vide_public/python_tools/pipeline_source/defaults.py

132 lines
3.8 KiB
Python

#+
# VIDE -- Void IDEntification pipeline -- ./pipeline/datasets/mergertree.py
# Copyright (C) 2010-2013 Guilhem Lavaux
# Copyright (C) 2011-2013 P. M. Sutter
#
# This program is free software; you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation; version 2 of the License.
#
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License along
# with this program; if not, write to the Free Software Foundation, Inc.,
# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA.
#+
import os
# -----------------------------------------------------------------------------
# -----------------------------------------------------------------------------
# DEFAULT CONFIGURATION
startCatalogStage = 1
endCatalogStage = 3
startAPStage = 1
endAPStage = 5
continueRun = True
dataPortions = ["central"]
# directory for the input simulation/observational particle files
catalogDir = os.getenv("HOME")+"/workspace/Voids/catalog/"
# path to HOD code
hodPath = os.getenv("HOME")+"/projects/Voids/hod/HOD.x"
# where to put the final void catalog, figures, and output logs
voidOutputDir = os.getenv("HOME")+"/workspace/Voids//"
figDir = os.getenv("PWD")+"/../figs/"
logDir = os.getenv("PWD")+"/../logs/"
# where to place the pipeline scripts
scriptDir = os.getenv("PWD")+"/scripts//"
# simulation or observation?
dataType = "simulation"
# available formats for simulation: gadget, mergertree
dataFormat = "sdf"
dataUnit = 1 # as multiple of Mpc/h
# place particles on the lightcone?
useLightCone = False
# also do peculiar velocities?
doPecVel = False
# common filename of particle files
particleFileBase = "mf_4s_1G_512_NNNNN"
particleFileDummy = 'NNNNN'
# list of file numbers for the particle files
# to get particle file name, we take particleFileBase+fileNum
fileNums = ["0.667", "0.500"]
# redshift of each file in the above list
redshifts = ["0.5", "1.0"]
# how many independent slices along the z-axis?
numSlices = 1
# how many subdivisions along the x- and y- axis?
# ( = 2 will make 4 subvolumes for each slice, = 3 will make 9, etc.)
numSubvolumes = 1
# prefix to give all outputs
prefix = "mt_"
# list of desired subsamples - these are in unts of h Mpc^-3!
subSamples = [1.0]
doSubSampling = True # do the subsampling in preparation script?
# common filename of halo files, leave blank to ignore halos
haloFileBase = "mf_4s_1G_512_bgc2_NNNNN.sdf"
haloFileDummy = 'NNNNN'
# minimum halo mass cuts to apply for the halo catalog
# use "none" to get all halos
minHaloMasses = [1.2e13]
# locations of data in the halo catalog
haloFileMCol = 6
haloFileXCol = 0
haloFileYCol = 1
haloFileZCol = 2
haloFileVXCol = 3
haloFileVYCol = 4
haloFileVZCol = 5
haloFileColSep = ','
haloFileNumComLines = 0
# adjust these two parameters given the memory contraints on your system:
# numZobovDivisions: how many sub-volumes per dimension will zobov process
# numZobovThreads: how many sub-volumes to process at once?
numZobovDivisions = 2
numZobovThreads = 2
# simulation information
numPart = 512*512*512
lbox = 999.983 # Mpc/h
omegaM = 0.2847979853038958
hubble = 0.6962
#galDens = 0.000225
hodParmList = [
{'name' : "dr9mid", #BOSS: Manera et al. 2012, eq. 26
'Mmin' : 0.0,
'M1' : 1.e14,
'sigma_logM' : 0.596,
'alpha' : 1.0127,
'Mcut' : 1.19399e13,
'galDens' : 0.0002,
},
]
# END CONFIGURATION
# -----------------------------------------------------------------------------
# -----------------------------------------------------------------------------