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  2. Thermal weapon sight - Wikipedia

    en.wikipedia.org/wiki/Thermal_weapon_sight

    A thermographic weapon sight, thermal imagery scope or thermal weapon sight is a sighting device combining a compact thermographic camera and an aiming reticle. [1] They can be mounted on a variety of small arms as well as some heavier weapons. [2] As with regular ultraviolet sensors, thermal weapon sights can operate in total darkness.

  3. AN/PAS-13 - Wikipedia

    en.wikipedia.org/wiki/AN/PAS-13

    The AN/PAS-13B thermal weapon sight (TWS) is an infrared sight developed for the United States military by Raytheon. The sight is designed for use on small arms in the U.S. military's inventory, but it can also be used as a standalone observation device. The AN/PAS-13B uses thermal imaging so that it can be used day or night. Thermal imaging ...

  4. Roland XP-50 - Wikipedia

    en.wikipedia.org/wiki/Roland_XP-50

    The Roland XP-50 is a music workstation that combines the synthesizer engine of Roland's JV-1080 sound module with the sequencing capabilities of their MRC-Pro sequencer and a 61-note keyboard.

  5. Night-vision device - Wikipedia

    en.wikipedia.org/wiki/Night-vision_device

    This essentially covers scopes using Gen0 technology, but not subsequent generations. [101] Minnesota, as of 2014, "A person may not possess night vision or thermal imaging equipment while taking wild animals or while having in possession [an uncased and loaded weapon] that could be used to take wild animals."

  6. Pulsar - Wikipedia

    en.wikipedia.org/wiki/Pulsar

    X-ray pulsar-based navigation and timing (XNAV) or simply pulsar navigation is a navigation technique whereby the periodic X-ray signals emitted from pulsars are used to determine the location of a vehicle, such as a spacecraft in deep space. A vehicle using XNAV would compare received X-ray signals with a database of known pulsar frequencies ...

  7. Five-hundred-meter Aperture Spherical Telescope - Wikipedia

    en.wikipedia.org/wiki/Five-hundred-meter...

    During the construction phase, a commissioning ultra-wide band receiver covering 260 MHz to 1620 MHz was proposed and built, which produced the first pulsar discovery from FAST. [39] At the moment, only the FAST L-band Receiver-array of 19 beams (FLAN [ 7 ] ) is installed and is operational between 1.05 GHz and 1.45 GHz.