1 code implementation • 5 Oct 2020 • Yijun Wang, Kris Pardo, Tzu-Ching Chang, Olivier Doré
While the detection threshold assuming the currently expected performance proves too high for detecting individual GWs in light of the expected supermassive black hole binary population distribution, we show that binaries with chirp mass $M_c>10^{8. 3}~M_\odot$ out to 100 Mpc can be detected if the telescope is able to achieve an astrometric accuracy of 0. 11 mas.
General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics
1 code implementation • 1 Jul 2020 • Kris Pardo, David N. Spergel
Measurements of the large-scale structure of galaxies at low redshift show much weaker features in the spectrum.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology