Search Results for "open solver"

ASTAP, Astrometric STAcking Program, astrometric solver and FITS image viewer. This program can view, measure, "astrometric (plate) solve" and stack deep sky images. Main features: - Stacking of astronomical images including dark frame and flat field correction - Native fast astrometric (plate) solver. - Alignment using an internal star match routine, internal Plate Solver, manual or ephemeris. - FITS viewer with swipe functionality, deep sky and star annotation,...

cmdline (used by Image16) and ui interfaces to ANSVR astrophotography plate solving images (FITS, TIFF, PNG, JPG, PXM, RAW and XCF) are submitted to ANSVR astrometry engine producing a text file with the plate solving result and a .png plot file TIFF, PXM, RAW and XCF files are converted to FITS by the cmdline utility all files are loaded and converted to FITS by the ui utility

HSPI offers to the astronomer the possibility to capture pictures from the CCD camera in a fast and intuitive way, keeping under control all the instrumentation in posses. HSPI can control the CCD camera, the mount, the focuser, the filter wheel and the dome from a single interface, and not only this: these features can be added on as many observatories and instrumentations you want. HSPI is ASCOM and INDI compatible, so if you want to use particular setups like Linux computers connected...

Nova is a simple astronomical image solver. It can currently open FITS files and identify some objects against star catalog objects.

DualSPHysics is based on the Smoothed Particle Hydrodynamics method and can be downloaded from the official website (www.dual.sphysics.org). The code is developed to study free-surface flow phenomena where Eulerian methods can be difficult to apply, such as waves or impact of dam-breaks on off-shore structures. DualSPHysics is a set of C++, CUDA and Java codes based on the SPHysics FORTRAN project (www.sphysics.org) that are designed to deal with real-life engineering problems and are...

Spectroscopic Double Star Solver