def test_file_check(test_directory, test_file):
assert not file_existing_and_readable(test_directory)
assert not file_existing_and_readable("this_does_not_exist")
assert file_existing_and_readable(test_file)
def __init__(self, name, maptree, response, n_transits=None, **kwargs):
# This controls if the likeHAWC class should load the entire
# map or just a small disc around a source (faster).
# Default is the latter, which is way faster. LIFF will decide
# autonomously which ROI to use depending on the source model
self.fullsky = False
if 'fullsky' in kwargs.keys():
self.fullsky = bool(kwargs['fullsky'])
self.name = str(name)
# Sanitize files in input (expand variables and so on)
self.maptree = os.path.abspath(sanitize_filename(maptree))
self.response = os.path.abspath(sanitize_filename(response))
# Check that they exists and can be read
if not file_existing_and_readable(self.maptree):
raise IOError("MapTree %s does not exist or is not readable" % maptree)
if not file_existing_and_readable(self.response):
raise IOError("Response %s does not exist or is not readable" % response)
# Post-pone the creation of the LIFF instance to when
# we have the likelihood model
self.instanced = False
# Number of transits
if n_transits is not None:
self._n_transits = float(n_transits)
else:
self._n_transits = None
# Default value for minChannel and maxChannel
self.minChannel = int(defaultMinChannel)
self.maxChannel = int(defaultMaxChannel)
# By default the fit of the CommonNorm is deactivated
self.deactivateCommonNorm()
# This is to keep track of whether the user defined a ROI or not
self.roi_ra = None
# Further setup
self.__setup()
def build_filter_library():
if not file_existing_and_readable(os.path.join(get_speclite_filter_path(),'filter_lib.yml')):
print ('Downloading optical filters. This will take a while.\n')
if internet_connection_is_active():
filter_dict={}
filter_dict = download_SVO_filters(filter_dict)
filter_dict = download_grond(filter_dict)
# Ok, finally, we want to keep track of the SVO filters we have
# so we will save this to a YAML file for future reference
with open(os.path.join(get_speclite_filter_path(),'filter_lib.yml'), 'w') as f:
yaml.safe_dump(filter_dict, f, default_flow_style=False)
return True
else:
print ("You do not have the 3ML filter library and you do not have an active internet connection.")
print ("Please connect to the internet to use the 3ML filter library.")
print ("pyspeclite filter library is still available.")
return False
else:
return True
def build_filter_library():
if not file_existing_and_readable(os.path.join(get_speclite_filter_path(),'filter_lib.yml')):
print ('Downloading optical filters. This will take a while.\n')
if internet_connection_is_active():
filter_dict={}
filter_dict = download_SVO_filters(filter_dict)
filter_dict = download_grond(filter_dict)
# Ok, finally, we want to keep track of the SVO filters we have
# so we will save this to a YAML file for future reference
with open(os.path.join(get_speclite_filter_path(),'filter_lib.yml'), 'w') as f:
yaml.safe_dump(filter_dict, f, default_flow_style=False)
return True
else:
print ("You do not have the 3ML filter library and you do not have an active internet connection.")
print ("Please connect to the internet to use the 3ML filter library.")
print ("pyspeclite filter library is still available.")
return False
else:
return True
def _read_arf_file(self, arf_file):
"""
read an arf file and apply it to the current_matrix
:param arf_file:
:param current_matrix:
:param current_mc_channels:
:return:
"""
arf_file = sanitize_filename(arf_file)
self._arf_file = arf_file
assert file_existing_and_readable(arf_file.split("{")[0]), "Ancillary file %s not existing or not " \
"readable" % arf_file
with pyfits.open(arf_file) as f:
data = f['SPECRESP'].data
arf = data.field('SPECRESP')
# Check that arf and rmf have same dimensions
if arf.shape[0] != self.matrix.shape[1]:
raise IOError(
"The ARF and the RMF file does not have the same number of channels"
)
# Check that the ENERG_LO and ENERG_HI for the RMF and the ARF
# are the same
energ_lo = data.field("ENERG_LO")
energ_hi = data.field("ENERG_HI")
assert self._are_contiguous(
energ_lo,
energ_hi), "Monte carlo energies in ARF are not contiguous!"
arf_mc_channels = np.append(energ_lo, [energ_hi[-1]])
# Declare the mc channels different if they differ by more than 1%
idx = (self.monte_carlo_energies > 0)
diff = old_div((self.monte_carlo_energies[idx] - arf_mc_channels[idx]),
self.monte_carlo_energies[idx])
if diff.max() > 0.01:
raise IOError(
"The ARF and the RMF have one or more MC channels which differ by more than 1%"
)
# Multiply ARF and RMF
matrix = self.matrix * arf
# Override the matrix with the one multiplied by the arf
self.replace_matrix(matrix)
def from_rsp2_file(cls, rsp2_file, exposure_getter, counts_getter, reference_time=0.0, half_shifted=True):
# This assumes the Fermi/GBM rsp2 file format
# make the rsp file proper
rsp_file = sanitize_filename(rsp2_file)
assert file_existing_and_readable(rsp_file), "OGIPResponse file %s not existing or not readable" % rsp_file
# Will fill up the list of matrices
list_of_matrices = []
# Read the response
with pyfits.open(rsp_file) as f:
n_responses = f['PRIMARY'].header['DRM_NUM']
# we will read all the matrices and save them
for rsp_number in range(1, n_responses + 1):
this_response = OGIPResponse(rsp2_file + '{%i}' % rsp_number)
list_of_matrices.append(this_response)
if half_shifted:
# Now the GBM format has a strange feature: the matrix, instead of covering from TSTART to TSTOP, covers
# from (TSTART + TSTOP) / 2.0 of the previous matrix to the (TSTART + TSTOP) / 2.0 of itself.
# So let's adjust the coverage intervals accordingly
if len(list_of_matrices) > 1:
for i, this_matrix in enumerate(list_of_matrices):
if i == 0:
# The first matrix covers from its TSTART to its half time
this_matrix._coverage_interval = TimeInterval(this_matrix.coverage_interval.start_time,
this_matrix.coverage_interval.half_time)
else:
# Any other matrix covers from the half time of the previous matrix to its half time
# However, the previous matrix has been already processed, so we use its stop time which
# has already begun the half time of what it was before processing
prev_matrix = list_of_matrices[i-1]
this_matrix._coverage_interval = TimeInterval(prev_matrix.coverage_interval.stop_time,
this_matrix.coverage_interval.half_time)
return InstrumentResponseSet(list_of_matrices, exposure_getter, counts_getter, reference_time)
def _read_arf_file(self, arf_file):
"""
read an arf file and apply it to the current_matrix
:param arf_file:
:param current_matrix:
:param current_mc_channels:
:return:
"""
arf_file = sanitize_filename(arf_file)
self._arf_file = arf_file
assert file_existing_and_readable(arf_file.split("{")[0]), "Ancillary file %s not existing or not " \
"readable" % arf_file
with pyfits.open(arf_file) as f:
data = f['SPECRESP'].data
arf = data.field('SPECRESP')
# Check that arf and rmf have same dimensions
if arf.shape[0] != self.matrix.shape[1]:
raise IOError("The ARF and the RMF file does not have the same number of channels")
# Check that the ENERG_LO and ENERG_HI for the RMF and the ARF
# are the same
energ_lo = data.field("ENERG_LO")
energ_hi = data.field("ENERG_HI")
assert self._are_contiguous(energ_lo, energ_hi), "Monte carlo energies in ARF are not contiguous!"
