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Researchers Poised to Decode Cosmic Dawn’s 21-Centimeter Signal

A Nature Astronomy model forecasts that calibrating REACH with ongoing SKA construction will reveal the masses of the universe’s first stars.

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Credit: REACH
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Overview

  • A Nature Astronomy paper introduces a model linking the 21 cm hydrogen signal to the masses of the first stars by consistently incorporating ultraviolet and X-ray emissions from early X-ray binaries.
  • Researchers found X-ray binaries in Population III star systems are both brighter and more numerous than previously estimated, intensifying their impact on the 21 cm signal.
  • The 21 cm wavelength emission, arising from a hydrogen spin-flip transition roughly 100 million years after the Big Bang, serves as a key marker of cosmic dawn.
  • The REACH telescope is undergoing calibration in South Africa’s Karoo region while the SKA array advances construction in Australia and South Africa, with operations expected to begin in 2027.
  • Study co-authors Anastasia Fialkov and Eloy de Lera Acedo say the upcoming data could illuminate how early stellar masses and compositions differ from those of modern stars.