mirror of
https://github.com/Richard-Sti/csiborgtools_public.git
synced 2025-05-12 13:41:13 +00:00
Calculate upglade redshifts (#128)
* Update redshift reading * Add helio to CMB redshift * Update imports * Update nb * Run for Quijote * Add script * Update * Update .gitignore * Update imports * Add Peery estimator * Add bulk flow scripts * Update typs * Add comment * Add blank space * Update submission script * Update description * Add barriers * Update nb * Update nb * Rename script * Move to old * Update imports * Add nb * Update script * Fix catalogue key * Update script * Update submit * Update comment * Update .gitignore * Update nb * Update for stationary obsrevers * Update submission * Add nb * Add better verbose control * Update nb * Update submit * Update nb * Add SN errors * Add draft of the script * Update verbosity flags * Add submission script * Debug script * Quickfix * Remove comment * Update nb * Update submission * Update nb * Processed UPGLADE
This commit is contained in:
parent
c447d2e7b0
commit
779f2e76ac
24 changed files with 2066 additions and 300 deletions
404
notebooks/match_observation/harry_clusters.ipynb
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404
notebooks/match_observation/harry_clusters.ipynb
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{
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"cells": [
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{
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"cell_type": "markdown",
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"metadata": {},
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"source": [
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"# Matching of haloes to clusters"
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]
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},
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{
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"cell_type": "code",
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"execution_count": 144,
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"metadata": {},
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"outputs": [
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{
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"name": "stdout",
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"output_type": "stream",
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"text": [
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"The autoreload extension is already loaded. To reload it, use:\n",
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" %reload_ext autoreload\n"
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]
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}
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],
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"source": [
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"import numpy as np\n",
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"import matplotlib.pyplot as plt\n",
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"from astropy.cosmology import FlatLambdaCDM\n",
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"\n",
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"import pandas as pd\n",
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"\n",
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"%load_ext autoreload\n",
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"%autoreload 2\n",
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"%matplotlib inline"
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]
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},
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{
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"cell_type": "markdown",
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"metadata": {},
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"source": [
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"### Load in the data\n",
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"Harry: the exact routine may not work, I had to edit the raw .txt file a little"
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]
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},
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{
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"cell_type": "code",
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"execution_count": 124,
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"metadata": {},
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"outputs": [
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{
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"name": "stdout",
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"output_type": "stream",
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"text": [
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"[34.14606699 9.28692846 11.11279198 16.85641068 3.71636485 33.43032196\n",
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" 24.65595192 29.91007806 40.31604335 9.346801 ]\n"
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]
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},
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{
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"data": {
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"text/html": [
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"<div>\n",
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"<style scoped>\n",
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" .dataframe tbody tr th:only-of-type {\n",
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" vertical-align: middle;\n",
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" }\n",
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"\n",
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" .dataframe tbody tr th {\n",
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" vertical-align: top;\n",
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" }\n",
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"\n",
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" .dataframe thead th {\n",
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" text-align: right;\n",
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" }\n",
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"</style>\n",
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"<table border=\"1\" class=\"dataframe\">\n",
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" <thead>\n",
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" <tr style=\"text-align: right;\">\n",
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" <th></th>\n",
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" <th>halo_ID</th>\n",
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" <th>KIND</th>\n",
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" <th>l[deg]</th>\n",
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" <th>b[deg]</th>\n",
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" <th>d[kpc]</th>\n",
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" <th>z</th>\n",
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" <th>Rdelta[kpc]</th>\n",
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" <th>rhos[Msol/kpc^3]</th>\n",
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" <th>rs[kpc]</th>\n",
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" <th>prof[keywrd]</th>\n",
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" <th>#1</th>\n",
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" <th>#2</th>\n",
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" <th>#3</th>\n",
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" <th>FOVDiam[deg]</th>\n",
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" </tr>\n",
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" </thead>\n",
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" <tbody>\n",
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" <tr>\n",
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" <th>0</th>\n",
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" <td>halo_647110</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>-47.66</td>\n",
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" <td>29.96</td>\n",
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" <td>-1</td>\n",
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" <td>0.01142</td>\n",
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" <td>4523.71</td>\n",
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" <td>643822.01573</td>\n",
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" <td>663.92743</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>37.74875</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>1</th>\n",