arf_mc_channels = np.append(energ_lo, [energ_hi[-1]])
# Declare the mc channels different if they differ by more than 1%
idx = (self.monte_carlo_energies > 0)
diff = (self.monte_carlo_energies[idx] - arf_mc_channels[idx]) / self.monte_carlo_energies[idx]
if diff.max() > 0.01:
raise IOError("The ARF and the RMF have one or more MC channels which differ by more than 1%")
# Multiply ARF and RMF
matrix = self.matrix * arf
# Override the matrix with the one multiplied by the arf
self.replace_matrix(matrix)
def download(
self,
remote_filename,
destination_path,
new_filename=None,
progress=True,
compress=False,
):
assert remote_filename in self.files, (
"File %s is not contained in this directory (%s)" %
(remote_filename, self._request_result.url))
destination_path = sanitize_filename(destination_path, abspath=True)
assert path_exists_and_is_directory(destination_path), (
"Provided destination does not exist or "
"is not a directory" % destination_path)
# If no filename is specified, use the same name that the file has on the remote server
if new_filename is None:
new_filename = remote_filename.split("/")[-1]
# Get the fully qualified path for the remote and the local file
remote_path = self._request_result.url + remote_filename
local_path = os.path.join(destination_path, new_filename)
# Ask the server for the file, but do not download it just yet
# (stream=True will get the HTTP header but nothing else)
# Use stream=True for two reasons:
# * so that the file is not downloaded all in memory before being written to the disk
# * so that we can report progress is requested
this_request = requests.get(remote_path, stream=True)
# Figure out the size of the file
file_size = int(this_request.headers["Content-Length"])
# Now check if we really need to download this file
if compress:
# Add a .gz at the end of the file path
local_path += ".gz"
if file_existing_and_readable(local_path):
local_size = os.path.getsize(local_path)
if local_size == file_size or compress:
# if the compressed file already exists
# it will have a smaller size
# No need to download it again
return local_path
# Chunk size shouldn't bee too small otherwise we are causing a bottleneck in the download speed
chunk_size = 1024 * 10
# If the user wants to compress the file, use gzip, otherwise the normal opener
if compress:
import gzip
opener = gzip.open
else:
opener = open
if progress:
# Set a title for the progress bar
bar_title = "Downloading %s" % new_filename
with progress_bar(file_size,
scale=1024 * 1024,
units="Mb",
title=bar_title) as bar: # type: ProgressBarBase
with opener(local_path, "wb") as f:
for chunk in this_request.iter_content(
chunk_size=chunk_size):
if chunk: # filter out keep-alive new chunks
f.write(chunk)
bar.increase(len(chunk))
this_request.close()
else:
with opener(local_path, "wb") as f:
for chunk in this_request.iter_content(chunk_size=chunk_size):
if chunk: # filter out keep-alive new chunks
f.write(chunk)
this_request.close()
return local_path
def add_svo_filter_to_speclite(observatory, instrument, ffilter, update=False):
"""
download an SVO filter file and then add it to the user library
:param observatory:
:param instrument:
:param ffilter:
:return:
"""
# make a directory for this observatory and instrument
filter_path = os.path.join(get_speclite_filter_path(), to_valid_python_name(observatory))
if_directory_not_existing_then_make(filter_path)
# grab the filter file from SVO
# reconvert 2MASS so we can grab it
if observatory == 'TwoMASS':
observatory = '2MASS'
if not file_existing_and_readable(os.path.join(filter_path,
"%s-%s.ecsv"%(to_valid_python_name(instrument),
to_valid_python_name(ffilter)))) or update:
url_response = urllib2.urlopen(
'http://svo2.cab.inta-csic.es/svo/theory/fps/fps.php?PhotCalID=%s/%s.%s/AB' % (observatory,
instrument,
ffilter))
# now parse it
data = votable.parse_single_table(url_response).to_table()
# save the waveunit
waveunit = data['Wavelength'].unit
# the filter files are masked arrays, which do not go to zero on
# the boundaries. This confuses speclite and will throw an error.
# so we add a zero on the boundaries
if data['Transmission'][0] != 0.:
w1 = data['Wavelength'][0] * .9
data.insert_row(0, [w1, 0])
if data['Transmission'][-1] != 0.:
w2 = data['Wavelength'][-1]* 1.1
data.add_row([w2, 0])
# filter any negative values
idx = data['Transmission'] < 0
data['Transmission'][idx] = 0
# build the transmission. # we will force all the wavelengths
# to Angstroms because sometimes AA is misunderstood
try:
transmission = spec_filter.FilterResponse(
wavelength=data['Wavelength'] * waveunit.to('Angstrom') * u.Angstrom,
response=data['Transmission'],
meta=dict(group_name=to_valid_python_name(instrument),
band_name=to_valid_python_name(ffilter)))
# save the filter
transmission.save(filter_path)
success = True
except(ValueError):
success = False
print('%s:%s:%s has an invalid wave table, SKIPPING'% (observatory, instrument, ffilter))
return success
else:
return True
def __init__(self,
name,
time_series,
response=None,
poly_order=-1,
unbinned=True,
verbose=True,
restore_poly_fit=None,
container_type=BinnedSpectrumWithDispersion):
"""
Class for handling generic time series data including binned and event list
series. Depending on the data, this class builds either a SpectrumLike or
DisperisonSpectrumLike plugin
For specific instruments, use the TimeSeries.from() classmethods
:param name: name for the plugin
:param time_series: a TimeSeries instance
:param response: options InstrumentResponse instance
:param poly_order: the polynomial order to use for background fitting
:param unbinned: if the background should be fit unbinned
:param verbose: the verbosity switch
:param restore_poly_fit: file from which to read a prefitted background
"""
assert isinstance(time_series,
TimeSeries), "must be a TimeSeries instance"
assert issubclass(container_type,
Histogram), 'must be a subclass of Histogram'
self._name = name
self._container_type = container_type
self._time_series = time_series # type: TimeSeries
# make sure we have a proper response
if response is not None:
assert isinstance(response, InstrumentResponse) or isinstance(
response, InstrumentResponseSet) or isinstance(
response,
str), 'Response must be an instance of InstrumentResponse'
# deal with RSP weighting if need be
if isinstance(response, InstrumentResponseSet):
# we have a weighted response
self._rsp_is_weighted = True
self._weighted_rsp = response
# just get a dummy response for the moment
# it will be corrected when we set the interval
self._response = InstrumentResponse.create_dummy_response(
response.ebounds, response.monte_carlo_energies)
else:
self._rsp_is_weighted = False
self._weighted_rsp = None
self._response = response
self._verbose = verbose
self._active_interval = None
self._observed_spectrum = None
self._background_spectrum = None
self._measured_background_spectrum = None
self._time_series.poly_order = poly_order
self._default_unbinned = unbinned
# try and restore the poly fit if requested
if restore_poly_fit is not None:
if file_existing_and_readable(restore_poly_fit):
self._time_series.restore_fit(restore_poly_fit)
if verbose:
print('Successfully restored fit from %s' %
restore_poly_fit)
else:
custom_warnings.warn("Could not find saved background %s." %
restore_poly_fit)
def download(self, remote_filename, destination_path, new_filename=None, progress=True, compress=False):
assert remote_filename in self.files, "File %s is not contained in this directory (%s)" % (remote_filename,
self._request_result.url)
destination_path = sanitize_filename(destination_path, abspath=True)
assert path_exists_and_is_directory(destination_path), "Provided destination does not exist or " \
