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# Copyright (c) 2016 Zhixian MA <zxma_sjtu@qq.com>
# MIT license
import numpy as np
import healpy as hp
from .base import BasePointSource
from ...utils import convert
class RadioQuiet(BasePointSource):
def __init__(self, configs):
super().__init__(configs)
self._set_configs()
# Number density matrix
self.rho_mat = self.calc_number_density()
# Cumulative distribution of z and lumo
self.cdf_z, self.cdf_lumo = self.calc_cdf()
def _set_configs(self):
"""Load the configs and set the corresponding class attributes"""
super()._set_configs()
pscomp = "extragalactic/pointsources/radioquiet/"
# point sources amount
self.num_ps = self.configs.getn(pscomp+"numps")
# prefix
self.prefix = self.configs.getn(pscomp+"prefix")
# redshift bin
z_type = self.configs.getn(pscomp+"z_type")
if z_type == 'custom':
start = self.configs.getn(pscomp+"z_start")
stop = self.configs.getn(pscomp+"z_stop")
step = self.configs.getn(pscomp+"z_step")
self.zbin = np.arange(start, stop + step, step)
else:
self.zbin = np.arange(0.1, 10, 0.05)
# luminosity bin
lumo_type = self.configs.getn(pscomp+"lumo_type")
if lumo_type == 'custom':
start = self.configs.getn(pscomp+"lumo_start")
stop = self.configs.getn(pscomp+"lumo_stop")
step = self.configs.getn(pscomp+"lumo_step")
self.lumobin = np.arange(start, stop + step, step)
else:
self.lumobin = np.arange(18.7, 25.7, 0.1) # [W/Hz/sr]
def calc_number_density(self):
"""
Calculate number density rho(lumo,z) of FRI
References
------------
[1] Wilman et al.,
"A semi-empirical simulation of the extragalactic radio continuum
sky for next generation radio telescopes",
2008, MNRAS, 388, 1335-1348.
http://adsabs.harvard.edu/abs/2008MNRAS.388.1335W
Returns
-------
rho_mat: np.ndarray
Number density matris (joint-distribution of luminosity and
reshift).
"""
# Init
rho_mat = np.zeros((len(self.lumobin), len(self.zbin)))
# Parameters
# Refer to Willman's section 2.4
alpha = 0.7 # spectral index
lumo_star = 10.0**21.3 # critical luminosity at 1400MHz
rho_l0 = 10.0**(-7) # normalization constant
z1 = 1.9 # cut-off redshift
k1 = -3.27 # index of space density revolution
# Calculation
for i, z in enumerate(self.zbin):
if z <= z1:
rho_mat[:, i] = ((rho_l0 * (10**self.lumobin / lumo_star) **
(-alpha) *
np.exp(-10**self.lumobin / lumo_star)) *
(1 + z)**k1)
else:
rho_mat[:, i] = ((rho_l0 * (10**self.lumobin / lumo_star) **
(-alpha) *
np.exp(-10**self.lumobin / lumo_star)) *
(1 + z1)**k1)
return rho_mat
def draw_single_ps(self, freq):
"""
Designed to draw the radio quiet AGN
Parameters
----------
ImgMat: np.ndarray
Two dimensional matrix, to describe the image
self.ps_catalog: pandas.core.frame.DataFrame
Data of the point sources
freq: float
frequency
"""
# Init
npix = hp.nside2npix(self.nside)
hpmap = np.zeros((npix,))
# Gen Tb list
Tb_list = self.calc_Tb(freq)
# Iteratively draw the ps
num_ps = self.ps_catalog.shape[0]
for i in range(num_ps):
# Angle to pix
lat = (self.ps_catalog['Lat (deg)'] + 90) / 180 * np.pi
lon = self.ps_catalog['Lon (deg)'] / 180 * np.pi
pix = hp.ang2pix(self.nside, lat, lon)
# Gen hpmap
hpmap[pix] += Tb_list[i]
return hpmap
def draw_ps(self, freq):
"""
Read csv ps list file, and generate the healpix structure vector
with the respect frequency.
"""
# Init
num_freq = len(freq)
npix = hp.nside2npix(self.nside)
hpmaps = np.zeros((npix, num_freq))
# Gen ps_catalog
self.gen_catalog()
# get hpmaps
for i in range(num_freq):
hpmaps[:, i] = self.draw_single_ps(freq[i])
return hpmaps
def calc_single_Tb(self, area, freq):
"""
Calculate brightness temperatur of a single ps
Parameters
------------
area: `~astropy.units.Quantity`
Area of the PS, e.g., `1.0*au.sr2`
freq: `~astropy.units.Quantity`
Frequency, e.g., `1.0*au.MHz`
Return
------
Tb:`~astropy.units.Quantity`
Average brightness temperature, e.g., `1.0*au.K`
"""
# Init
freq_ref = 1400 # [MHz]
freq = freq # [MHz]
# Luminosity at 1400MHz
lumo_1400 = self.lumo # [Jy]
# Calc flux
flux = (freq / freq_ref)**(-0.7) * lumo_1400
# Calc brightness temperature
Tb = convert.Fnu_to_Tb_fast(flux, area, freq)
return Tb
def calc_Tb(self, freq):
"""
Calculate the surface brightness temperature of the point sources.
Parameters
------------
area: `~astropy.units.Quantity`
Area of the PS, e.g., `1.0*au.sr`
freq: `~astropy.units.Quantity`
Frequency, e.g., `1.0*au.MHz`
Return
------
Tb_list: list
Point sources brightness temperature
"""
# Tb_list
num_ps = self.ps_catalog.shape[0]
Tb_list = np.zeros((num_ps,))
# Iteratively calculate Tb
for i in range(num_ps):
ps_area = self.ps_catalog['Area (sr)'][i] # [sr]
Tb_list[i] = self.calc_single_Tb(ps_area, freq)
return Tb_list
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