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Tools for measuring Intrinsic Alignments in spectroscopic data

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cmlamman/spec-IA

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spec-IA

This repository contains tools for measuring intrinsic alignments of galaxies and galaxy groups in spectroscopic data.

Installation

spec-IA requires Python and the following libraries:

  • NumPy
  • Matplotlib
  • Pandas
  • SciPy
  • Astropy
  • Corrfunc (optional, for correlation functions)

These can be installed through pip:

bash pip install numpy matplotlib pandas scipy astropy

or conda:

bash conda install numpy matplotlib pandas scipy astropy

The repository can be cloned via

bash git clone https://github.com/cmlamman/spec-IA

Group Alignment

gal_groups.py contains functions for identifying and measuring the alignment of galaxy groups. The alignment estimator is defined as the projected orienation of groups relative to a tracer sample, $\cos(2\Theta)$, as a function of projected separation $R$. A high-level example of this can be found in basic_group_alignment.ipynb.

The minimum to run these basic functions is a catalog with the columns RA, DEC (in degrees) and Z (redshift).

schematic

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