Run a set of commands, one at a time. ... If any command fails, the script aborts. You may save your commands to a file and retrieve them again later. The results of the commands do not show up in the Run_Commands window. ... A tui wait command: tui wait sec . ... Example: # sample commands that are safe to run tcc show status tui wait 0.3 tcc show time . ... The currently executing command is highlighted (and remains highlighted if the script aborts or is cancelled.) ...

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• lsst.tcc: tcc.msg.formatObjFields Namespace Reference
• TUI:Telescope:User Catalogs
• Astrophysical Research Consortium - Apache Point Observatory

... AstroAsciiData is a Python module to handle ASCII tables. ... The idea to develop this Python module emerged from the fact that ASCII tables continue to be one of the most popular and widely used data exchange formats in astronomy and probably science in general. ... To load this ASCII table, go into Python, load the AstroAsciiData module and read in the table with: . ... demo = asciidata.open('webexa.txt') . ... Users who only want to work with ASCII tables neeed no further python modules. ...

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• HSTPOLPOINTS (V1.00) --- May99 --- HSTPOLPOINTS (V1.00)

RTT150 . ... This search system is designed for generating the necessary information on series of pointings (observations of each source consist of sets of exposures with different filters and sometimes with different exposure times) for observed sources. Search results appear at the separate page as a table with the following data: . DATE - real (not evening!) observations date (in YYYY-MM-DD format); . ... Bin - minimal CCD binning mode (may vary during the observations); . ...

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... 2011 . ... 2007 . ... Results of solar observations by the CORONAS-F payload Advances in Space Research, V. 47, P. 1538-1543, 2011 . Download in format .pdf, 845 867 B . ... Download in format .pdf, 925 828 B . ... S.V.Shestov , A.M.Urnov , S.V.Kuzin , I.A.Zhitnik , S.A.Bogachev , . Electron Density Diagnostics for Various Plasma Structures of the Solar Corona Based on Fe XI - Fe XIII Lines in the Range 176-207 A Measured in the SPIRIT/CORONAS-F Experiment Astronomy Letters, V. 35, No. 1, pp. ...

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• Publications - 2011

The XV_VTDF is a viewer for TDF format files (extension to TIFF 6.0 format for storage of high-resolution satellite data). More information about TDF format and relevant topics, as well as satellite data in this format you may receive from Space Monitoring Information Support lab (Space Research Institute, Moscow, Russia) . ... XV_VTDF <filename> - load TDF file at startup (default size) . ... The XV_VTDF operates with fixed-size satellite images in TDF format. ... Back to SMIS Home Page . ...

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• TDF Viewer (Satellite Data Format)
• SMIS IKI RAN (Satellite data)
• REGIONAL DATA ARCHIVE (SMIS IKI RAN Project)

This example shows a difference between CSS's table model for HTML and for other document formats. The first, HTML, example is defined by HTML to be illegal, as it would lead to overlapping cells if HTML's rules for layout are followed. ... The diagram depicts how the two examples, the HTML one and the almost identical non-HTML one, might be rendered. ... The rendering of the non-HTML example is on the right, it follows the CSS rules and thus has no overlapping cells. ...

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• Dynamic HTML in Communicator
• Format
• A Simple Example With a Single Chirp Component

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The ionogram catalogue is divided into the data file and the key file. ... The station codes database consists of the data file and two key files. ... This database consists of the data file and the key file. ... The antenna DB consists of two interrelated databases. ... The data file contains the following information: antenna type, antenna name, antenna parameters names, measurement units, and ranges of parameters. ...

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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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• Format Documentation of *.wdc Files
• Format Documentation of kpyymm.tab Files
• List of currently available KP AZ.

... Impact of Covariance Information on the Orientation Parameters Between Radio Source Position Catalogs, IVS 2012 General Meeting Proceedings, p.339­341 http://ivscc.gsfc.nasa.gov/publications/gm2012/sokolova.pdf Impact of Covariance Information on the Orientation Parameters Between Radio Source ... IVS Analysis Centers provide these catalogs in a standard IERS format, where together with radio source positions and other relevant information, RA/DE correlations are reported. ...

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• Data in zip-format
• Pulkovo NEO Page: Estimation of Accuracy of the Observations

Next: Mission Operations Data Transfer . ... VLBI Tape Management . VLBI Tapes . ... When: As soon as the correlator is satisfied with the correlator output. back to top . ... What: Each correlator will maintain a data base including the status of all VLBI tapes under its control. ... The correlators will distribute tapes to mission elements based on the Observation Summary File produced by the RSOG ( Observation Summary File ) to ensure each element has enough tapes to support SVLBI observations. ...

