Alma and Cosmology

@inproceedings{Casoli2005AlmaAC,
  title={Alma and Cosmology},
  author={Francesca Casoli and Thierry Contini and Jean – Marie Hameury and Laurent Pagani and Françoise Combes},
  year={2005}
}
ALMA is a privileged instrument to tackle high redshift galaxies , due to the negative K-correction in the millimeter domain. Many dusty star-forming galaxies, invisible in the optical or NIR, will be detected easily through the peak of their emission in the FIR redshifted in the submm between z=10 and z=5. Their mass and dynamics will be determined through… CONTINUE READING