The "Open On-Chip Debugger" provides JTAG/SWD access from GDB (or directly with TCL scripts) to processors with ARM and MIPS based cores.
See website for full list of supported targets.
The Linux GPIB Package is a support package for GPIB (IEEE 488.2) hardware. The package contains a development environment consisting of a GPIB library written in C, kernel driver modules, and bindings for several other languages.
BRL-CAD is a powerful cross-platform constructive solid geometry solid modeling system that includes an interactive geometry editor, ray-tracing for rendering & geometric analyses, network distributed framebuffer support, image & signal-processing tools.
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Please note that OWFS source code, and all Issue/Tickets/merge requests have now been moved to https://github.com/owfs/owfs/.
Developer mailing lists will still be kept at Sourceforge.
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OWFS -- 1-Wire file system. Use the Dallas 1-Wire and iButton chips with standard filesystem commands. Create temperature loggers. Monitor everything. OWHTTPD -- same system, only used as a light weight web server. OWFS is also ported to embedded routers, Mac OSX and Windows.
Basically you can use...
Drivers and applications for the range of Scientific CCD cameras produced by
Apogee Instruments Inc. Both ISA and Parallel interfaces are supported.
A high level library and GUI are provided for Astronomical applications.
RSMeter is a package for interfacing to the RadioShack/Metex 22-168A series of serial-connected multimeters. Currently, it includes an ncurses interface and a script to graph readings. Support for other meters is planned in the future, with an API.
Fostering the development of self-made open design slate style handheld devices and associated software (Chalk Dust) targeting education. We welcome participants from a variety of disciplines including industrial design, electrical engineering, and educa
Software to support TASS, The Amateur Sky Survey. We are taking photometric measurements of all stars in the sky in several filters measurements repeated frequently to allow detection of variable stars