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gCAD3D for Linux 1.40
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gCAD3D is a 3D-CAD/CAM-software.
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  • License: Freeware Free
  • OS: Windows 7/Vista/XP
  • Requirements: No special requirements
  • Publisher: Anne Cox

    • License: GPL Free
    • OS: Windows XP/2000/98
    • Requirements: .NET Framework 4.0
    • Publisher: CBSommers

    • License: Freeware Free
    • OS: Windows 7/Vista/XP
    • Requirements: No special requirements
    • Publisher: Unknown Publisher

    • License: Freeware Free
    • OS: Windows XP/2000/98
    • Requirements: Java Runtime Environment
    • Publisher: Felix Seifert

    • License: Others Free
    • OS: Windows XP/2000/98
    • Requirements: Java Runtime Environment 1.5 or higher
    • Publisher: Matthew Rowles

    • License: Freeware Free
    • OS: Windows 7/Vista/XP
    • Requirements: No special requirements
    • Publisher: Unknown Publisher

    • License: Freeware Free
    • OS: Windows 7/Vista/2003/XP
    • Requirements: No special requirements
    • Publisher: AutoFEM Software LLP

    • License: Freeware Free
    • OS: Linux
    • Requirements: No special requirements
    • Publisher: Franz Reiter

    EJS Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s Star Gages Model is a Photo & Image software developed by Todd Timberlake. After our trial and test, the software is proved to be official, secure and free. Here is the official description for EJS Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s Star Gages Model:

    EditByBSEditor: The EJS Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s Star Gages Model illustrates William Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s methods of \\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\"star gages\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\" by which he attempted to map out the shape of our galaxy in 1785. Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s star gages relied on two important assumptions: that Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s Telescope could see to the ends of the galaxy, and that within the galactic system stars are distributed uniformly. If the first assumption holds then the stars seen in the telescope all lie within a conical region of space with the apex at the telescope and the base at the edge of the galaxy. If the second assumption holds then the number of stars seen in the telescope is proportional to the volume of this cone. Since the volume of the cone is proportional to the cube of its height, the distance to the galactic edge in any direction is proportional to the cube root of the number of stars seen in that direction.

    This simulation allows the user to use Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s method of star gages to map out the shape of an artificial \\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\"star system\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\" for which Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s assumptions are valid. One window shows the view through a telescope, with a slider to change the telescopes direction . Another window shows a 3D view of the star system, showing either all of the stars in the system or only those stars visible through the telescope. A third window shows a plot of the star gages. Plotting star gages for many different directions maps out a cross-section of the star system. An optional slider allows the user to decrease the distance to at which stars are no longer visible, and a menu allows the user to select a star system in which the stars are not distributed uniformly. These options let the user explore how violations of Herschel\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\'s two fundamental assumptions invalidate his star gage method.
    Faraday Loop Model is a Photo & Image software developed by Anne Cox. After our trial and test, the software is proved to be official, secure and free. Here is the official description for Faraday Loop Model:

    Observation Log is a Photo & Image software developed by CBSommers. After our trial and test, the software is proved to be official, secure and free. Here is the official description for Observation Log:

    A .NET 4.0 Windows program to log astronomy observations. The program uses an SQL Server Compact Edition database, and comes with a database containing the full Messier Catalog.
    MANTiS is a Photo & Image software developed by Unknown Publisher. After our trial and test, the software is proved to be official, secure and free. Here is the official description for MANTiS:

    - builds a Relational database integrating, in a phylogenetic framework, all Ensembl genes, corresponding Panther molecular functions and biological Processes, as well as GNF, e-genetics, and HMDEG expression data;
    - makes extensively use of the Ensembl ortholog/Paralog Prediction pipeline for identifying gene duplication events;
    - and implements a dynamical programming approach for the mapping of gene gains, duplications, and losses on the phylogenetic tree.

    Through a user-friendly interface, MANTiS allows the user to identify
    - gains and losses on specific branches of the tree,
    - genome content of ancestral species,
    - statistically over- or under-represented molecular functions, biological processes and anatomical systems , and
    - tissue specificity of gained, duplicated, and lost genes.

    Finally, the entire set of information available in MANTiS can be exploited further using an advanced system of queries by which gene identity, mapping, and function parameters can be combined using logical operators.
    miRpp is a Photo & Image software developed by Felix Seifert. After our trial and test, the software is proved to be official, secure and free. Here is the official description for miRpp:

    convas2 is a Photo & Image software developed by Matthew Rowles. After our trial and test, the software is proved to be official, secure and free. Here is the official description for convas2:

    BSEditor: convas2 allows for the merging of multiple diffraction patterns collected at the Powder Diffraction beamline of the Australian Synchrotron. This program allows for the interpolation of data to a constant 2theta step size and to normalise to intensities to beam current and/or count rate.
    NeurotaskNeurotask Alpha is a Photo & Image software developed by Unknown Publisher. After our trial and test, the software is proved to be official, secure and free. Here is the official description for NeurotaskNeurotask Alpha:

    BSEditor: Neurotask is a handy, easy to use, Java based application specially designed to offer users a neural network simulator.
    AutoFEM Analysis Lite is a Photo & Image software developed by AutoFEM Software LLP. After our trial and test, the software is proved to be official, secure and free. Here is the official description for AutoFEM Analysis Lite:

    BSEditor: AutoFEM Analysis Lite is a system of finite-element analysis. The main feature of the system is its deep integration with AutoCAD 2007-2010. AutoFEM Analysis Lite offers an easy-to-use first step analysis tool for every AutoCAD user. It is available for every user of AutoCAD at no cost.

    AutoFEM Analysis Lite uses the same finite element technology that a commercial version of AutoFEM Analysis. AutoFEM Analysis Lite is used to perform all kind of finite element analysis: -Static analysis -Frequency analysis -Buckling analysis -Thermal analysis.
    gCAD3D for Linux is a Photo & Image software developed by Franz Reiter. After our trial and test, the software is proved to be official, secure and free. Here is the official description for gCAD3D for Linux:


    gCAD3D has its own:
    import and export-programs,
    integrated 3D-OpenGL Viewer,
    program interpreter for geometry and NC commands in 3D,
    integrated NC processor.
    programming interface for userprograms

    gCAD3D is freeware:
    - may be used for any purposes free of costs
    - may be copied and distributed without restrictions
    - no restrictions for AddOn-Software

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