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2. Cosmic microwave background - Wikipedia

   en.wikipedia.org/wiki/Cosmic_microwave_background

   The telescope is designed for observations in the microwave, millimeter-wave, and submillimeter-wave regions of the electromagnetic spectrum, with the particular design goal of measuring the faint, diffuse emission from the cosmic microwave background (CMB). [49]

3. Cosmic background radiation - Wikipedia

   en.wikipedia.org/wiki/Cosmic_background_radiation

   Cosmic background radiation is electromagnetic radiation that fills all space. The origin of this radiation depends on the region of the spectrum that is observed. One component is the cosmic microwave background .

4. The Great Wave off Kanagawa - Wikipedia

   en.wikipedia.org/wiki/The_Great_Wave_off_Kanagawa

   The Great Wave off Kanagawa is also the subject of the 93rd episode of the BBC radio series A History of the World in 100 Objects produced in collaboration with the British Museum, which was released on 4 September 2010. [86] A replica of The Great Wave off Kanagawa was created for a documentary film about Hokusai released by the British Museum ...

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6. BICEP and Keck Array - Wikipedia

   en.wikipedia.org/wiki/BICEP_and_Keck_Array

   BICEP (Background Imaging of Cosmic Extragalactic Polarization) and the Keck Array are a series of cosmic microwave background (CMB) experiments. They aim to measure the polarization of the CMB; in particular, measuring the B -mode of the CMB.

7. Gravitational wave background - Wikipedia

   en.wikipedia.org/wiki/Gravitational_wave_background

   An astrophysical background is produced by the combined noise of many weak, independent, and unresolved astrophysical sources. [2] For instance, the astrophysical background from stellar mass binary black-hole mergers is expected to be a key source of the stochastic background for the current generation of ground based gravitational-wave detectors.

8. Pulsar timing array - Wikipedia

   en.wikipedia.org/wiki/Pulsar_timing_array

   The main goal of PTAs is measuring the amplitude of background GWs, possibly caused by a history of supermassive black hole mergers. The amplitudes can describe the history of how galaxies were formed. The bound on the amplitude of the background waves is called an upper limit. The amplitude of the GW background is less than the upper limit.

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   www.aol.com/horoscopes

   Get your free daily horoscope, and see how it can inform your day through predictions and advice for health, body, money, work, and love.