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" <td>halo_10128802</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>-90.76</td>\n",
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" <td>25.97</td>\n",
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" <td>-1</td>\n",
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" <td>0.00310</td>\n",
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" <td>1975.98</td>\n",
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" <td>611499.11522</td>\n",
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" <td>294.56973</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>60.00762</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>2</th>\n",
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" <td>halo_1338057</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>-35.42</td>\n",
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" <td>-6.15</td>\n",
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" <td>-1</td>\n",
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" <td>0.00371</td>\n",
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" <td>2738.50</td>\n",
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" <td>593219.40743</td>\n",
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" <td>413.73423</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>69.19885</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>3</th>\n",
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" <td>halo_20419495</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>87.42</td>\n",
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" <td>88.09</td>\n",
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" <td>-1</td>\n",
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" <td>0.00563</td>\n",
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" <td>3082.73</td>\n",
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" <td>596355.51967</td>\n",
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" <td>465.36921</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>51.83070</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>4</th>\n",
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" <td>halo_20355327</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>-94.48</td>\n",
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" <td>75.29</td>\n",
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" <td>-1</td>\n",
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" <td>0.00124</td>\n",
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" <td>1644.94</td>\n",
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" <td>635981.23866</td>\n",
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" <td>240.83028</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>119.66328</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>5</th>\n",
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" <td>halo_2503990</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>-35.24</td>\n",
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" <td>-12.06</td>\n",
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" <td>-1</td>\n",
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" <td>0.01118</td>\n",
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" <td>3164.45</td>\n",
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" <td>600754.77263</td>\n",
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" <td>478.21044</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>27.04669</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>6</th>\n",
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" <td>halo_21251859</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>31.15</td>\n",
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" <td>44.45</td>\n",
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||||
" <td>-1</td>\n",
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" <td>0.00824</td>\n",
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" <td>2731.34</td>\n",
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" <td>595715.63380</td>\n",
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" <td>413.32640</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>31.59913</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>7</th>\n",
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" <td>halo_745775</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>-47.49</td>\n",
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" <td>36.08</td>\n",
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" <td>-1</td>\n",
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" <td>0.01000</td>\n",
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" <td>2878.14</td>\n",
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" <td>597011.32933</td>\n",
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" <td>435.71418</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>27.49495</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>8</th>\n",
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" <td>halo_3003328</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>39.76</td>\n",
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" <td>-46.41</td>\n",
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" <td>-1</td>\n",
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" <td>0.01349</td>\n",
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" <td>3172.97</td>\n",
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" <td>602266.09230</td>\n",
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" <td>479.82208</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>22.50342</td>\n",
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" </tr>\n",
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" <tr>\n",
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" <th>9</th>\n",
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" <td>halo_4200359</td>\n",
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" <td>CLUSTER</td>\n",
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" <td>-28.67</td>\n",
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" <td>-22.77</td>\n",
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" <td>-1</td>\n",
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" <td>0.00312</td>\n",
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" <td>1826.88</td>\n",
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" <td>621061.51007</td>\n",
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" <td>270.55674</td>\n",
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" <td>kZHAO</td>\n",
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" <td>1.0</td>\n",
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" <td>3.0</td>\n",
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" <td>1.0</td>\n",
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" <td>55.35257</td>\n",
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" </tr>\n",
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" </tbody>\n",
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"</table>\n",
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"</div>"
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],
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"text/plain": [
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" halo_ID KIND l[deg] b[deg] d[kpc] z Rdelta[kpc] \\\n",
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"0 halo_647110 CLUSTER -47.66 29.96 -1 0.01142 4523.71 \n",
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"1 halo_10128802 CLUSTER -90.76 25.97 -1 0.00310 1975.98 \n",
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"2 halo_1338057 CLUSTER -35.42 -6.15 -1 0.00371 2738.50 \n",
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"3 halo_20419495 CLUSTER 87.42 88.09 -1 0.00563 3082.73 \n",
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"4 halo_20355327 CLUSTER -94.48 75.29 -1 0.00124 1644.94 \n",
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"5 halo_2503990 CLUSTER -35.24 -12.06 -1 0.01118 3164.45 \n",
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"6 halo_21251859 CLUSTER 31.15 44.45 -1 0.00824 2731.34 \n",
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"7 halo_745775 CLUSTER -47.49 36.08 -1 0.01000 2878.14 \n",
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"8 halo_3003328 CLUSTER 39.76 -46.41 -1 0.01349 3172.97 \n",
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"9 halo_4200359 CLUSTER -28.67 -22.77 -1 0.00312 1826.88 \n",
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"\n",
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" rhos[Msol/kpc^3] rs[kpc] prof[keywrd] #1 #2 #3 FOVDiam[deg] \n",
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"0 643822.01573 663.92743 kZHAO 1.0 3.0 1.0 37.74875 \n",
