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author | Aaron LI <aaronly.me@outlook.com> | 2016-10-28 21:33:43 +0800 |
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committer | Aaron LI <aaronly.me@outlook.com> | 2016-10-28 21:33:43 +0800 |
commit | dbfab5d3ce42f99df4a76c165d6300d09c65e9e4 (patch) | |
tree | e2110bb09d9b807ef36e532859d436d9ad262663 | |
parent | 1c2e43ebdc199136584099ec1c5ef743aff2457c (diff) | |
download | fg21sim-ps.tar.bz2 |
pointsources/base.py: Partially rewrite and FIXME marksps
NOTE: There are many "FIXME" needs further rewrite
-rw-r--r-- | fg21sim/extragalactic/pointsources/base.py | 237 |
1 files changed, 151 insertions, 86 deletions
diff --git a/fg21sim/extragalactic/pointsources/base.py b/fg21sim/extragalactic/pointsources/base.py index 1544f5b..101b6cb 100644 --- a/fg21sim/extragalactic/pointsources/base.py +++ b/fg21sim/extragalactic/pointsources/base.py @@ -1,97 +1,125 @@ # Copyright (c) 2016 Zhixian MA <zxma_sjtu@qq.com> +# Copyright (c) 2016 Weitian LI <liweitianux@live.com> # MIT license """ -Simulation of point sources for 21cm signal detection +Simulation the radio emissions from various types of point sources (PS) -Point sources types -------------------- -1. Star forming (SF) galaxies -2. Star bursting (SB) galaxies -3. Radio quiet AGN (RQ_AGN) -4. Faranoff-Riley I (FRI) -5. Faranoff-Riley II (FRII) +Currently supported PS types: + +* Star-forming (SF) galaxies +* Star-bursting (SB) galaxies +* Radio-quiet AGNs +* Radio-loud AGNs: Fanaroff-Riley type I (FRI) +* Radio-loud AGNs: Fanaroff-Riley type II (FRII) 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 -[2] Jelic et al., - "Foreground simulations for the LOFAR-Epoch of Reionization - Experiment", - 2008, MNRAS, 389, 1319-1335. - http://adsabs.harvard.edu/abs/2008MNRAS.389.1319W -[3] Spherical uniform distribution - https://www.jasondavies.com/maps/random-points/ +.. [Wilman2008] + 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 + +.. [Jelic2008] + Jelic et al., + "Foreground simulations for the LOFAR-Epoch of Reionization + Experiment", + 2008, MNRAS, 389, 1319-1335, + http://adsabs.harvard.edu/abs/2008MNRAS.389.1319W """ + + import os +import logging + import numpy as np +import astropy.units as au +from astropy.cosmology import FlatLambdaCDM import pandas as pd import healpy as hp -from .psparams import PixelParams +from ...utils.random import spherical_uniform + + +logger = logging.getLogger(__name__) class BasePointSource: """ - The basic class of point sources + Base class for point sources simulation + + FIXME: rewrite this doc string! - Parameters + Attributes ---------- - z: float; + z: float Redshift, z ~ U(0,20) dA: au.Mpc; Angular diameter distance, which is calculated according to the - cosmology constants. In this work, it is calculated by module - basic_params - lumo: au.Jy; - Luminosity at the reference frequency. + cosmology constants. + lumo: au.Jy; + Luminosity at the reference frequency lat: au.deg; - The colatitude angle in the spherical coordinate system + The latitude in the spherical coordinate system lon: au.deg; - The longtitude angle in the spherical coordinate system + The longitude in the spherical coordinate system area: au.sr; - Area of the point sources, sr = rad^2 - + Angular size/area of the point sources """ - # Init + # Identifier of the PS component + comp_id = "extragalactic/pointsources" + # ID of this PS type + ps_type = None + # Name of this PS type + name = None def __init__(self, configs): # configures self.configs = configs - # PS_list