Project Apollo - NASSP (also known as NASSP or NCPP) is an add-on for the Orbiter space flight simulator. Project Apollo simulates the Apollo missions to Earth orbit and the Moon and the planned post-Apollo missions that never flew.
Parallel Iterative Deconvolution is a multithreaded ImageJ plugin for iterative image deblurring.
A virtual planetarium for observers of the real sky.
Aciqra is a virtual planetarium and sky mapping program which tracks celestial bodies including planets, deep sky objects and stars to an accuracy of a fraction of a degree for thousands of years into both the future and the past. It includes the 2.5 million stars of the Tycho-2 catalog supplemented by data of 120,000 stars from the Hipparcos catalog, 13,000 deep space objects from the NGC and IC catalogs and a large number of asteroids and comets from the Minor Planet Center. The program is platform-independent and can be made to work on most modern computers that support OpenGL.
Plan and preview your astronomical shots
A handy tool designed to help beginner Astronomers. The software Astronomy CCD Calculator uses NASA/SkyView survey resource which provides CCD images of the night sky.It helps you plan an observation by letting you play with different instruments resulting various "Fields Of View" so you can see what your camera will capture and choose the best target for the session.
A collection of Java ports of open source terrain and solar system generation packages. Code has been extensively refactored, extended and documented. GPL License with exception for required libraries.
Routines for wavefront propagation in IDL, Matlab, and Python
PROPER is a library of routines for the propagation of wavefronts through an optical system using Fourier-based methods. It was developed at the Jet Propulsion Laboratory for modeling stellar coronagraphs, but it can be applied to other optical systems were diffraction propagation is of concern. It is currently available for IDL (Interactive Data Language), Matlab and Python (2.7 & 3.x). It includes routines for generating complex apertures and obscurations and aberrations (Zernike & PSD-defined). It includes a model of a deformable mirror for wavefront control. The routines perform near and far field propagation with automatic selection of propagators. The latest version for IDL and Python is v3.0 released on 7 Aug 2017. For Matlab it is v3.0.1 released on 22 Aug 2017 (bug fix in prop_readmap).
Parallel Spectral Deconvolution is a multithreaded ImageJ plugin for spectral image deblurring.
Astrophoto image & video processor. Full cycle with new technology
Astronomy program for selecting, viewing, aligning and stacking images. Creates 16-bit AVI gray/color video files from images series, concatenates videos together into one video file. The program helps to rebuild sequences of images and restore continuous order of files after they were edited, deleted, renamed or moved. PGMania converts images from one format to another. Supports batch converting operations, also for image sequences. Image formats can be any of well known image formats 8/16/32 bpp b/w/c. The program aligns and fits the pairs of images or image series, with each other or over master, calibrates them in pairs. Program detects stars and get stars statistics. Calculates fwhm, snr and star magnitudes. Image editor with alive histogram, contrast stretching, filters, evaluates and post process. XML and txt logging of all actions and results. *) PGMania uses original algorithm for image calibration. No need for dark & bias files for calibration and fit images.
This is MyCalendar object which extends GregorianCalendar object, user can get lunar information by reading related attributes.
The Aciqra Library Of Astronomical Calculations (Aloac) is a library of theories and formulas relating to astronomy to track planets, the sun and moon as well as conversions between coordinate systems. Formerly known as Aciv.
Focuser based on ASCOM platform
It provides an USB connection for the communication with the PC, it uses a stepper motor that provides higher precision, you can set the motor in full step or in microstepp mode (1, 1/2, 1/4, 1/8). The focuser include a temperature sensor. This driver has a ToolBox with which you can control manually the focuser (for example you can set the limits).
A personal coder keys applied to developement nuk friendly for
Source code and diagrams for a dual focuser motor controller for a telescope. Includes source for an ASCOM driver that interfaces with the controller.
Program na spracovanie pozorovaní slnečných škvŕn
Program vznikol ako ročníková práca z informatiky na Gymnáziu Jána Adama Raymana v Prešove. Vznikol na základe programu PC – Sun (autor: V. Feik), ktorý slúži na digitalizáciu pozorovaní Slnka na Hvezdárni Františka Pešty v Sezimovom Ústí (ČR). Program Slnečné škvrny slúži na digitalizáciu pozorovaní slnečných škvŕn a fakulových polí. Pozorovania sú následne štatisticky spracované do tabuliek a grafov popisujúcich aktivitu Slnka. Program taktiež umožňuje výpočet fyzikálnych súradníc Slnka, Carringtonovej otočky a juliánskeho dátumu. Program je určený pre astronómov – amatérov aj profesionálnych astronómov. Program rieši komplexne problém pozorovania slnečných škvŕn. Taktiež realizuje kontrolu vstupných dát od užívateľa. Pre správne fungovanie programu je potrebné dať užívateľovi právo zapisovať do priečinku "C:\Program Files\Slnecne skvrny".
Universal Worker Service is a pattern for asynchronous web-services that is used in the VIrtual Observatory field.