Speaker
Santiago Jaraba
(Instituto de Física Teórica (UAM-CSIC))
Description
Astrometric surveys can be used to constrain the stochastic gravitational wave background (SGWB) at very low frequencies. The European Space Agency's (ESA) Gaia mission, launched in 2013 and with a recent data release (DR3) in 2022, shows great potential for this purpose. In this talk, I will present a recent work in which we used Gaia DR3 to set constraints on the SGWB amplitude. I will also comment on previous works which computed similar constraints and discuss the potential of future Gaia data releases to impose tighter bounds.
Primary author
Santiago Jaraba
(Instituto de Física Teórica (UAM-CSIC))
