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NDI, when running on x86 or x86-64 architectures, requires CPUs that include the SSSE3 instruction set. Most Intel CPU designs starting in 2006 have this instruction set, AMD added support starting in 2011. While not a requirement, NDI will take advantage of Advanced Vector Extensions (AVX) and AVX2 instruction sets for additional performance.
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OBS Studio is a free and open-source app for screencasting and live streaming. Written in C / C++ and built with Qt , OBS Studio provides real-time capture, scene composition, recording, encoding, and broadcasting via Real-Time Messaging Protocol (RTMP), HLS , SRT, RIST or WebRTC .
PDF viewer support from Chromium's PDFium PDF viewer is still supported though. The single-process run mode is not supported, but still present; currently is being used for debugging purposes only. [8] On March 16, 2019, the CEF version numbering changed with the release of CEF 73.1.3+g46cf800+chromium-73.0.3683.75.
Therefore, a runtime library is always specific to the platform and compiler. The runtime library may implement a portion of the runtime environment's behavior, but if one reads the code of the calls available, they are typically only thin wrappers that simply package information, and send it to the runtime environment or operating system.
WinRT is not a runtime in a traditional sense but rather a language-independent application binary interface based on COM to allow object-oriented APIs to be consumed from multiple languages, with services usually provided by a full-blown runtime, such as type activation. [1] That is, WinRT is an "API delivery system".
The National Democratic Institute (NDI) [a] is a non-profit American non-governmental organization whose stated mission is to "support and strengthen democratic institutions worldwide through citizen participation, openness and accountability". [1]
Gaia is a space observatory of the European Space Agency (ESA), launched in 2013 and operated until March 2025 (planned). The spacecraft is designed for astrometry: measuring the positions, distances and motions of stars with unprecedented precision, [5] [6] and the positions of exoplanets by measuring attributes about the stars they orbit such as their apparent magnitude and color. [7]