The PAU Survey: Galaxy stellar population properties estimates with narrowband data
A newfound interest has been seen in narrowband galaxy surveys as a promising method for achieving the necessary accuracy on the photometric redshift estimate of individual galaxies for next-generation stage IV cosmological surveys. One key advantage is the ability to provide higher spectral resolution information on galaxies, which ought to allow
Csizi, B. et al.
Fecha de publicación:
9
2024