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#Results from heasarc_fermilpsc: Fermi LAT 4-Year Point Source Catalog | |
#Coordinate system: Galactic | |
|name |_Lii |_Bii |flux_1_100_gev|flux_1_100_gev_error|spectral_index|spectral_index_error|detection_significance|assoc_name_1 |lii |bii |semi_major_axis_68|semi_minor_axis_68|position_angle_68|semi_major_axis_95|semi_minor_axis_95|position_angle_95|pivot_energy|flux_density|flux_density_error|energy_flux|energy_flux_error|curve_significance|spectrum_type |beta |beta_error|cutoff |cutoff_error|exp_index|exp_index_error|powerlaw_index|flux_30_100_mev|flux_30_100_mev_pos_err|flux_30_100_mev_neg_err|nufnu_30_100_mev|sqrt_ts_30_100_mev|flux_100_300_mev|flux_100_300_mev_pos_err|flux_100_300_mev_neg_err|nufnu_100_300_mev|sqrt_ts_100_300_mev|flux_0p3_1_gev|flux_0p3_1_gev_pos_err|flux_0p3_1_gev_neg_err|nufnu_0p3_1_gev|sqrt_ts_0p3_1_gev|flux_1_3_gev|flux_1_3_gev_pos_err|flux_1_3_gev_neg_err|nufnu_1_3_gev|sqrt_ts_1_3_gev|flux_3_10_gev|flux_3_10_gev_pos_err|flux_3_10_gev_neg_er |
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#!/usr/bin/env bash | |
# rmate | |
# Copyright (C) 2011-2015 by Harald Lapp <[email protected]> | |
# | |
# 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, either version 3 of the License, or | |
# (at your option) any later version. | |
# |
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############################################################################### | |
# run_11bin.py | |
############################################################################### | |
# | |
# Perform scan to obtain best-fit disk and bulge PS population parameters | |
# | |
# Here using the 4D efficiency function and the new 11 binning | |
# | |
############################################################################### |
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import numpy as np | |
from astropy.cosmology import Planck15 | |
from units import * | |
import sys, os | |
if os.environ['DIFF']: # Whether to use Theano version of lensing gradients | |
from profiles_theano import * | |
else: | |
from profiles import * |
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import numpy as np | |
import sys | |
sys.path.append("../Lensing-PowerSpectra/Simulations/") | |
from units import * | |
import theano.tensor as tt | |
def deflection_sis(x, y, x0=0, y0=0, b=1.5): | |
""" Deflection for singular isothermal ellipsoid, from astro-ph/0102341 | |
""" | |
# Go into shifted coordinats of the potential |
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%%cython | |
import cython | |
cimport cython | |
import numpy as np | |
cimport numpy as np | |
import warnings |
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# define a theano Op for our likelihood function | |
class LogLikeWithGrad(tt.Op): | |
itypes = [tt.dvector] # expects a vector of parameter values when called | |
otypes = [tt.dscalar] # outputs a single scalar value (the log likelihood) | |
def __init__(self, loglike): | |
""" | |
Initialise with various things that the function requires. Below | |
are the things that are needed in this particular example. |
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jupyter nbconvert --to rst examples/*.ipynb | |
rm -r docs/Example* | |
mv examples/*rst examples/*_files docs/ | |
cd docs/ | |
perl -pi -w -e 's/.. code:: ipython3/.. code:: python/g;' *.rst |