Source code for dustmaps.planck

#!/usr/bin/env python
#
# planck.py
# Reads the Planck Collaboration dust reddening maps.
#
# Copyright (C) 2016  Gregory M. Green
#
# 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 2 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License along
# with this program; if not, write to the Free Software Foundation, Inc.,
# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA.
#

from __future__ import print_function, division

import os
import numpy as np
import healpy as hp
import astropy.io.fits as fits
import astropy.units as units

from .std_paths import *
from .healpix_map import HEALPixFITSQuery
from . import fetch_utils
from . import dustexceptions


[docs]class PlanckQuery(HEALPixFITSQuery): """ Queries the Planck Collaboration (2013) dust map. """
[docs] def __init__(self, map_fname=None, component='extragalactic'): """ Args: map_fname (Optional[:obj:`str`]): Filename of the Planck map. Defaults to ```None``, meaning that the default location is used. component (Optional[:obj:`str`]): Which measure of reddening to use. There are seven valid components. Three denote reddening measures: ``'extragalactic'``, ``'tau'`` and ``'radiance'``. Four refer to dust properties: ``'temperature'``, ``'beta'``, ``'err_temp'`` and ``'err_beta'``. Defaults to ``'extragalactic'``. """ if map_fname is None: map_fname = os.path.join( data_dir(), 'planck', 'HFI_CompMap_ThermalDustModel_2048_R1.20.fits' ) if component.lower() in ('ebv','extragalactic'): field = 'EBV' self._scale = 1. elif component.lower() in ('tau','tau353','tau_353','optical depth'): field = 'TAU353' self._scale = 1.49e4 elif component.lower() in ('radiance','r'): field = 'RADIANCE' self._scale = 5.4e5 elif component.lower() in ('temperature','temp','t'): field = 'TEMP' self._scale = units.Kelvin elif component.lower() in ('sigma_temp','sigma_t','err_temp','err_t'): field = 'ERR_TEMP' self._scale = units.Kelvin elif component.lower() in ('beta','b'): field = 'BETA' self._scale = 1. elif component.lower() in ('sigma_beta','sigma_b','err_beta','err_b'): field = 'ERR_BETA' self._scale = 1. else: raise ValueError(( "Invalid `component`: '{}'\n" "Valid components for reddening are 'extragalactic', 'tau', " "and 'radiance'. Valid components for dust properties are " "'temperature', 'err_temp', 'beta' and 'err_beta'." ).format(component)) try: with fits.open(map_fname) as hdulist: super(PlanckQuery, self).__init__( hdulist, 'galactic', hdu='COMP-MAP', field=field, dtype='f4', scale=self._scale ) except IOError as error: print(dustexceptions.data_missing_message('planck', 'Planck Collaboration')) raise error
[docs] def query(self, coords, **kwargs): """ Returns E(B-V) (or a different Planck dust inference, depending on how the class was intialized) at the specified location(s) on the sky. Args: coords (:obj:`astropy.coordinates.SkyCoord`): The coordinates to query. Returns: A float array of the selected Planck component, at the given coordinates. The shape of the output is the same as the shape of the input coordinate array, ``coords``. If extragalactic E(B-V), tau_353 or radiance was chosen, then the output has units of magnitudes of E(B-V). If the selected Planck component is temperature (or temperature error), then an :obj:`astropy.Quantity` is returned, with units of Kelvin. If beta (or beta error) was chosen, then the output is unitless. """ return super(PlanckQuery, self).query(coords, **kwargs)
[docs]class PlanckGNILCQuery(HEALPixFITSQuery): """ Queries the Planck Collaboration (2016) GNILC dust map. """
[docs] def __init__(self, map_fname=None, load_errors=False): """ Args: map_fname (Optional[:obj:`str`]): Filename of the Planck map. Defaults to ```None``, meaning that the default location is used. load_errors (Optional[:obj:`str`]): If ``True``, then the error estimates will be loaded as well, and returned with any query. If ``False`` (the default), then queries will only return the the reddening estimate, without any error estimate. """ if load_errors: self._has_errors = True field = None dtype = [('EBV','f4'), ('EBV_err','f4')] else: self._has_errors = False field = 'TAU353' dtype = 'f4' if map_fname is None: map_fname = os.path.join( data_dir(), 'planck', 'COM_CompMap_Dust-GNILC-Model-Opacity_2048_R2.01.fits' ) try: with fits.open(map_fname) as hdulist: super(PlanckGNILCQuery, self).__init__( hdulist, 'galactic', hdu=1, field=field, dtype=dtype, scale=1.49e4 ) except IOError as error: print(dustexceptions.data_missing_message('planck', 'Planck GNILC')) raise error
[docs] def has_errors(self): """ Returns ``True`` if the error estimates have been loaded. """ return self._has_errors
[docs] def query(self, coords, **kwargs): """ Returns E(B-V) at the specified location(s) on the sky. Args: coords (:obj:`astropy.coordinates.SkyCoord`): The coordinates to query. Returns: If the error estimates have been loaded, then a structured array containing ``'EBV'`` and ``'EBV_err'`` is returned. Otherwise, returns a float array of E(B-V), at the given coordinates. The shape of the output is the same as the shape of the input coordinate array, ``coords``. """ return super(PlanckGNILCQuery, self).query(coords, **kwargs)
[docs]def fetch(which='2013'): """ Downloads the Planck dust maps, placing them in the default ``dustmaps`` directory. There are two different Planck dust maps that can be downloaded: the Planck Collaboration (2013) map and the "GNILC" (Planck Collaboration 2016) map. Args: which (Optional[:obj:`str`]): The name of the dust map to download. Should be either ``2013`` (the default) or ``GNILC``. """ planck_maps = { '2013': { 'url': 'http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=HFI_CompMap_ThermalDustModel_2048_R1.20.fits', 'md5': '8d804f4e64e709f476a63f0dfed1fd11', 'fname': 'HFI_CompMap_ThermalDustModel_2048_R1.20.fits' }, 'GNILC': { 'url': 'http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=COM_CompMap_Dust-GNILC-Model-Opacity_2048_R2.01.fits', 'md5': 'fc385c2ee5e82edf039cbca6e82d6872', 'fname': 'COM_CompMap_Dust-GNILC-Model-Opacity_2048_R2.01.fits' } } if which not in planck_maps: raise ValueError( 'Unknown map: "{}". Must be one of {}.'.format( which, tuple(planck_maps.keys()) ) ) props = planck_maps[which] fname = os.path.join(data_dir(), 'planck', props['fname']) fetch_utils.download_and_verify(props['url'], props['md5'], fname=fname)
def main(): from astropy.coordinates import SkyCoord q = PlanckQuery() c = SkyCoord([0., 180., 0.], [0., 0., 90.], frame='galactic', unit='deg') print(q(c)) if __name__ == '__main__': main()