and Temperature - E-mode-polarisation (TE) and E-mode-polarisation - E-mode-polarisation (EE) power spectra, low l-range of Cls plikHM_TTTEEE_lowTEB_BAO - as above, but use also use BAO data (Baryon ...

For decades, the cosmological field was working under the assumption that, after the universe began in a hot dense soup of energy that expanded in the Big Bang, it continued to expand, forming the ...

Roughly 400,000 years after the Big Bang, the universe cooled just enough to allow photons to escape from the primordial cosmological soup. Over the next 14 billion years, these ancient photons ...