility|PLOT . The one on the left is the general plot selection widget, the one on the right, the (data) index selection widget, is created when additional input is required as to the indices of the selected data. ... The calibration is applied to all stars selected in the plot selection widget. ... Below is the screen print after clicking on "Calibrate". Solution calculated for OB= 1, Bl= 1, Ch= 2. RMS [%] = 1.876) . ...

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• ESO - European ALMA Regional Centre
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• ESO - ALMA

. Album : asv-album :: Travels to distant places and countries :: 1994/08 Hague, Amsterdam, Rotterdam (Netherlands) . Up . In the centre of the city. Amsterdam consists of streets cut by small and big channels. Here's the big one (or Amstel river itself?) . Next >> . Created with the tool photo album generator from Marginal Hacks by David Ljung on Tue Jun 23 14:45:46 2015 .

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• Image: Canal in the centre of the Leiden
• Image: Amir Temur. At the very centre of the city.
• Image: In the small park near the town centre.

For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...

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• Determination of atmospheric parameters and calculation of chemical composition

As it is in Ephemerides task, O–C can be calculated with different accuracy. ... It presents three modes of accuracy. One can calculate position of a minor planet by the formulae of elliptic motion starting from the fundamental set of elements for given minor planet. ... Also there is possibility to calculate positions taking into account perturbations from different sets of perturbing bodies by numerical integration ( Integration mode). ... Accuracy of integration is equal to 10**(–10) AU. ...

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A time adjustment from the Earth's centre to the observer's location is quantified and shown to improve the residuals between the observed time of pronounced Leonid showers and the time calculated from perturbed dust trails. A correlation with the exact time of closest approach to the nominal dust trail orbit would allow a further improvement in the residuals. ... These results indicate that approaches to dust trails within 0.0005 AU are predictable with an uncertainty of around 5 minutes. ...

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• Armagh Observatory
• Strong Gravity in the Vicinity of Supermassive Black Holes - by Eamon Scullion,
• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...

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• East Siberian Center for the Earth's Ionosphere Research. Back-scattering

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• Perl at the Joint Astronomy Centre
• The INTEGRAL Science Data Centre
• Non-parametric Algorithms in Data Reduction at RATAN-600

Next: *upspecrdf, downspecrdf* - Transform Up: Spectral Analysis Previous: *grid_plot* - Plot Results . The conversion of count rate to flux depends on the intrinsic spectrum of the source, so xflux must be used in conjunction with fit . Fit generates a table of the best fit intrinsic spectrum ( _int.tab extension). xflux uses this table to calculate either the integrated flux between two energy limits or the flux density at a specific energy. ... This produces ``..._obs.tab'' file. ...

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• Latitudes and Attitudes - Links
• Calculation of Extinction from Optical Colors
• *srcinten* - Calculate Source Intensity

Download Izmccd (~2.7 MB). ... If you want to calculate equatorial coordinates of object: . Click the " File " menu, and then click " Open " ; or press  on toolbar. Choose a file with image. ... Also see section " Viewing of image ". ... Before, if it is necessary, you must make an account dark current and flat field (See section " Preliminary processing of images ".) ... Measure the marked stars. ... Click the " Calculations " menu, and then click " Coordinates " or . ...

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... We have measured this "redshift" for the pink black holes, and allowed for it in our calculations. ... We see this effect in the emission from gas around these pink black holes, but it is far too small an effect to account for the pinkness. Thus the swirling motions of gas around or into the black holes cannot produc the colour. ... At first we thought that these things were normal blue black holes hidden behind clouds of interstellar dust, that absorbed the blue light and made them appear pink. ...

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• Centre of the Eagle Nebula
• The Visitor's Centre, 74 inch telescope and Workshops
• The 30 inch is at centre, Woolley and Duffield Buildings at the right

Tail Probe is one of the satellites of the INTERBALL program. ... Collection of the orbital elements | ... Flight situation analysis during operations scheduling . ... Two stages of the orbital situation analysis are presented: . ... The satellites motion calculation during the flight situation analysis is based on the orbital elements, determined by the Ballistic center at KIAM RAN. The modified (by backward integration) orbital elements are usedduring the aposteriory situation analysis. ...

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• INTERBALL AURORAL PROBE SITUATION ANALYSIS
• STDA files
• Le Principe de la Fus?e

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil Zoom †а grand champ sur le centre de la Voie lact†йe . ... Au centre de la Voie lact†йe, les †йpais nuages sombres qui occupent le plan galactique ressortent avec contraste. ... 07/04/2016 - Plong†йe au centre de la Voie lact†йe ...

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• Plong†йe au centre de la Voie lact†йe | Ciel et Espace
• Vista recense 84 millions d'†йtoiles du centre galactique | Ciel et Espace
• Discovery atterrit au centre spatial Kennedy | Ciel et Espace

Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 02 - 08.09.2013, Forecast on 09 - 16.09.2013, Carrington Rotation 2041 (31,87.08.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN REMAINED AT THE AVERAGE LEVEL BUT AFTER 5.09 - THE LOW. WEEKLY, THE AVERAGE OF SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM WAS MADE W=035+15/-21. ... NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE LOW AND AVERAGE LEVEL. ... FLARE ACTIVITY WAS FOR AT A LOW LEVEL, BUT AFTER 6.09 - AT A VERY LOW LEVEL. ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2016/obzor20160222.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2016/obzor20160214.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2016/obzor20160321.en.txt

... This letter contains information about scientific contest - Olympiad, which is held yearly in Chernogolovka: a small pictures- que village not far from Moscow, in which the Noginsk Scientific Center (NSC) of the Russian Academy of sciences is situated. The contest is participated by pupils of the 8-th to the 11-th forms and consists in solving problems in physics, astronomy and mathema- tics. The Olympiad is one of interesting traditions of our scienti- fic centre. ...

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• Olympiad of Scientific Centres
• Astronomy: Olympiad of Scientific Centres: Краткие сведения о Черноголовке
• Astronomy: Olympiad of Scientific Centres: A Brief History of Chernogolovka

... Astrophysics Group . ... Opening of Battcock Centre for Experimental Astrophysics . ... SKA AAVS0 array . ... SKA production design with Cambridge Consultants Ltd . ... Astronomy, Astrophysics and Cosmology have historically been among the very strongest scientific disciplines in Cambridge. ... Paul Alexander, Head of the Cavendish Astrophysics Group and Director of the Battcock Centre for Experimental Astrophysics, is the leader of CambridgeБЂ™s involvement in the SKA: . ...

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• A Calculation of derivatives
• Bojan Nikolic -- Calculating dispersive path delay due to the atmosphere
• DUST: dustiface.h File Reference

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . St. John's Centre of the Royal Astronomical Society of Canada (RASC). Last Update November 03, 2004 . Listed Since November 03, 2004 . ... St. John's, NF A1E 5H9 . Canada . ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Joint Astronomy Centre - JAC, AstroGuide Listing
• Calgary Centre, Royal Astronomical Society of Canada, AstroGuide Listing
• So How Can We Calculate The Mass Of The BH? - an Astronomy Net Blackholes Forum