"is not a directory" % destination_path
# If no filename is specified, use the same name that the file has on the remote server
if new_filename is None:
new_filename = remote_filename.split("/")[-1]
# Get the fully qualified path for the remote and the local file
remote_path = self._request_result.url + remote_filename
local_path = os.path.join(destination_path, new_filename)
# Ask the server for the file, but do not download it just yet
# (stream=True will get the HTTP header but nothing else)
# Use stream=True for two reasons:
# * so that the file is not downloaded all in memory before being written to the disk
# * so that we can report progress is requested
this_request = requests.get(remote_path, stream=True)
# Figure out the size of the file
file_size = int(this_request.headers['Content-Length'])
# Now check if we really need to download this file
if compress:
# Add a .gz at the end of the file path
local_path += '.gz'
if file_existing_and_readable(local_path):
local_size = os.path.getsize(local_path)
if local_size == file_size or compress:
# if the compressed file already exists
# it will have a smaller size
# No need to download it again
return local_path
# Chunk size shouldn't bee too small otherwise we are causing a bottleneck in the download speed
chunk_size = 1024 * 10
# If the user wants to compress the file, use gzip, otherwise the normal opener
if compress:
import gzip
opener = gzip.open
else:
opener = open
if progress:
# Set a title for the progress bar
bar_title = "Downloading %s" % new_filename
with progress_bar(file_size, scale=1024 * 1024, units='Mb',
title=bar_title) as bar: # type: ProgressBarBase
with opener(local_path, 'wb') as f:
for chunk in this_request.iter_content(chunk_size=chunk_size):
if chunk: # filter out keep-alive new chunks
f.write(chunk)
bar.increase(len(chunk))
this_request.close()
else:
with opener(local_path, 'wb') as f:
for chunk in this_request.iter_content(chunk_size=chunk_size):
if chunk: # filter out keep-alive new chunks
f.write(chunk)
this_request.close()
return local_path
def get_heasarc_table_as_pandas(heasarc_table_name, update=False, cache_time_days=1):
"""
Obtain a a VO table from the HEASARC archives and return it as a pandas table indexed
by object/trigger names. The heasarc_table_name values are the ones referenced at:
https://heasarc.gsfc.nasa.gov/docs/archive/vo/
In order to speed up the processing of the tables, 3ML can cache the XML table in a cache
that is updated every cache_time_days. The cache can be forced to update, i.e, reload from
the web, by setting update to True.
:param heasarc_table_name: the name of a HEASARC browse table
:param update: force web read of the table and update cache
:param cache_time_days: number of days to hold the current cache
:return: pandas DataFrame with results and astropy table
"""
# make sure the table is a string
assert type(heasarc_table_name) is str
# point to the cache directory and create it if it is not existing
cache_directory = os.path.join(os.path.expanduser('~'), '.threeML', '.cache')
if_directory_not_existing_then_make(cache_directory)
cache_file = os.path.join(cache_directory, '%s_cache.yml' % heasarc_table_name)
cache_file_sanatized = sanitize_filename(cache_file)
# build and sanitize the votable XML file that will be saved
file_name = os.path.join(cache_directory, '%s_votable.xml' % heasarc_table_name)
file_name_sanatized = sanitize_filename(file_name)
if not file_existing_and_readable(cache_file_sanatized):
print("The cache for %s does not yet exist. We will try to build it\n" % heasarc_table_name)
write_cache = True
cache_exists = False
else:
with open(cache_file_sanatized) as cache:
# the cache file is two lines. The first is a datetime string that
# specifies the last time the XML file was obtained
yaml_cache = yaml.safe_load(cache)
cached_time = astro_time.Time(datetime.datetime(*map(int, yaml_cache['last save'].split('-'))))
# the second line how many seconds to keep the file around
cache_valid_for = float(yaml_cache['cache time'])
# now we will compare it to the current time in UTC
current_time = astro_time.Time(datetime.datetime.utcnow(), scale='utc')
delta_time = current_time - cached_time
if delta_time.sec >= cache_valid_for:
# ok, this is an old file, we will update it
write_cache = True
cache_exists = True
else:
# we
write_cache = False
cache_exists = True
if write_cache or update:
print("Building cache for %s.\n" % heasarc_table_name)
# go to HEASARC and get the requested table
heasarc_url = 'http://heasarc.gsfc.nasa.gov/cgi-bin/W3Browse/getvotable.pl?name=%s' % heasarc_table_name
try:
urllib.urlretrieve(heasarc_url, filename=file_name_sanatized)
except(IOError):
warnings.warn('The cache is outdated but the internet cannot be reached. Please check your connection')
else:
# Make sure the lines are interpreted as Unicode (otherwise some characters will fail)
with open(file_name_sanatized) as table_file:
new_lines = map(lambda x: x.decode("utf-8", errors="ignore"), table_file.readlines())
# now write the decoded lines back to the file
with codecs.open(file_name_sanatized, "w+", "utf-8") as table_file:
table_file.write("".join(new_lines))
# save the time that we go this table
with open(cache_file_sanatized, 'w') as cache:
yaml_dict = {}
current_time = astro_time.Time(datetime.datetime.utcnow(), scale='utc')
yaml_dict['last save'] = current_time.datetime.strftime('%Y-%m-%d-%H-%M-%S')
seconds_in_day = 86400.
yaml_dict['cache time'] = seconds_in_day * cache_time_days
yaml.dump(yaml_dict, stream=cache, default_flow_style=False)
# use astropy routines to read the votable
with warnings.catch_warnings():
warnings.simplefilter("ignore")
vo_table = votable.parse(file_name_sanatized)
table = vo_table.get_first_table().to_table(use_names_over_ids=True)
# create a pandas table indexed by name
pandas_df = table.to_pandas().set_index('name')
del vo_table
return pandas_df
def download(
self,
remote_filename,
destination_path: str,
new_filename=None,
progress=True,
compress=False,
):
assert (remote_filename in self.files
), "File %s is not contained in this directory (%s)" % (
remote_filename,
self._request_result.url,
)
destination_path: Path = sanitize_filename(destination_path,
abspath=True)
assert path_exists_and_is_directory(destination_path), (
f"Provided destination {destination_path} does not exist or "
"is not a directory")
# If no filename is specified, use the same name that the file has on the remote server
if new_filename is None:
new_filename: str = remote_filename.split("/")[-1]
# Get the fully qualified path for the remote and the local file
remote_path: str = self._request_result.url + remote_filename
local_path: Path = destination_path / new_filename
# Ask the server for the file, but do not download it just yet
# (stream=True will get the HTTP header but nothing else)
# Use stream=True for two reasons:
# * so that the file is not downloaded all in memory before being written to the disk
# * so that we can report progress is requested
this_request = requests.get(remote_path, stream=True)
# Figure out the size of the file
file_size = int(this_request.headers["Content-Length"])
log.debug(f"downloading {remote_filename} of size {file_size}")
# Now check if we really need to download this file
if compress:
# Add a .gz at the end of the file path
log.debug(
f"file {remote_filename} will be downloaded and compressed")
local_path: Path = Path(f"{local_path}.gz")
if file_existing_and_readable(local_path):
local_size = os.path.getsize(local_path)
if local_size == file_size or compress:
# if the compressed file already exists
# it will have a smaller size
# No need to download it again
log.info(f"file {remote_filename} is already downloaded!")
