Speaker
Tatiane de Paula Moraes
(Federal University of Espirito Santo)
Description
A decade after the first gravitational-wave detection, the field has rapidly expanded, opening new opportunities to address key cosmological problems such as the Hubble tension and the study of large-scale structure. As the number of detections continues to increase, the development of robust and efficient computational tools has become essential. In this work, we focus on dark siren line-of-sight (LOS) analyses using CHIMERA and present a comparison between LOS and the Peak Siren method.
Author
Tatiane de Paula Moraes
(Federal University of Espirito Santo)
Co-author
Prof.
Miguel Quartin
(CBPF)