vide_public/c_source/prep/prepObservation.ggo
Paul M. Sutter 3dce2593d9 Implemented (yet another) new boundary handling scheme, whereby we scan radially along survey edge while flagging nearest galaxies. The prepObservation routine was significantly cleaned up to accommodate this, but it was ultimately implemented in python (surveyTools.py) for ease of prototyping, with the intent to move it back into C later.
Some general housekeeping, making sure some new parameters are passed around correctly, and removing the storage of some unused files.

This update is considered HIGHLY UNSTABLE. It will almost certainly break somewhere for simulations.

Still under active development.
2025-01-07 20:04:29 +08:00

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package "prepObservation"
version "alpha"
option "configFile" - "Configuration filename" string optional
option "catalog" - "Input NYU-VAGC catalog" string required
option "mask" - "Healpix mask of unobserved data (in Equatorial coordinates)" string required
option "density_fake" - "Number density of boundary fake tracers (1 h^3/ Mpc^3)" double optional default="1"
option "zMin" - "Minimum redshift of data" double required
option "zMax" - "Maximum redshift of data" double required
option "output" - "Filename of particle datafile" string required
option "params" - "Output parameters of the datacube" string required
option "useComoving" - "Convert to real space using LCDM cosmology" flag off
option "omegaM" - "Omega Matter for fiducial cosmology" double optional default="0.27"
option "nsideForContour" - "HEALPix NSIDE resolution for figuring out mask contours" int optional default="-1"
option "meanPartSep" - "Estimated mean tracer seperation in h^3 / Mpc^3" double optional default="1"