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• Navigation Pre-Observation Products
• Ground Radio Telescope (GRT) Products

grd2xyz - Converting a grdfile to an ASCII or binary table grd2xyz grdfile [ -H [ nrec ] ] [ -R west / east / south / north [ r ] [ -S ] [ -Z [ flags ] ] [ -bo [ s ] ] grd2xyz reads a binary 2-D grdfile and writes out xyz-triplets in ASCII [or binary] format to standard output. Modify the precision of the ASCII output format by editing the D_FORMAT parameter in your .gmtdefaults file, or choose binary output using single or double precision storage. ... Ignored if binary output is selected. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/grdreformat.html
• http://xray.sai.msu.ru/~ivan/gmt/man/xyz2grd.html
• Dynamics of Bianchi IX ...

... GCN 8471 | ... TITLE: GCN CIRCULAR NUMBER: 8516 SUBJECT: GRB 081102: MASTER refind and final results DATE: 08/11/11 15:50:10 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, P.Balanutsa Sternberg Astronomical Institute, Moscow State University A. Tlatov, A.Parkhomenko Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinski, I.Zalognikh Ural State GCN Circ 8470, Lipunov et al., ...

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Three different forms are possible for representing Results of calculation of spherical coordinates: . the form designated as EMP is similar to that used in the Ephemerides of Minor Planets, having formal precision of 0.01 minute of time in right ascension and 0.1 minute of arc in declination. Longitude, latitude, azimuth and altitude are also displayed with comparable formal precision. the form designated as Positions has enhanced formal precision. ...

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• Conference WPLTN-2012 | Conference page
• Information for Authors of Articles
• AKO-2005

Color separation notes ====================== As an example I took the raw Nikon image file DSC_0100.NEF and processed it with Cinepaint to read all 16 bits in each color. I stored the resultant image as DSC_0100.TIF which is a 16-bit format that ImageJ can read. ... When read in with ImageJ, the color tif file will display as a stack. ... Consequently the usm images are not color shifted from the original, have a less contrast than the hc images, but noticably enhance rays and crater edge detail. ...

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• http://www.astro.louisville.edu/software/archive/colorspec/colorspec-1.0/README
• PGM_Reader (ImageJ API)
• FileSaver (ImageJ API)

... We computed the permanently shadowed areas and temperatures inside the craters for the variation of the position of the lunar pole of rotation with respect to the ecliptic pole with a period of 18.6 years. ... According to our results, the total permanently shadowed area in the polar craters of the Moon is equal to 50428.7 km2, or 0.13% of the total area of the lunar surface [3]. ... The area of permanently shaded part of a crater makes 59 % from all area of a crater [3]. ...

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• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
• http://selena.sai.msu.ru/San/Publications/ms38/ms059.pdf
• http://selena.sai.msu.ru/Greg/Publications/ms38/ms090.pdf

The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...

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• Model realization and some results
• Query Results from Astronomy Database

We have designed the laboratory model of static Fourier spectrometer for onboard usage for spectral study of atmosphere and ionosphere. The gain of model is to simulate onboard FS which will not have any moving elements (all its optical elements will be mounted at fused quartz monolithic construction), to compare experimental results with theoretical estimations and to measure MTF of CCD array. ... This fact connected with low frequency response of CCD array due to small format of it. ...

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fitshdr - FITS-file headers manipulation tool fitshdr [options] [FITSfile_name] . ... fitshdr [options] --edit FITSfile_name . ... If You want to modify headers of FITSFILE using new FITS-header lines from HEADER file (or from stdin), You have to use this option (You can skip this option, if -H or --header option is used). ... Empty header lines are not displayed (in 'dump' mode only). --line-offsets . ... In 'dump' mode: file offset will be displayed for each header line. --no-line-offsets . ...

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• IDL programs
• Data bases of Natural Satellites. Documentation. Structure
• Data bases of Natural Satellites. Documentation. Sources

A star has recently been discovered travelling in a circular orbit around our galaxy (the Milky Way). ItтАЩs orbit is 80 kilo-parsecs out, and it is traveling at a speed of 320 km/s. Deduce the mass of our galaxy from this. Compare your answer to the mass of everything we can see in our galaxy (1.2x10 42 kg). A kilo-parsec is 1000 parsecs, and a parsec is 3.1x10 16 m. Click here to download the webcast (8 minutes, 11 MB, m4v format, can be viewed with Quicktime, iTunes or iPods)

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• Observational Techniques: Assignment 1

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Protected Member Functions | ... Protected Attributes . MultiLevelJsonBase Class Reference abstract . ... More... #include < MultiLevelJsonBase.hpp > . ... voidљ . initFromUrl (const QString &url) . ... boolљ . ... Definition at line 34 of file MultiLevelJsonBase.hpp . ... Load the element information from a JSON file. virtual void MultiLevelJsonBase::loadFromQVariantMap . ... Definition at line 107 of file MultiLevelJsonBase.hpp . ...

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• Stellarium: StelQGLTextureBackend Class Reference
• Stellarium: SphericalRegionP Class Reference
• SphericalTexturedPolygon Class Reference