information + # FIXME: get rid of this `columns` + # Basic PS catalog columns self.columns = ['z', 'dA (Mpc)', 'luminosity (Jy)', 'Lat (deg)', 'Lon (deg)', 'Area (sr)'] - self.nCols = len(self.columns) self._set_configs() def _set_configs(self): - """ - Load the configs and set the corresponding class attributes. - """ - comp = "extragalactic/pointsources/" - # common + """Load the configs and set the corresponding class attributes.""" + # Configurations shared between all supported PS types + comp = self.comp_id + self.resolution = self.configs.getn(comp+"/resolution") * au.arcmin + self.catalog_pattern = self.configs.getn(comp+"/catalog_pattern") + self.save = self.configs.getn(comp+"/save") + self.output_dir = self.configs.get_path(comp+"/output_dir") + # Specific configurations for this PS type + pstype = "/".join([self.comp_id, self.ps_type]) + self.number = self.configs.getn(pstype+"/number") + self.prefix2 = self.configs.getn(pstype+"/prefix2") + self.save2 = self.configs.getn(pstype+"/save2") + # + self.use_float = self.configs.getn("output/use_float") + self.clobber = self.configs.getn("output/clobber") self.nside = self.configs.getn("common/nside") - # resolution - self.resolution = self.configs.getn(comp+"resolution") - # save flag - self.save = self.configs.getn(comp+"save") - # Output_dir - self.output_dir = self.configs.get_path(comp+"output_dir") + self.npix = hp.nside2npix(self.nside) + # Cosmology model + self.H0 = self.configs.getn("cosmology/H0") + self.OmegaM0 = self.configs.getn("cosmology/OmegaM0") + self.cosmo = FlatLambdaCDM(H0=self.H0, Om0=self.OmegaM0) + # + logger.info("Loaded and set up configurations") def calc_number_density(self): - pass + raise NotImplementedError("Sub-class must implement this method!") + # FIXME: directly sample from joint distribution of z and flux/luminosity def calc_cdf(self): """ Calculate cumulative distribution functions for simulating of samples with corresponding reshift and luminosity. - Parameter - ----------- + Parameters + ---------- rho_mat: np.ndarray rho(lumo,z) The number density matrix (joint-distribution of z and flux) of this type of PS. @@ -111,6 +139,7 @@ class BasePointSource: # Cumulative function cdf_z = np.zeros(pdf_z.shape) cdf_lumo = np.zeros(pdf_lumo.shape) + # FIXME: use `cumsum()` for i in range(len(pdf_z)): cdf_z[i] = np.sum(pdf_z[:i]) for i in range(len(pdf_lumo)): @@ -118,12 +147,13 @@ class BasePointSource: return cdf_z, cdf_lumo + # FIXME: get rid of self.* ! def get_lumo_redshift(self): """ Randomly generate redshif and luminosity at ref frequency using the CDF functions. - Paramaters + Parameters ---------- df_z, cdf_lumo: np.ndarray Cumulative distribution functions of redshift and flux. @@ -136,8 +166,7 @@ class BasePointSource: Redshift. lumo: au.W/Hz/sr Luminosity. - """ - # Uniformlly generate random number in interval [0,1] + """ rnd_z = np.random.uniform(0, 1) rnd_lumo = np.random.uniform(0, 1) # Get redshift @@ -148,56 +177,92 @@ class BasePointSource: dist_lumo = np.abs(self.cdf_lumo - rnd_lumo) idx_lumo = np.where(dist_lumo == dist_lumo.min()) lumo = 10 ** self.lumobin[idx_lumo[0]] - return float(z), float(lumo) + # FIXME: Get rid of this function! def gen_single_ps(self): - """ - Generate single point source, and return its data as a list. - """ + """Generate the information of one single point source""" # Redshift and luminosity - self.z, self.lumo = self.get_lumo_redshift() + z, lumo = self.get_lumo_redshift() # angular diameter distance - self.param = PixelParams(self.z) - self.dA = self.param.dA - # W/Hz/Sr to Jy - dA = self.dA * 3.0856775814671917E+22 # Mpc to meter - self.lumo = self.lumo / dA**2 / (10.0**-24) # [Jy] + DA = self.cosmo.angular_diameter_distance(z).to(au.Mpc).value + # [ W/Hz/sr ] => [ Jy ] + DA_m = DA * 3.0856775814671917E+22 # Mpc to meter + lumo = lumo / DA_m**2 / 1e-24 # [Jy] # Position - x = np.random.uniform(0, 1) - self.lat = (np.arccos(2 * x - 1) / np.pi * 180 - 90) # [deg] - self.lon = np.random.uniform(0, np.pi * 2) / np.pi * 180 # [deg] + theta, phi = spherical_uniform() + glon = np.rad2deg(phi) + glat = 90.0 - np.rad2deg(theta) # Area - npix = hp.nside2npix(self.nside) - self.area = 4 * np.pi / npix # [sr] - - ps_list = [self.z, self.dA, self.lumo, self.lat, self.lon, self.area] - return ps_list + area = 4 * np.pi / self.npix # [sr] + ps_data = [z, DA_m, lumo, glat, glon, area] + return ps_data + # FIXME: The catalog should be simulated on the column based, not on + # single PS based, which slows the speed! def gen_catalog(self): """ Generate num_ps of point sources and save them into a csv file. """ - # Init - ps_table = np.zeros((self.num_ps, self.nCols)) - for x in range(self.num_ps): - ps_table[x, :] = self.gen_single_ps() - - # Transform into Dataframe - self.ps_catalog = pd.DataFrame(ps_table, columns=self.columns, - index=list(range(self.num_ps))) + shape = (self.number, len(self.columns)) + catalog = np.zeros(shape) + for i in range(shape[0]): + catalog[i, :] = self.gen_single_ps() + self.catalog = pd.DataFrame(catalog, columns=self.columns) + logger.info("Done simulate the catalog") - def save_as_csv(self): + def save_catalog(self): """Save the catalog""" if not os.path.exists(self.output_dir): os.mkdir(self.output_dir) + logger.info("Created output directory: %s" % self.output_dir) + # Append the prefix for the specific PS type + if self.prefix2 is not None: + prefix = "_".join([self.prefix, self.prefix2]) + filepath = self._make_filepath(pattern=self.catalog_pattern, + prefix=prefix) + # Save catalog data + if os.path.exists(filepath): + if self.clobber: + logger.warning("Remove existing catalog file: %s" % filepath) + os.remove(filepath) + else: + raise OSError("Output file already exists: %s" % filepath) + self.catalog.to_csv(filepath, header=True, index=False) + logger.info("Save clusters catalog in use to: {0}".format(filepath)) - pattern = "{prefix}.csv" - filename = pattern.format(prefix=self.prefix) + def output(self): + raise NotImplementedError("TODO") - # save to csv - if self.save: - file_name = os.path.join(self.output_dir, filename) - self.ps_catalog.to_csv(file_name) + def _make_filepath(self, pattern=None, **kwargs): + """Make the path of output file according to the filename pattern + and output directory loaded from configurations. - return file_name + Parameters + ---------- + pattern : str, optional + Specify the filename (without the extension) pattern in string + format template syntax. If not specified, then use + ``self.filename_pattern``. + **kwargs : optional + Other named parameters used to format the filename pattern. + + Returns + ------- + filepath : str + The full path to the output file (with directory and extension). + """ + data = { + "prefix": self.prefix, + } + data.update(kwargs) + if pattern is None: + pattern = self.filename_pattern + filename = pattern.format(**data) + filetype = self.configs.getn("output/filetype") + if filetype == "fits": + filename += ".fits" + else: + raise NotImplementedError("unsupported filetype: %s" % filetype) + filepath = os.path.join(self.output_dir, filename) + return filepath |