Stochastic gravitational wave background constraints from Gaia DR3 astrometry

Astrometric surveys can be used to constrain the stochastic gravitational wave background (SGWB) at very low frequencies. We use proper motion data provided by Gaia DR3 to fit a generic dipole+quadrupole field. We analyse several quasar-based data sets and discuss their purity and idoneity to set constraints on gravitational waves. For the cleanest data set, we derive an upper bound on the (frequency-integrated) energy density of the SGWB h(70)(2) Omega(GW) less than or similar to 0.087 for 4.2 x10(-18) Hz less than or similar to f less than or similar to 1.1 x10(-8) Hz. We also reanalyse previous VLBI-based data to set the constraint h(70)(2) Omega(GW) less than or similar to 0.024 for 5.8 x10(-18) Hz less than or similar to f less than or similar to 1.4 x10(-9) Hz under the same formalism, standing as the best astrometric constraint on GWs. Based on our results, we discuss the potential of future Gaia data releases to impose tighter constraints.

Automated summary

Astrometric surveys using Gaia DR3 data are used to set constraints on the stochastic gravitational wave background (SGWB) at low frequencies. Analysis of quasar-based data sets allows for the determination of upper bounds on the energy density of the SGWB. The results also indicate the potential for future Gaia data releases to impose tighter constraints.