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  2. High Energy Transient Explorer 1 - Wikipedia

    en.wikipedia.org/wiki/High_Energy_Transient...

    The concept of a satellite capable of multi-wavelength observations of gamma-ray bursts (GRB) was discussed at the Santa Cruz, California meeting on GRBs in 1981. In 1986, the first realistic implementation of the HETE concept by a Massachusetts Institute of Technology MIT-led International Team was proposed.

  3. Ultra-high-energy cosmic ray - Wikipedia

    en.wikipedia.org/wiki/Ultra-high-energy_cosmic_ray

    In astroparticle physics, an ultra-high-energy cosmic ray (UHECR) is a cosmic ray with an energy greater than 1 EeV (10 18 electronvolts, approximately 0.16 joules), [1] far beyond both the rest mass and energies typical of other cosmic ray particles. The origin of these highest energy cosmic ray is not known.

  4. Troop Zero - Wikipedia

    en.wikipedia.org/wiki/Troop_Zero

    Troop Zero had its world premiere as the closing film of Sundance Film Festival on February 1, 2019, and was released in the United States by Amazon Studios on January 17, 2020. The film was met with mixed reviews.

  5. Microsoft and Amazon are using performance reviews to decide ...

    www.aol.com/finance/microsoft-amazon-using...

    Microsoft and Amazon are using performance reviews to decide who gets laid off—experts warn these surefire mistakes will get you cut. Emma Burleigh. Updated January 30, 2025 at 10:41 AM.

  6. High-energy astronomy - Wikipedia

    en.wikipedia.org/wiki/High-energy_astronomy

    High-energy astronomy is the study of astronomical objects that release electromagnetic radiation of highly energetic wavelengths. It includes X-ray astronomy, gamma-ray astronomy, extreme UV astronomy, neutrino astronomy, and studies of cosmic rays. The physical study of these phenomena is referred to as high-energy astrophysics. [1]

  7. Ultra-high-energy gamma ray - Wikipedia

    en.wikipedia.org/wiki/Ultra-high-energy_gamma_ray

    Ultra-high-energy gamma rays are gamma rays with photon energies higher than 100 TeV (0.1 PeV). They have a frequency higher than 2.42 × 10 28 Hz and a wavelength shorter than 1.24 × 10 −20 m. The existence of these rays was confirmed in 2019. [ 1 ]

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