Observables: Connecting Theory to Observations¶
The Observables module connects theoretical predictions to observational measurements.
This module handles the transformation from theoretical quantities to observable measurements, accounting for survey-specific effects.
Overview¶
This module computes survey-specific quantities including selection functions, window functions, and bias parameters that distinguish real observations from idealized theoretical predictions.
This module addresses:
- Window functions for weak lensing surveys and CMB lensing
- Galaxy bias modeling and corrections
- Redshift-space power spectra P(k, μ)
Two Flavors of Observables¶
cloelib has two types of observable protocols, each serving different purposes:
Tracer Protocol¶
For photometric observables (angular correlations, weak lensing)
SpectroPower Protocol¶
For spectroscopic observables (3D clustering, redshift-space distortions)
Next Steps¶
Ready to compute final statistics with your observables?
- Summary Statistics – Combine tracers into C_ℓ and multipoles
- Perturbations – Review structure formation
- Background – Review the foundation
- API Reference – Full technical details
- Back to Overview – Review the architecture