return local_path
if local_path.is_file():
first_byte = os.path.getsize(local_path)
else:
first_byte = 0
# Chunk size shouldn't bee too small otherwise we are causing a bottleneck in the download speed
chunk_size = 1024 * 10
# If the user wants to compress the file, use gzip, otherwise the normal opener
if compress:
import gzip
opener = gzip.open
else:
opener = open
if threeML_config["interface"]["progress_bars"]:
# Set a title for the progress bar
bar_title = "Downloading %s" % new_filename
total_size = int(this_request.headers.get('content-length', 0))
bar = tqdm(
initial=first_byte,
unit_scale=True,
unit_divisor=1024,
unit="B",
total=int(this_request.headers["Content-Length"]),
desc=bar_title,
)
with opener(local_path, "wb") as f:
for chunk in this_request.iter_content(chunk_size=chunk_size):
if chunk: # filter out keep-alive new chunks
f.write(chunk)
bar.update(len(chunk))
this_request.close()
bar.close()
else:
with opener(local_path, "wb") as f:
for chunk in this_request.iter_content(chunk_size=chunk_size):
if chunk: # filter out keep-alive new chunks
f.write(chunk)
this_request.close()
return local_path
def from_root_file(cls, map_tree_file, roi):
"""
Create a MapTree object from a ROOT file and a ROI. Do not use this directly, use map_tree_factory instead.
:param map_tree_file:
:param roi:
:return:
"""
map_tree_file = sanitize_filename(map_tree_file)
# Check that they exists and can be read
if not file_existing_and_readable(map_tree_file):
raise IOError("MapTree %s does not exist or is not readable" %
map_tree_file)
# Make sure we have a proper ROI (or None)
assert isinstance(roi, HealpixROIBase) or roi is None, "You have to provide an ROI choosing from the " \
"available ROIs in the region_of_interest module"
if roi is None:
custom_warnings.warn(
"You have set roi=None, so you are reading the entire sky")
# Read map tree
with open_ROOT_file(map_tree_file) as f:
data_bins_labels = list(
root_numpy.tree2array(f.Get("BinInfo"), "name"))
# A transit is defined as 1 day, and totalDuration is in hours
# Get the number of transit from bin 0 (as LiFF does)
n_transits = root_numpy.tree2array(f.Get("BinInfo"),
"totalDuration") / 24.0
n_bins = len(data_bins_labels)
# These are going to be Healpix maps, one for each data analysis bin_name
data_analysis_bins = []
for i in range(n_bins):
name = data_bins_labels[i]
bin_label = "nHit0%s/%s" % (name, "data")
bkg_label = "nHit0%s/%s" % (name, "bkg")
# Get ordering scheme
nside = f.Get(bin_label).GetUserInfo().FindObject(
"Nside").GetVal()
nside_bkg = f.Get(bkg_label).GetUserInfo().FindObject(
"Nside").GetVal()
assert nside == nside_bkg
scheme = f.Get(bin_label).GetUserInfo().FindObject(
"Scheme").GetVal()
scheme_bkg = f.Get(bkg_label).GetUserInfo().FindObject(
"Scheme").GetVal()
assert scheme == scheme_bkg
assert scheme == 0, "NESTED scheme is not supported yet"
if roi is not None:
# Only read the elements in the ROI
active_pixels = roi.active_pixels(nside,
system='equatorial',
ordering='RING')
counts = cls._read_partial_tree(nside, f.Get(bin_label),
active_pixels)
bkg = cls._read_partial_tree(nside, f.Get(bkg_label),
active_pixels)
this_data_analysis_bin = DataAnalysisBin(
name,
SparseHealpix(counts, active_pixels, nside),
SparseHealpix(bkg, active_pixels, nside),
active_pixels_ids=active_pixels,
n_transits=n_transits[i],
scheme='RING')
else:
# Read the entire sky.
counts = tree_to_ndarray(f.Get(bin_label),
"count").astype(np.float64)
bkg = tree_to_ndarray(f.Get(bkg_label),
"count").astype(np.float64)
this_data_analysis_bin = DataAnalysisBin(
name,
DenseHealpix(counts),
DenseHealpix(bkg),
active_pixels_ids=None,
n_transits=n_transits[i],
scheme='RING')
data_analysis_bins.append(this_data_analysis_bin)
return cls(data_bins_labels, data_analysis_bins, roi)
def __init__(self, response_file_name):
# Make sure file is readable
response_file_name = sanitize_filename(response_file_name)
# Check that they exists and can be read
if not file_existing_and_readable(response_file_name):
raise IOError("Response %s does not exist or is not readable" % response_file_name)
self._response_file_name = response_file_name
# Read response
with open_ROOT_file(response_file_name) as f:
# Get the name of the trees
object_names = get_list_of_keys(f)
# Make sure we have all the things we need
assert 'LogLogSpectrum' in object_names
assert 'DecBins' in object_names
assert 'AnalysisBins' in object_names
# Read spectrum used during the simulation
self._log_log_spectrum = TF1Wrapper(f.Get("LogLogSpectrum"))
# Get the analysis bins definition
dec_bins = tree_to_ndarray(f.Get("DecBins"))
dec_bins_lower_edge = dec_bins['lowerEdge'] # type: np.ndarray
dec_bins_upper_edge = dec_bins['upperEdge'] # type: np.ndarray
dec_bins_center = dec_bins['simdec'] # type: np.ndarray
self._dec_bins = zip(dec_bins_lower_edge, dec_bins_center, dec_bins_upper_edge)
# Read in the ids of the response bins ("analysis bins" in LiFF jargon)
response_bins_ids = tree_to_ndarray(f.Get("AnalysisBins"), "id") # type: np.ndarray
# Now we create a list of ResponseBin instances for each dec bin_name
self._response_bins = collections.OrderedDict()
for dec_id in range(len(self._dec_bins)):
this_response_bins = []
min_dec, dec_center, max_dec = self._dec_bins[dec_id]
for response_bin_id in response_bins_ids:
this_response_bin = ResponseBin(f, dec_id, response_bin_id, self._log_log_spectrum,
min_dec, dec_center, max_dec)
this_response_bins.append(this_response_bin)
self._response_bins[self._dec_bins[dec_id][1]] = this_response_bins
del f
def __init__(self, name, time_series, response=None,
poly_order=-1, unbinned=True, verbose=True, restore_poly_fit=None, container_type=BinnedSpectrumWithDispersion):
"""
Class for handling generic time series data including binned and event list
series. Depending on the data, this class builds either a SpectrumLike or
DisperisonSpectrumLike plugin
For specific instruments, use the TimeSeries.from() classmethods
:param name: name for the plugin
:param time_series: a TimeSeries instance
:param response: options InstrumentResponse instance
:param poly_order: the polynomial order to use for background fitting
:param unbinned: if the background should be fit unbinned
:param verbose: the verbosity switch
:param restore_poly_fit: file from which to read a prefitted background
"""
assert isinstance(time_series, TimeSeries), "must be a TimeSeries instance"
assert issubclass(container_type,Histogram), 'must be a subclass of Histogram'
self._name = name
