Stellar angular momentum of intermediate-redshift galaxies in muse surveys

HIGHLIGHTS

• What: The authors investigate the rotational support in galaxies at different cosmic times and environments with the purpose of determining how galaxy stellar angular momentum evolves. The authors aim to study a specific range in the redshift space (z and amp;lt; 1) making use of the long spectral coverage of MUSE, as Ca II H and K lines are redshifted to 7936 and 7868 Å at z=1, respectively. The authors focused on the recovery of the two first-order moments of the line-of-sight velocity distribution (LOSVD), the radial mean velocity (V), and the velocity . . .
  

   

  

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