/Mop-c-GT

Model-to-observable projection code for galaxy thermodynamics

Primary LanguagePython

Mop-c GT

Model-to-observable projection code for galaxy thermodynamics

Authors: Stefania Amodeo, Nicholas Battaglia

Requirements: numpy, scipy.

Takes in input models of density and pressure radial profiles of halos of given mass and redshift.

Returns 2D profiles of observable quantities, specifically the temperature shifts in CMB maps measured within disks of varying radii due to the kSZ and tSZ effects, respectively, by implementing:

  • line-of-sight projection
  • instrumental beam convolution
  • aperture photometry filter

Applications to:

  • generalized NFW parametric models
  • polytropic gas model based on Ostriker, Bode, Balbus (2005).

Includes implementation of the analytical model of the “two-halo term” (contribution to the halo gas profiles from neighboring halos), following the halo model of Vikram et al. (2017) (based on the formalism of Cooray & Sheth 2002).

Extra packages needed for the two-halo computation:

Presented in Amodeo et al. 2021 Phys. Rev. D, 103, 063514

DOI: 10.1103/PhysRevD.103.063514

arXiv:2009.05558