self._container_type = container_type
self._time_series = time_series # type: TimeSeries
# make sure we have a proper response
if response is not None:
assert isinstance(response, InstrumentResponse) or isinstance(response,
InstrumentResponseSet) or isinstance(response, str), 'Response must be an instance of InstrumentResponse'
# deal with RSP weighting if need be
if isinstance(response, InstrumentResponseSet):
# we have a weighted response
self._rsp_is_weighted = True
self._weighted_rsp = response
# just get a dummy response for the moment
# it will be corrected when we set the interval
self._response = InstrumentResponse.create_dummy_response(response.ebounds,
response.monte_carlo_energies)
else:
self._rsp_is_weighted = False
self._weighted_rsp = None
self._response = response
self._verbose = verbose
self._active_interval = None
self._observed_spectrum = None
self._background_spectrum = None
self._measured_background_spectrum = None
self._time_series.poly_order = poly_order
self._default_unbinned = unbinned
# try and restore the poly fit if requested
if restore_poly_fit is not None:
if file_existing_and_readable(restore_poly_fit):
self._time_series.restore_fit(restore_poly_fit)
if verbose:
print('Successfully restored fit from %s'%restore_poly_fit)
else:
custom_warnings.warn(
"Could not find saved background %s." % restore_poly_fit)
def get_heasarc_table_as_pandas(heasarc_table_name, update=False, cache_time_days=1):
"""
Obtain a a VO table from the HEASARC archives and return it as a pandas table indexed
by object/trigger names. The heasarc_table_name values are the ones referenced at:
https://heasarc.gsfc.nasa.gov/docs/archive/vo/
In order to speed up the processing of the tables, 3ML can cache the XML table in a cache
that is updated every cache_time_days. The cache can be forced to update, i.e, reload from
the web, by setting update to True.
:param heasarc_table_name: the name of a HEASARC browse table
:param update: force web read of the table and update cache
:param cache_time_days: number of days to hold the current cache
:return: pandas DataFrame with results and astropy table
"""
# make sure the table is a string
assert type(heasarc_table_name) is str
# point to the cache directory and create it if it is not existing
cache_directory = os.path.join(os.path.expanduser("~"), ".threeML", ".cache")
if_directory_not_existing_then_make(cache_directory)
cache_file = os.path.join(cache_directory, "%s_cache.yml" % heasarc_table_name)
cache_file_sanatized = sanitize_filename(cache_file)
# build and sanitize the votable XML file that will be saved
file_name = os.path.join(cache_directory, "%s_votable.xml" % heasarc_table_name)
file_name_sanatized = sanitize_filename(file_name)
if not file_existing_and_readable(cache_file_sanatized):
print(
"The cache for %s does not yet exist. We will try to build it\n"
% heasarc_table_name
)
write_cache = True
cache_exists = False
else:
with open(cache_file_sanatized) as cache:
# the cache file is two lines. The first is a datetime string that
# specifies the last time the XML file was obtained
yaml_cache = yaml.load(cache, Loader=yaml.SafeLoader)
cached_time = astro_time.Time(
datetime.datetime(*list(map(int, yaml_cache["last save"].split("-"))))
)
# the second line how many seconds to keep the file around
cache_valid_for = float(yaml_cache["cache time"])
# now we will compare it to the current time in UTC
current_time = astro_time.Time(datetime.datetime.utcnow(), scale="utc")
delta_time = current_time - cached_time
if delta_time.sec >= cache_valid_for:
# ok, this is an old file, we will update it
write_cache = True
cache_exists = True
else:
# we
write_cache = False
cache_exists = True
if write_cache or update:
print("Building cache for %s.\n" % heasarc_table_name)
# go to HEASARC and get the requested table
heasarc_url = (
"http://heasarc.gsfc.nasa.gov/cgi-bin/W3Browse/getvotable.pl?name=%s"
% heasarc_table_name
)
try:
urllib.request.urlretrieve(heasarc_url, filename=file_name_sanatized)
except (IOError):
warnings.warn(
"The cache is outdated but the internet cannot be reached. Please check your connection"
)
else:
# # Make sure the lines are interpreted as Unicode (otherwise some characters will fail)
with open(file_name_sanatized) as table_file:
# might have to add this in for back compt J MICHAEL
# new_lines = [x. for x in table_file.readlines()]
new_lines = table_file.readlines()
# now write the decoded lines back to the file
with codecs.open(file_name_sanatized, "w+", "utf-8") as table_file:
table_file.write("".join(new_lines))
# save the time that we go this table
with open(cache_file_sanatized, "w") as cache:
yaml_dict = {}
current_time = astro_time.Time(datetime.datetime.utcnow(), scale="utc")
yaml_dict["last save"] = current_time.datetime.strftime(
"%Y-%m-%d-%H-%M-%S"
)
seconds_in_day = 86400.0
yaml_dict["cache time"] = seconds_in_day * cache_time_days
yaml.dump(yaml_dict, stream=cache, default_flow_style=False)
# use astropy routines to read the votable
with warnings.catch_warnings():
warnings.simplefilter("ignore")
vo_table = votable.parse(file_name_sanatized)
table = vo_table.get_first_table().to_table(use_names_over_ids=True)
# make sure we do not use this as byte code
table.convert_bytestring_to_unicode()
# create a pandas table indexed by name
pandas_df = table.to_pandas().set_index("name")
del vo_table
return pandas_df
def __init__(self, rsp_file, arf_file=None):
"""
:param rsp_file:
:param arf_file:
"""
# Now make sure that the response file exist
rsp_file = sanitize_filename(rsp_file)
assert file_existing_and_readable(rsp_file.split("{")[0]), "OGIPResponse file %s not existing or not " \
"readable" % rsp_file
# Check if we are dealing with a .rsp2 file (containing more than
# one response). This is checked by looking for the syntax
# [responseFile]{[responseNumber]}
if '{' in rsp_file:
tokens = rsp_file.split("{")
rsp_file = tokens[0]
rsp_number = int(tokens[-1].split('}')[0].replace(" ", ""))
else:
rsp_number = 1
self._rsp_file = rsp_file
# Read the response
with pyfits.open(rsp_file) as f:
try:
# This is usually when the response file contains only the energy dispersion
data = f['MATRIX', rsp_number].data
header = f['MATRIX', rsp_number].header
if arf_file is None:
warnings.warn("The response is in an extension called MATRIX, which usually means you also "
"need an ancillary file (ARF) which you didn't provide. You should refer to the "
"documentation of the instrument and make sure you don't need an ARF.")
