Search Results for "java image diff"

This software is a remake of Foucault Test Image Analyzer created by Dejan Vucinic and published on SourceForge at 2002 (https://sourceforge.net/projects/foucault/). "If you are an amateur telescope maker, this software can take the tedium out of measuring the shape of your mirror."

ProStack - a platform for image processing and analysis. It implements various image processing methods as separate modules, that can be joined in a complex image processing scenario by use of a graphical user interface. RPMs are available at https://build.opensuse.org/project/repositories/home:mackoel:compbio

Parallel Iterative Deconvolution is a multithreaded ImageJ plugin for iterative image deblurring.

Parallel Spectral Deconvolution is a multithreaded ImageJ plugin for spectral image deblurring.

Welcome to the StarFiles Homepage! This application is designed to sort FITS star image files taken by professional astronomers at observatories. The application sorts the files by their image type: Bias, Dark, Flat, and Object. The Flat and Object images are sorted by filters U, B, V, R, and I. The application allows the user to create and save a profile of a given observatory's FITS header format, for future sorting use. This application also provides a header viewer for FITS image file.

jFITS is a Java Swing based application and applet for quickly viewing and performing simple operations on astronomical FITS formatted CCD imaging data.

Calculates the shape of a telescope mirror from a sequence of Foucault test images. Java-based GUI simplifies entering and organizing measurement data. Logging and comparison functions enable quantification of the effects of various figuring strokes.

A self-sufficient java framework for numerical solution of ODEs (diff eqs) and visualization. Samples are aeronautics/astronautics/physics/rocketry themed. Focus on clean design, modularity, reusability and documentation. Educational project.

Automated supernova finder is a software package to automatically compare FITS images to a nominated reference image with the aim of finding supernovae or other optical transient phenomena.