Search Results for "linux astronomy image stacking"

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

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."

IMG2GSLIB is a small command line tool that converts images to grids into GEO-EAS format readable by geoscientific software such as GSLIB, SGeMS, Isatis, Gocad, Petrel, etc. It now can output 3D volumes from image stacking. The ASCII result is sent to stdout, so you can redirect it using the > operator if you want to save it to a file. Run java -jar IMG2GSLIB.jar without arguments to get help on usage. Requirements: -Java 1.7

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.

Astronomical Image Processing

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.

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.