author: ginevra favole, johan comparat.
contact: g.favole@csic.es, johan.comparat_at_gmail.com


Acknowledgement:
================

If you use these results, please cite Favole, Comparat et al. 2016 :
http://adsabs.harvard.edu/abs/2016MNRAS.461.3421F

Mocks for ELG at z=0.8
======================

Each mock is characterized by 3 parameters: 

The halo mass distribution is characterized by a Gaussian with XX as a mean and YY as scatter. The third parameter is the fraction of satellite : ZZ.

For each mock, you have the following files :

MOCKS : 
-------

SHAM_norm-meanXX-sigYY-fsatZZ_ELGdensity_allCols.cat.gz
is the complete catalog that contains ra, dec, redshift, halo mass, central / satelite flag

SHAM_norm-meanXX-sigYY-fsatZZ_ELGdensity_radecz.cat
same as before but only the columns ra,dec,z

SHAM_norm-meanXX-sigYY-fsatZZ_ELGdensity_radecz.cat.random.cat
is a random unclustered catalog with the same ra, dec, redshift distribution.

DERIVED QUANTITIES :
--------------------

SHAM_norm-meanXX-sigYY-fsatZZ_ELGdensity_allCols.pdf
is a plot showing log halo mass vs. redshift of the catalog. It gives the exact fraction of satellite.

SHAM_norm-meanXX-sigYY-fsatZZ_ELGdensity_radecz_angular_combined.dat
is the angular clustering of the mock. theta, w(theta), poisson errors, DD, DR, RR

SHAM_norm-meanXX-sigYY-fsatZZ_ELGdensity_radecz_monopole.dat
is the monopole clustering of the mock. s, xi(s), poisson errors, DD, DR, RR