except Exception as e:
warnings.warn("The default choice for MATRIX extension failed:"+repr(e)+\
"available: "+" ".join([repr(e.header.get('EXTNAME')) for e in f]))
# Other detectors might use the SPECRESP MATRIX name instead, usually when the response has been
# already convoluted with the effective area
# Note that here we are not catching any exception, because
# we have to fail if we cannot read the matrix
data = f['SPECRESP MATRIX', rsp_number].data
header = f['SPECRESP MATRIX', rsp_number].header
# These 3 operations must be executed when the file is still open
matrix = self._read_matrix(data, header)
ebounds = self._read_ebounds(f['EBOUNDS'])
mc_channels = self._read_mc_channels(data)
# Now, if there is information on the coverage interval, let's use it
header_start = header.get("TSTART", None)
header_stop = header.get("TSTOP", None)
if header_start is not None and header_stop is not None:
super(OGIPResponse, self).__init__(matrix=matrix,
ebounds=ebounds,
monte_carlo_energies=mc_channels,
coverage_interval=TimeInterval(header_start, header_stop))
else:
super(OGIPResponse, self).__init__(matrix=matrix,
ebounds=ebounds,
monte_carlo_energies=mc_channels)
# Read the ARF if there is any
# NOTE: this has to happen *after* calling the parent constructor
if arf_file is not None and arf_file.lower() != 'none':
self._read_arf_file(arf_file)
else:
self._arf_file = None
def check_if_fit_exists(self, destination='.', save_info=''):
file_name = "%s/%s_%s_%s.fits" % (destination, self._band, self._snid,
save_info)
return file_existing_and_readable(file_name)
def __init__(self, name, maptree, response, n_transits=None, fullsky=False):
# This controls if the likeHAWC class should load the entire
# map or just a small disc around a source (faster).
# Default is the latter, which is way faster. LIFF will decide
# autonomously which ROI to use depending on the source model
self._fullsky = bool(fullsky)
# Sanitize files in input (expand variables and so on)
self._maptree = os.path.abspath(sanitize_filename(maptree))
self._response = os.path.abspath(sanitize_filename(response))
# Check that they exists and can be read
if not file_existing_and_readable(self._maptree):
raise IOError("MapTree %s does not exist or is not readable" % maptree)
if not file_existing_and_readable(self._response):
raise IOError("Response %s does not exist or is not readable" % response)
# Post-pone the creation of the LIFF instance to when
# we have the likelihood model
self._instanced = False
# Number of transits
if n_transits is not None:
self._n_transits = float(n_transits)
else:
self._n_transits = None
# Default list of bins
self._bin_list = self._min_and_max_to_list(defaultMinChannel, defaultMaxChannel)
# By default the fit of the CommonNorm is deactivated
# NOTE: this flag sets the internal common norm minimization of LiFF, not
# the common norm as nuisance parameter (which is controlled by activate_CommonNorm() and
# deactivate_CommonNorm()
self._fit_commonNorm = False
# This is to keep track of whether the user defined a ROI or not
self._roi_ra = None
self._roi_fits = None
self._roi_galactic = False
# Create the dictionary of nuisance parameters
self._nuisance_parameters = collections.OrderedDict()
param_name = "%s_ComNorm" % name
self._nuisance_parameters[param_name] = Parameter(
param_name, 1.0, min_value=0.5, max_value=1.5, delta=0.01
)
self._nuisance_parameters[param_name].fix = True
super(HAWCLike, self).__init__(name, self._nuisance_parameters)
def from_root_file(map_tree_file, roi):
"""
Create a MapTree object from a ROOT file and a ROI. Do not use this directly, use map_tree_factory instead.
:param map_tree_file:
:param roi:
:return:
"""
from ..root_handler import open_ROOT_file, root_numpy, tree_to_ndarray
map_tree_file = sanitize_filename(map_tree_file)
# Check that they exists and can be read
if not file_existing_and_readable(map_tree_file): # pragma: no cover
raise IOError("MapTree %s does not exist or is not readable" % map_tree_file)
# Make sure we have a proper ROI (or None)
assert isinstance(roi, HealpixROIBase) or roi is None, "You have to provide an ROI choosing from the " \
"available ROIs in the region_of_interest module"
if roi is None:
custom_warnings.warn("You have set roi=None, so you are reading the entire sky")
# Read map tree
with open_ROOT_file(map_tree_file) as f:
data_bins_labels = list(root_numpy.tree2array(f.Get("BinInfo"), "name"))
# A transit is defined as 1 day, and totalDuration is in hours
# Get the number of transit from bin 0 (as LiFF does)
n_transits = root_numpy.tree2array(f.Get("BinInfo"), "totalDuration") / 24.0
# The map-maker underestimate the livetime of bins with low statistic by removing time intervals with
# zero events. Therefore, the best estimate of the livetime is the maximum of n_transits, which normally
# happen in the bins with high statistic
n_transits = max(n_transits)
n_bins = len(data_bins_labels)
# These are going to be Healpix maps, one for each data analysis bin_name
data_analysis_bins = collections.OrderedDict()
for i in range(n_bins):
name = data_bins_labels[i]
data_tobject = _get_bin_object(f, name, "data")
bkg_tobject = _get_bin_object(f, name, "bkg")
# Get ordering scheme
nside = data_tobject.GetUserInfo().FindObject("Nside").GetVal()
nside_bkg = bkg_tobject.GetUserInfo().FindObject("Nside").GetVal()
assert nside == nside_bkg
scheme = data_tobject.GetUserInfo().FindObject("Scheme").GetVal()
scheme_bkg = bkg_tobject.GetUserInfo().FindObject("Scheme").GetVal()
assert scheme == scheme_bkg
assert scheme == 0, "NESTED scheme is not supported yet"
if roi is not None:
# Only read the elements in the ROI
active_pixels = roi.active_pixels(nside, system='equatorial', ordering='RING')
counts = _read_partial_tree(data_tobject, active_pixels)
bkg = _read_partial_tree(bkg_tobject, active_pixels)
counts_hpx = SparseHealpix(counts, active_pixels, nside)
bkg_hpx = SparseHealpix(bkg, active_pixels, nside)
this_data_analysis_bin = DataAnalysisBin(name,
counts_hpx,
bkg_hpx,
active_pixels_ids=active_pixels,
n_transits=n_transits,
scheme='RING')
else:
