Inferring the astrophysical population of gravitational wave sources in the presence of noise transients
Inferring the astrophysical population of gravitational wave sources in the presence of noise transients
ABSTRACT The global network of interferometric gravitational wave (GW) observatories (LIGO, Virgo, KAGRA) has detected and characterized nearly 100 mergers of binary compact objects. However, many more real GWs are lurking sub-threshold, which need to be sifted from terrestrial-origin noise triggers (known as glitches). Because glitches are not due to …