Measurement of the galaxy-velocity power spectrum of DESI tracers with the kinematic Sunyaev–Zeldovich effect using DESI DR2 and ACT DR6

  • kinetic SZ: Doppler shift of CMB photons scattered by electrons moving with a bulk velocity relative to the CMB rest frame

 

  • thermal SZ:  inverse Compton scattering of CMB photons by hot electrons in galaxy clusters

 

  • Cosmic Infrared Background: thermal dust emission from unresolved star-forming galaxies throughout cosmic history

 

Measurement of the galaxy-velocity power spectrum of DESI tracers with thekinematic Sunyaev–Zeldovich effect using DESI DR2 and ACT DR6.

By Arnaud De Mattia

Measurement of the galaxy-velocity power spectrum of DESI tracers with thekinematic Sunyaev–Zeldovich effect using DESI DR2 and ACT DR6.

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