# Read the entire sky.
counts = tree_to_ndarray(data_tobject, "count").astype(np.float64)
bkg = tree_to_ndarray(bkg_tobject, "count").astype(np.float64)
this_data_analysis_bin = DataAnalysisBin(name,
DenseHealpix(counts),
DenseHealpix(bkg),
active_pixels_ids=None,
n_transits=n_transits,
scheme='RING')
data_analysis_bins[name] = this_data_analysis_bin
return data_analysis_bins
def __init__(self, name, phafile, bkgfile, rspfile, arffile=None):
self.name = name
# Check that all file exists
notExistant = []
inputFiles = [phafile, bkgfile, rspfile]
for i in range(3):
# The file could contain a {#} specification, like spectrum.pha{3},
# which indicate the 3rd spectrum in the spectrum.pha file
inputFiles[i] = file_utils.sanitize_filename(inputFiles[i].split("{")[0])
if not file_utils.file_existing_and_readable(inputFiles[i]):
raise IOError("File %s does not exist or is not readable" % (inputFiles[i]))
phafile, bkgfile, rspfile = inputFiles
# Check the arf, if provided
if arffile is not None:
arffile = file_utils.sanitize_filename(arffile.split("{")[0])
if not file_utils.file_existing_and_readable(arffile):
raise IOError("File %s does not exist or is not readable" % (arffile))
self.phafile = OGIPPHA(phafile, filetype="observed")
self.exposure = self.phafile.getExposure()
self.bkgfile = OGIPPHA(bkgfile, filetype="background")
self.response = Response(rspfile, arffile)
# Start with an empty mask (the user will overwrite it using the
# setActiveMeasurement method)
self.mask = numpy.asarray(numpy.ones(self.phafile.getRates().shape), numpy.bool)
# Get the counts for this spectrum
self.counts = self.phafile.getRates()[self.mask] * self.exposure
# Check that counts is positive
idx = self.counts < 0
if numpy.sum(idx) > 0:
warnings.warn(
"The observed spectrum for %s " % self.name + "has negative channels! Fixing those to zero.",
RuntimeWarning,
)
self.counts[idx] = 0
pass
# Get the background counts for this spectrum
self.bkgCounts = self.bkgfile.getRates()[self.mask] * self.exposure
# Check that bkgCounts is positive
idx = self.bkgCounts < 0
if numpy.sum(idx) > 0:
warnings.warn(
"The background spectrum for %s " % self.name + "has negative channels! Fixing those to zero.",
RuntimeWarning,
)
self.bkgCounts[idx] = 0
# Check that the observed counts are positive
idx = self.counts < 0
if numpy.sum(idx) > 0:
raise RuntimeError("Negative counts in observed spectrum %s. Data are corrupted." % (phafile))
# Keep a copy which will never be modified
self.counts_backup = numpy.array(self.counts, copy=True)
self.bkgCounts_backup = numpy.array(self.bkgCounts, copy=True)
# Effective area correction is disabled by default, i.e.,
# the nuisance parameter is fixed to 1
self.nuisanceParameters = {}
self.nuisanceParameters["InterCalib"] = Parameter("InterCalib", 1, min_value=0.9, max_value=1.1, delta=0.01)
self.nuisanceParameters["InterCalib"].fix = True
def __init__(self, name, maptree, response, n_transits=None, fullsky=False):
# This controls if the likeHAWC class should load the entire
# map or just a small disc around a source (faster).
# Default is the latter, which is way faster. LIFF will decide
# autonomously which ROI to use depending on the source model
self._fullsky = bool(fullsky)
# Sanitize files in input (expand variables and so on)
self._maptree = os.path.abspath(sanitize_filename(maptree))
self._response = os.path.abspath(sanitize_filename(response))
# Check that they exists and can be read
if not file_existing_and_readable(self._maptree):
raise IOError("MapTree %s does not exist or is not readable" % maptree)
if not file_existing_and_readable(self._response):
raise IOError("Response %s does not exist or is not readable" % response)
# Post-pone the creation of the LIFF instance to when
# we have the likelihood model
self._instanced = False
# Number of transits
if n_transits is not None:
self._n_transits = float(n_transits)
else:
self._n_transits = None
# Default list of bins
self._bin_list = self._min_and_max_to_list(defaultMinChannel,
defaultMaxChannel)
# By default the fit of the CommonNorm is deactivated
# NOTE: this flag sets the internal common norm minimization of LiFF, not
# the common norm as nuisance parameter (which is controlled by activate_CommonNorm() and
# deactivate_CommonNorm()
self._fit_commonNorm = False
# This is to keep track of whether the user defined a ROI or not
self._roi_ra = None
self._roi_fits = None
self._roi_galactic = False
# Create the dictionary of nuisance parameters
self._nuisance_parameters = collections.OrderedDict()
param_name = "%s_ComNorm" % name
self._nuisance_parameters[param_name] = Parameter(param_name, 1.0, min_value=0.5, max_value=1.5, delta=0.01)
self._nuisance_parameters[param_name].fix = True
super(HAWCLike, self).__init__(name, self._nuisance_parameters)
def add_svo_filter_to_speclite(observatory, instrument, ffilter, update=False):
"""
download an SVO filter file and then add it to the user library
:param observatory:
:param instrument:
:param ffilter:
:return:
"""
# make a directory for this observatory and instrument
filter_path = os.path.join(
get_speclite_filter_path(), to_valid_python_name(observatory)
)
if_directory_not_existing_then_make(filter_path)
# grab the filter file from SVO
# reconvert 2MASS so we can grab it
if observatory == "TwoMASS":
observatory = "2MASS"
if (
not file_existing_and_readable(
os.path.join(
filter_path,
"%s-%s.ecsv"
% (to_valid_python_name(instrument), to_valid_python_name(ffilter)),
)
)
or update
):
url_response = urllib.request.urlopen(
"http://svo2.cab.inta-csic.es/svo/theory/fps/fps.php?PhotCalID=%s/%s.%s/AB"
% (observatory, instrument, ffilter)
)
# now parse it
data = votable.parse_single_table(url_response).to_table()
# save the waveunit
waveunit = data["Wavelength"].unit
# the filter files are masked arrays, which do not go to zero on
# the boundaries. This confuses speclite and will throw an error.
# so we add a zero on the boundaries
if data["Transmission"][0] != 0.0:
w1 = data["Wavelength"][0] * 0.9
data.insert_row(0, [w1, 0])
if data["Transmission"][-1] != 0.0:
w2 = data["Wavelength"][-1] * 1.1
data.add_row([w2, 0])
# filter any negative values
idx = data["Transmission"] < 0
data["Transmission"][idx] = 0
# build the transmission. # we will force all the wavelengths
# to Angstroms because sometimes AA is misunderstood
try:
transmission = spec_filter.FilterResponse(
wavelength=data["Wavelength"] * waveunit.to("Angstrom") * u.Angstrom,
response=data["Transmission"],
meta=dict(
group_name=to_valid_python_name(instrument),
band_name=to_valid_python_name(ffilter),
),
)
# save the filter
transmission.save(filter_path)
success = True
except (ValueError):
success = False
print(
"%s:%s:%s has an invalid wave table, SKIPPING"
% (observatory, instrument, ffilter)
)
return success
else:
return True
def __init__(self, rsp_file, arf_file=None):
"""
:param rsp_file:
:param arf_file:
"""
# Now make sure that the response file exist
rsp_file = sanitize_filename(rsp_file)
assert file_existing_and_readable(rsp_file.split("{")[0]), "OGIPResponse file %s not existing or not " \
"readable" % rsp_file
# Check if we are dealing with a .rsp2 file (containing more than
# one response). This is checked by looking for the syntax
# [responseFile]{[responseNumber]}
if '{' in rsp_file:
tokens = rsp_file.split("{")
rsp_file = tokens[0]
rsp_number = int(tokens[-1].split('}')[0].replace(" ", ""))
else:
rsp_number = 1
self._rsp_file = rsp_file
# Read the response
with pyfits.open(rsp_file) as f:
try:
# This is usually when the response file contains only the energy dispersion
data = f['MATRIX', rsp_number].data
header = f['MATRIX', rsp_number].header
if arf_file is None:
warnings.warn(
"The response is in an extension called MATRIX, which usually means you also "
"need an ancillary file (ARF) which you didn't provide. You should refer to the "
"documentation of the instrument and make sure you don't need an ARF."
