email: [email protected]
Building tools for reconstructing and using large-scale velocity modes
Reconstructed modes are very valuable for cosmological inference as their reconstruction noise scales like and provide better signal-to-noise on largest scales. This makes velocity modes very useful for sample-variance cancellation.
This rep includes various tools and pipelines for reconstruction large-scale velocities from maps of cosmic microwave background (CMB) and galaxy-surveys.
tools include: (work on progress)
- 3D velocity template reconstruction from halo catalogs
- uses galaxy catalog to compute 3D overdensity field.
- uses the 3D overdensity field to compute 3D velocity 3-vector.
- makes redshift-binned healpix maps out of 3D velocities
Requires:
healpy
nbodykit
- stacking algoritm for moving lens effect
- uses halo distributions and CMB maps (with moving lens effect).
- orients CMB patches to be aligned with the velocity field template.
- fits a grid with fixed size in where is the scale radius. (See related stacker description.)
- stacks the grids to extract the signal.
Moving lens signal is a dipolar modulation in the CMB, alighed with the peculiar velocities of gravitational potentials, e.g. arxiv:1812.03167
where
similar to the lensing deflection angle. (See more notes at the stacker folder.)
Requires:
healpy
- moving lens effect map maker: https://github.com/jbmertens/websky_post
- uses halo catalog to paint maps of the moving-lens effect.
Requires:
healpy
see also related work by Siavash Yasini https://github.com/syasini/AstroPaint
- spherical harmonic reconstruction of the transverse velocities: https://github.com/jbmertens/websky_post (work on progress)
Requires:
healpy