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  2. Cosmic microwave background - Wikipedia

    en.wikipedia.org/wiki/Cosmic_microwave_background

    The cosmic microwave background ( CMB or CMBR) is microwave radiation that fills all space in the observable universe. It is sometimes called relic radiation. With a standard optical telescope, the background space between stars and galaxies is almost completely dark. However, a sufficiently sensitive radio telescope detects a faint background ...

  3. Planck (spacecraft) - Wikipedia

    en.wikipedia.org/wiki/Planck_(spacecraft)

    Planck was a space observatory operated by the European Space Agency (ESA) from 2009 to 2013. It was an ambitious project that aimed to map the anisotropies of the cosmic microwave background (CMB) at microwave and infrared frequencies, with high sensitivity and angular resolution. The mission was highly successful and substantially improved ...

  4. Cosmic microwave background spectral distortions - Wikipedia

    en.wikipedia.org/wiki/Cosmic_microwave...

    CMB spectral distortions are tiny departures of the average cosmic microwave background (CMB) frequency spectrum from the predictions given by a perfect black body. They can be produced by a number of standard and non-standard processes occurring at the early stages of cosmic history , and therefore allow us to probe the standard picture of ...

  5. Sunyaev–Zeldovich effect - Wikipedia

    en.wikipedia.org/wiki/Sunyaev–Zeldovich_effect

    The Sunyaev–Zeldovich effect (named after Rashid Sunyaev and Yakov B. Zeldovich and often abbreviated as the SZ effect) is the spectral distortion of the cosmic microwave background (CMB) through inverse Compton scattering by high-energy electrons in galaxy clusters, in which the low-energy CMB photons receive an average energy boost during collision with the high-energy cluster electrons.

  6. Wilkinson Microwave Anisotropy Probe - Wikipedia

    en.wikipedia.org/wiki/Wilkinson_Microwave...

    The Wilkinson Microwave Anisotropy Probe ( WMAP ), originally known as the Microwave Anisotropy Probe ( MAP and Explorer 80 ), was a NASA spacecraft operating from 2001 to 2010 which measured temperature differences across the sky in the cosmic microwave background (CMB) – the radiant heat remaining from the Big Bang. [ 5][ 6] Headed by ...

  7. Observational cosmology - Wikipedia

    en.wikipedia.org/wiki/Observational_cosmology

    The first published recognition of the CMB radiation as a detectable phenomenon appeared in a brief paper by Soviet astrophysicists A. G. Doroshkevich and Igor Novikov, in the spring of 1964. [25] In 1964, David Todd Wilkinson and Peter Roll, Dicke's colleagues at Princeton University , began constructing a Dicke radiometer to measure the ...

  8. BOOMERanG experiment - Wikipedia

    en.wikipedia.org/wiki/BOOMERanG_experiment

    BOOMERanG experiment ( Balloon Observations Of Millimetric Extragalactic Radiation And Geophysics) was an experiment that flew a telescope on a (high-altitude) balloon and measured the cosmic microwave background radiation of a part of the sky during three sub-orbital flights. It was the first experiment to make large, high-fidelity images of ...

  9. China Medical Board - Wikipedia

    en.wikipedia.org/wiki/China_Medical_Board

    China Medical Board was founded in 1914 as the second major project of the Rockefeller Foundation. With additional endowments from the Rockefeller Foundation, China Medical Board became an independent private foundation in 1928. CMB established Peking Union Medical College, which brought modern Western medical education to China and "quickly ...