)
except Exception as e:
warnings.warn("The default choice for MATRIX extension failed:"+repr(e)+\
"available: "+" ".join([repr(e.header.get('EXTNAME')) for e in f]))
# Other detectors might use the SPECRESP MATRIX name instead, usually when the response has been
# already convoluted with the effective area
# Note that here we are not catching any exception, because
# we have to fail if we cannot read the matrix
data = f['SPECRESP MATRIX', rsp_number].data
header = f['SPECRESP MATRIX', rsp_number].header
# These 3 operations must be executed when the file is still open
matrix = self._read_matrix(data, header)
ebounds = self._read_ebounds(f['EBOUNDS'])
mc_channels = self._read_mc_channels(data)
# Now, if there is information on the coverage interval, let's use it
header_start = header.get("TSTART", None)
header_stop = header.get("TSTOP", None)
if header_start is not None and header_stop is not None:
super(OGIPResponse,
self).__init__(matrix=matrix,
ebounds=ebounds,
monte_carlo_energies=mc_channels,
coverage_interval=TimeInterval(
header_start, header_stop))
else:
super(OGIPResponse,
self).__init__(matrix=matrix,
ebounds=ebounds,
monte_carlo_energies=mc_channels)
# Read the ARF if there is any
# NOTE: this has to happen *after* calling the parent constructor
if arf_file is not None and arf_file.lower() != 'none':
self._read_arf_file(arf_file)
else:
self._arf_file = None
def from_root_file(cls, response_file_name):
"""
Build response from a ROOT file. Do not use directly, use the hawc_response_factory function instead.
:param response_file_name:
:return: a HAWCResponse instance
"""
from ..root_handler import open_ROOT_file, get_list_of_keys, tree_to_ndarray
# Make sure file is readable
response_file_name = sanitize_filename(response_file_name)
# Check that they exists and can be read
if not file_existing_and_readable(
response_file_name): # pragma: no cover
raise IOError("Response %s does not exist or is not readable" %
response_file_name)
# Read response
with open_ROOT_file(response_file_name) as root_file:
# Get the name of the trees
object_names = get_list_of_keys(root_file)
# Make sure we have all the things we need
assert 'LogLogSpectrum' in object_names
assert 'DecBins' in object_names
assert 'AnalysisBins' in object_names
# Read spectrum used during the simulation
log_log_spectrum = root_file.Get("LogLogSpectrum")
# Get the analysis bins definition
dec_bins_ = tree_to_ndarray(root_file.Get("DecBins"))
dec_bins_lower_edge = dec_bins_['lowerEdge'] # type: np.ndarray
dec_bins_upper_edge = dec_bins_['upperEdge'] # type: np.ndarray
dec_bins_center = dec_bins_['simdec'] # type: np.ndarray
dec_bins = zip(dec_bins_lower_edge, dec_bins_center,
dec_bins_upper_edge)
# Read in the ids of the response bins ("analysis bins" in LiFF jargon)
try:
response_bins_ids = tree_to_ndarray(
root_file.Get("AnalysisBins"), "name") # type: np.ndarray
except ValueError:
try:
response_bins_ids = tree_to_ndarray(
root_file.Get("AnalysisBins"),
"id") # type: np.ndarray
except ValueError:
# Some old response files (or energy responses) have no "name" branch
custom_warnings.warn(
"Response %s has no AnalysisBins 'id' or 'name' branch. "
"Will try with default names" % response_file_name)
response_bins_ids = None
response_bins_ids = response_bins_ids.astype(str)
# Now we create a dictionary of ResponseBin instances for each dec bin_name
response_bins = collections.OrderedDict()
for dec_id in range(len(dec_bins)):
this_response_bins = collections.OrderedDict()
min_dec, dec_center, max_dec = dec_bins[dec_id]
# If we couldn't get the reponse_bins_ids above, let's use the default names
if response_bins_ids is None:
# Default are just integers. let's read how many nHit bins are from the first dec bin
dec_id_label = "dec_%02i" % dec_id
n_energy_bins = root_file.Get(dec_id_label).GetNkeys()
response_bins_ids = range(n_energy_bins)
for response_bin_id in response_bins_ids:
this_response_bin = ResponseBin.from_ttree(
root_file, dec_id, response_bin_id, log_log_spectrum,
min_dec, dec_center, max_dec)
this_response_bins[response_bin_id] = this_response_bin
response_bins[dec_bins[dec_id][1]] = this_response_bins
# Now the file is closed. Let's explicitly remove f so we are sure it is freed
del root_file
# Instance the class and return it
instance = cls(response_file_name, dec_bins, response_bins)
return instance
def from_root_file(cls, response_file_name):
# Make sure file is readable
response_file_name = sanitize_filename(response_file_name)
# Check that they exists and can be read
if not file_existing_and_readable(
response_file_name): # pragma: no cover
raise IOError("Response %s does not exist or is not readable" %
response_file_name)
# Read response
with open_ROOT_file(response_file_name) as f:
# Get the name of the trees
object_names = get_list_of_keys(f)
# Make sure we have all the things we need
assert 'LogLogSpectrum' in object_names
assert 'DecBins' in object_names
assert 'AnalysisBins' in object_names
# Read spectrum used during the simulation
log_log_spectrum = f.Get("LogLogSpectrum")
# Get the analysis bins definition
dec_bins_ = tree_to_ndarray(f.Get("DecBins"))
dec_bins_lower_edge = dec_bins_['lowerEdge'] # type: np.ndarray
dec_bins_upper_edge = dec_bins_['upperEdge'] # type: np.ndarray
dec_bins_center = dec_bins_['simdec'] # type: np.ndarray
dec_bins = zip(dec_bins_lower_edge, dec_bins_center,
dec_bins_upper_edge)
# Read in the ids of the response bins ("analysis bins" in LiFF jargon)
response_bins_ids = tree_to_ndarray(f.Get("AnalysisBins"),
"id") # type: np.ndarray
# Now we create a list of ResponseBin instances for each dec bin_name
response_bins = {}
for dec_id in range(len(dec_bins)):
this_response_bins = []
min_dec, dec_center, max_dec = dec_bins[dec_id]
for response_bin_id in response_bins_ids:
this_response_bin = ResponseBin.from_ttree(
f, dec_id, response_bin_id, log_log_spectrum, min_dec,
dec_center, max_dec)
this_response_bins.append(this_response_bin)
response_bins[dec_bins[dec_id][1]] = this_response_bins
# Now the file is closed. Let's explicitly remove f so we are sure it is freed
del f
# Instance the class and return it
instance = cls(response_file_name, dec_bins, response_bins)
return instance