The Steady State model of the Universe was proposed in 1948 by Bondi and Gold and by Hoyle. ... At the time the Steady State model was proposed, the Big Bang model was in trouble because the value of the Hubble constant was clearly bigger than the inverse of the age of the Universe. ... Thus the Steady State model has flat spatial sections like the critical density Big Bang model. ... The Steady State model has no adjustable parameters to correct for this error, but the Big Bang does. ...

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• The ROSAT All-Sky Survey Faint Source Catalogue
• Source Positions
• The ROSAT All-Sky Survey Bright Source Catalogue

The cumulative system performance is plotted for each receiver. ... When something occurs that may change the gain of the system (moving a horn, shimming the elevation rails) then a new epoch will be started. The old data is moved to the old system performance data page (the old data link points to this). ... Gain,Tsys,Sefd... (.ps) (.pdf) . ... Pointing errors (.ps) (.pdf) . ... Hour of day when sources measured (.ps). (.pdf) . list of sources with dates and filenames Old data . ...

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• pntModelGradients
• Pnt correction after may11 level platform.
• rotaPlatToSky

... Meta Index / Home Page This section documents warnings and errors generated by this task (if any). ... There is more than one source in the EPIC source list with a given ML_ID_SRC or BOX_ID_SRC number. tooManyProposals . ... The instrument recorded in the source list header keyword INSTRUME is not the same as that derived from the value of the instexpid parameter. corrective action: The task uses the value from the source list header. expIdStrClash . ... Too many (over 99) EPIC source lists are read...

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• Elaborations.

Current status of the source finding service: HALTED . ... Also fixing a bug preventing the sorting of output source lists. 13/6/2012 - v1.6, r15987 - Improved Gaussian fitting, performance improvements, use of casacore-1.4.0 and a few bug fixes. ... A major part of the ASKAP software development is to produce an effective source-finding tool to automatically process the images and cubes that come out of the pipeline imager. ... Please report any bugs or problems via the Redmine ticket system . ...

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• Widget: Value
• Widget: View2Datasets
• Tracking accuracy

... This chapter discusses some of the error sources associated with WFPC2 data. Most of the chapter focuses on specific calibration errors, complementing and partially overlapping the discussion given in "Improving the Pipeline Calibration in section 3.5 . ... Note that many of the error sources affecting calibrated WFPC2 data can be reduced by either recalibration with newer reference files or post-pipeline improvements, such as correction flatfields (see section 3.5.2 ). ...

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• README file for GOODS Catalogs r1.0z based on v1.0 data
• FOC Data Handbook
• NICMOS Data Handbook

... This plug-in enables you to add various types of lighting effects to your (RGB) image. ... Directional light . ... Well, you get the idea :) The default settings for this light-type is [-0.5,-0.5,-1.0]. ... Higher values makes your image reflect a lot of light (appear lighter or more intense), while smaller values makes it appear more dull or matte. ... A value of 1.0 makes your image very shiny (bright high-lights) while smaller values makes you image less shiny, making the high-lights dimmer. ...

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• The Sparkle Plug-In: The Sparkle Dialog Box
• Open Source Convention

... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...

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• Writing programs that use comedi and comedilib
• comedi_loglevel
• Format of data description

... JavaScript version 1.3 provides the following new features and enhancements: . ... See the Client-Side JavaScript Guide for details. ... Changes to the Array object. ... The push method returns the new length of the array rather than the last element added to the array. ... Changes to the Date object. ... Added a day parameter to the setMonth method. ... Added the apply method, which allows you to apply a method of another object in the context of a different object (the calling object). ...

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• mod_ext_filter - Apache HTTP Server
• Converting Modules from Apache 1.3 to Apache 2.0 - Apache HTTP Server
• htpasswd - Manage user files for basic authentication - Apache HTTP Server

GrIm II . ... The MC has been modified to change the way GRIM images are stored to disk when FITS format is selected. ... The solution the Grim team has come up with is to internally add a constant of 10000 to every pixel of the 'bias subtracted' grim image which makes it conform to the unsigned 16-bit number standard, in that all pixel values after this addition of 10000 are in the range 0-65535. ... We have now implemented this for storage of GRIM files in FITS format. ... filetype fits . ...

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• lsst.tcc: include/tcc/telConst.h Source File
• lsst.tcc: src/telMod.cc Source File
• lsst.tcc: python/tcc/msg/formatObjFields.py Source File

On 1 February 2002 this Mirror was upgraded from NVSSlist v2.10 to NVSSlist v2.17 . ... This form searches the source catalog produced by the NRAO/VLA Sky Survey (NVSS). ... Object name [optional] : . ... Search radius and verification halfwidth in arcseconds [Optional] : . ... Enter a list of positions to search: . ... The contents of the NVSS source catalog and the techniques used by NVSSlist to derive error estimates and other parameters are described here. ...

