This module implements an expression for the frequency-dependent antenna response functions of ground-based gravitational wave detectors.
- develop a likelihood functional given a PSD
- need to do this for line-of-sight coordinates (perform the conversion, then delegate to existing functions)
- this will likely help the sampler converge much better
- better acceptance fraction?
- plug the likelihood into emcee or an equivalent to sample over localization parameters
- need to check for diagonal pp plots
- look at autocorrelation of chains!
- if this doesn't work, compute the Fisher matrix for localization parameters and use that
- set up injection sets and recover both with and without the frequency dependence in the antenna patterns
- quantify the change in localization areas
- quantify the biases associated with the omission
- do this for single detectors as well as a few simple networks
- aLIGO LHO + aLIGO LLO + aVirgo
- aLIGO LHO + CE (at LLO)
- ET + CE?
- consider how directionality and frequency dependence of anteanna patterns could affect how templated searches work
- phase involved in antenna patterns (which are different for h+ and hx) could mean we cannot simply search for a single template?
- this could be compounded by a directional dependence, meaning one has to perform an explicit all sky search?
Expressions are taken from LIGO-T060237 and Anderson, et all PhysRevD 63(04) 2003