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"1 611499.11522 294.56973 kZHAO 1.0 3.0 1.0 60.00762 \n",
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"2 593219.40743 413.73423 kZHAO 1.0 3.0 1.0 69.19885 \n",
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"3 596355.51967 465.36921 kZHAO 1.0 3.0 1.0 51.83070 \n",
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"4 635981.23866 240.83028 kZHAO 1.0 3.0 1.0 119.66328 \n",
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"5 600754.77263 478.21044 kZHAO 1.0 3.0 1.0 27.04669 \n",
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"6 595715.63380 413.32640 kZHAO 1.0 3.0 1.0 31.59913 \n",
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"7 597011.32933 435.71418 kZHAO 1.0 3.0 1.0 27.49495 \n",
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"8 602266.09230 479.82208 kZHAO 1.0 3.0 1.0 22.50342 \n",
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"9 621061.51007 270.55674 kZHAO 1.0 3.0 1.0 55.35257 "
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]
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},
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"execution_count": 124,
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"metadata": {},
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"output_type": "execute_result"
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}
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],
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"source": [
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"\n",
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"cosmo = FlatLambdaCDM(H0=100, Om0=0.307)\n",
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"\n",
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"data0 = pd.read_csv(\"/mnt/users/rstiskalek/csiborgtools/data/top10_pwave_coords.txt\", sep='\\s+')\n",
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"data = {}\n",
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"\n",
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"data[\"id\"] = np.array([int(x.split(\"_\")[-1]) for x in data0[\"halo_ID\"].values])\n",
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"data[\"l\"] = data0[\"l[deg]\"].values\n",
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"data[\"b\"] = data0[\"b[deg]\"].values\n",
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"data[\"dist\"] = cosmo.comoving_distance(data0[\"z\"].values).value\n",
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"\n",
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"print(data[\"dist\"])\n",
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"data0"
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]
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},
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{
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"cell_type": "markdown",
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"metadata": {},
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"source": [
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"### Load in the halo catalogue"
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]
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},
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{
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"cell_type": "code",
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"execution_count": 126,
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"metadata": {},
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"outputs": [],
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"source": [
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"boxsize = 677.7\n",
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"\n",
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"halos = np.load(\"/users/hdesmond/Mmain/Mmain_9844.npy\")\n",
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"names = [\"id\", \"x\", \"y\", \"z\", \"M\"]\n",
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"halos = {k: halos[:, i] for i, k in enumerate(names)}\n",
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"halos[\"id\"] = halos[\"id\"].astype(int)\n",
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"# Coordinates are in box units. Convert to Mpc/h\n",
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"for p in (\"x\", \"y\", \"z\"):\n",
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" halos[p] = halos[p] * boxsize\n",
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"\n",
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"halos[\"dist\"] = np.sqrt((halos[\"x\"] - boxsize/2)**2 + (halos[\"y\"] - boxsize/2)**2 + (halos[\"z\"] - boxsize/2)**2)\n"
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]
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},
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{
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"cell_type": "code",
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"execution_count": 142,
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"metadata": {},
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"outputs": [
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{
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"name": "stdout",
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"output_type": "stream",
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"text": [
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"5791\n"
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]
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}
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],
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"source": [
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"# Find which item in the catalogue matches the nth halo in the .txt file\n",
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"n = 0\n",
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"k = np.where(data[\"id\"][n] == halos[\"id\"])[0][0]\n",
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"print(k)"
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]
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},
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{
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"cell_type": "code",
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"execution_count": 143,
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"metadata": {},
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"outputs": [
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{
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"data": {
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"text/plain": [
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"(34.14606698507264, 149.24046381654668)"
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]
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},
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"execution_count": 143,
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"metadata": {},
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"output_type": "execute_result"
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}
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],
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"source": [
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"data[\"dist\"][n], halos[\"dist\"][k]"
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]
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}
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],
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"metadata": {
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"kernelspec": {
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"display_name": "venv_csiborg",
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"language": "python",
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"name": "python3"
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},
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"language_info": {
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"codemirror_mode": {
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"name": "ipython",
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"version": 3
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},
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"file_extension": ".py",
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"mimetype": "text/x-python",
|
||||
"name": "python",
|
||||
"nbconvert_exporter": "python",
|
||||
"pygments_lexer": "ipython3",
|
||||
"version": "3.11.7"
|
||||
}
|
||||
},
|
||||
"nbformat": 4,
|
||||
"nbformat_minor": 2
|
||||
}
|
Loading…
Add table
Add a link
Reference in a new issue