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• Introduction to SCons Bojan Nikolic web pages (r. 329)
• exchange.h File Reference
• OptInt PmWiki : Trolley Software | History

Overlapping Astronomical Sources : Utilizing Spectral Information David Jones Advisor: Xiao-Li Meng Collaborators: Vinay Kashyap (CfA) and David van Dyk (Imperial College) CHASC Astrostatistics Group April 15, 2014 1 / 30 Introduction X-ray telescope data : spatial co ordinates of photon detections photon energy Instrument error: diffraction in the telescope means recorded photon positions are spread out according to the point spread function ...

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• Doug Burke's Perl/S-Lang pages: Structure examples
• Doug Burke's Perl/S-Lang pages: Array examples
• Chandra Images for SNRJ 0540.1-6919

... St Petersburg 23, September 2014 1 Motivation · Origin of Martian moons? ... Considered error sources: ­ Phobos a priori ephemerides; ­ Phobos a priori GM value; ­ measurements noise; ­ different strategies; · Methods: ­ real data analysis; ­ simulations. ... St Petersburg 23, September 2014 8 Simulations: sensitivity of the measurements to the a priori GM value Simulations: zero noise+ IMCCE a priori ephemerides +GMPH = 7.16 * 105 m3/sec2. ... St Petersburg 23, September 2014 14 Thank you! ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm13r.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/kurdubov.pdf
• http://www.gao.spb.ru/personal/neo/eng/accuracy/data/errors.txt

... ESO copyright, division, department . ... Any document produced by the DFS Department has to apply the official ESO document template: MSWORD format (ZIP compressed) , Latex format as compressed tar file (courtesy of Ralf and Pascal), or StarOffice format . ... Template for Test Plan and Test Report : as HTML page (for complete testing - to be edited with DreamWeaver, as Twiki page (for basic testing) Any HTML page produced by the DFS Department has to apply the official DFS web page template . ...

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• The Cross-correlations
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• SPECINHOLUCY (V1.00) --- Dec02 stecf.specres --- SPECINHOLUCY (V1.00)

... Clean . ... Flux Sign Expo . ... The map above is movable . The image is shown in significance with a squared root color map ranging from 0 to 25. ... Original shows mosaics with all data available. Flux map Error map Significance Exposure . Flux and error maps are in mCrab units. ... Exposure maps are in ksec. INTEGRAL/IBIS 9-year Galactic Hard X-Ray Survey* , A , Volume 545, id.A27 { NASA ADS | ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ... Exposure . ...

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... R. E. Jackson . ... H.-M. Adorf . ... D. C. Wells . ... AstroWeb is a World Wide Web (WWW) interface to a collection of Internet accessible resources aimed at the astronomical community. ... The goal of AstroWeb is to be the most complete, up to date, and useful listing of Internet accessible astronomical resources available anywhere. ... Jackson, Wells, and Adorf noticed that they and others had created largely overlapping lists of Astronomical resources. ...

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• QPSIM: An IRAF/PROS Tool for Source Simulation
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• ADASS 2003 Conference Proceedings

The Texas survey of radio sources covering -35.5{deg} < {delta} < 71.5{deg} at 365MHz . ... We present the Texas Survey of discrete radio sources between -35.5deg and 71.5deg declination (B1950), which was carried out at 365MHz with the Texas Interferometer during 1974-1983. ... The Texas Survey . ... The sources in the simpler model. ... Right Ascension 1950 . ... field separator . ... Some sources came from Version 6 of the Texas Survey ('TS6' in strp field) or Version 7 ('TS7' in strp field) . ...

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• Description of the RadioAstron project, english version
• MEMORANDUM

. To make lasting changes to the value of an environment variable: . 1. Use your editor to open the .bash_profile file and add the line: VARNAME= value_of_variable ;export VARNAME . 2. Save the file and leave the editor. 3. Enter the command: source $HOME/.bash_profile . This adds the new value to your working environment. Examples .

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• Examples of changing environment variables: BASH shell
• Changing default access permissions
• Examples of changing environment variables: C and TC shell

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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• Identities
• Lagrangian Points
• Pictures/Рисунки

... B.1 New functionality . ... B.3 Semantic changes from CSS1 . ... CSS2 builds on CSS1 and all valid CSS1 style sheets are valid CSS2 style sheets. The changes between the CSS1 specification (see [CSS1] ) and this specification fall into three groups: new functionality, updated descriptions of CSS1 functionality, and changes to CSS1. ... Several internationalization features, including list numbering styles , support for bidirectional text , and support for language-sensitive quotation marks . ...

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• SunSoft
• Conformance: requirements and recommendations
• Tutorial on Fortran 90, Digital UNIX

Stellarium 0.12.3 . ... FileљStructure . FileљList . FileљMembers . core . planetsephems . calc_interpolated_elements.h . ... 6 љ copy of this software and associated documentation files (the "Software"), . ... 26 љ void CalcInterpolatedElements( const double t, double elem[], . ... 36 љ The cache consists of 3 sets of values: . 37 љ e0[0..dim-1] are the cached values at time *t0, . ... 41 љ (*calc_func)(t,elem) calculates the values elem[0..dim-1] at time t, . ...

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• Stellarium: core/modules/Landscape.hpp Source File
• Stellarium: core/renderer/StelGLSLShader.hpp Source File
• Stellarium: core/renderer/StelGLUtilityFunctions.hpp Source File