# Licensed under a 3-clause BSD style license - see LICENSE.rst
import collections.abc
import copy
import logging
import numpy as np
from astropy.coordinates import SkyCoord
from astropy.time import Time
from astropy.units import Quantity
from gammapy.irf import Background3D, load_cta_irfs
from gammapy.utils.fits import LazyFitsData, earth_location_from_dict
from gammapy.utils.testing import Checker
from .event_list import EventListChecker
from .filters import ObservationFilter
from .gti import GTI
from .pointing import FixedPointingInfo
__all__ = ["Observation", "Observations"]
log = logging.getLogger(__name__)
[docs]class Observation:
"""In-memory observation.
Parameters
----------
obs_id : int
Observation id
obs_info : dict
Observation info dict
aeff : `~gammapy.irf.EffectiveAreaTable2D`
Effective area
edisp : `~gammapy.irf.EnergyDispersion2D`
Energy dispersion
psf : `~gammapy.irf.PSF3D`
Point spread function
bkg : `~gammapy.irf.Background3D`
Background rate model
gti : `~gammapy.data.GTI`
Table with GTI start and stop time
events : `~gammapy.data.EventList`
Event list
obs_filter : `ObservationFilter`
Observation filter.
"""
aeff = LazyFitsData(cache=False)
edisp = LazyFitsData(cache=False)
psf = LazyFitsData(cache=False)
bkg = LazyFitsData(cache=False)
_events = LazyFitsData(cache=False)
_gti = LazyFitsData(cache=False)
def __init__(
self,
obs_id=None,
obs_info=None,
gti=None,
aeff=None,
edisp=None,
psf=None,
bkg=None,
events=None,
obs_filter=None,
):
self.obs_id = obs_id
self.obs_info = obs_info
self.aeff = aeff
self.edisp = edisp
self.psf = psf
self.bkg = bkg
self._gti = gti
self._events = events
self.obs_filter = obs_filter or ObservationFilter()
@property
def events(self):
events = self.obs_filter.filter_events(self._events)
return events
@property
def gti(self):
events = self.obs_filter.filter_gti(self._gti)
return events
@staticmethod
def _get_obs_info(pointing, deadtime_fraction):
"""Create obs info dict from in memory data"""
return {
"RA_PNT": pointing.icrs.ra.deg,
"DEC_PNT": pointing.icrs.dec.deg,
"DEADC": 1 - deadtime_fraction,
}
[docs] @classmethod
def create(
cls,
pointing,
obs_id=0,
livetime=None,
tstart=None,
tstop=None,
irfs=None,
deadtime_fraction=0.0,
reference_time="2000-01-01",
):
"""Create an observation.
User must either provide the livetime, or the start and stop times.
Parameters
----------
pointing : `~astropy.coordinates.SkyCoord`
Pointing position
obs_id : int
Observation ID as identifier
livetime : ~astropy.units.Quantity`
Livetime exposure of the simulated observation
tstart : `~astropy.units.Quantity`
Start time of observation w.r.t reference_time
tstop : `~astropy.units.Quantity` w.r.t reference_time
Stop time of observation
irfs : dict
IRFs used for simulating the observation: `bkg`, `aeff`, `psf`, `edisp`
deadtime_fraction : float, optional
Deadtime fraction, defaults to 0
reference_time : `~astropy.time.Time`
the reference time to use in GTI definition
Returns
-------
obs : `gammapy.data.MemoryObservation`
"""
if tstart is None:
tstart = Quantity(0.0, "hr")
if tstop is None:
tstop = tstart + Quantity(livetime)
gti = GTI.create([tstart], [tstop], reference_time=reference_time)
obs_info = cls._get_obs_info(
pointing=pointing, deadtime_fraction=deadtime_fraction
)
return cls(
obs_id=obs_id,
obs_info=obs_info,
gti=gti,
aeff=irfs.get("aeff"),
bkg=irfs.get("bkg"),
edisp=irfs.get("edisp"),
psf=irfs.get("psf"),
)
[docs] @classmethod
def from_caldb(
cls,
pointing,
obs_id=None,
livetime=None,
tstart=None,
tstop=None,
caldb="prod2",
irf="South0.5hr",
deadtime_fraction=0.0,
):
"""Create an observation using IRFs from a given CTA CALDB.
Parameters
----------
pointing : `~astropy.coordinates.SkyCoord`
Pointing position
obs_id : int
Observation ID as identifier
livetime : ~astropy.units.Quantity`
Livetime exposure of the simulated observation
tstart : `~astropy.units.Quantity`
Start time of observation
tstop : `~astropy.units.Quantity`
Stop time of observation
caldb : str
Calibration database
irf : str
Type of Instrumental response function.
deadtime_fraction : float, optional
Deadtime fraction, defaults to 0
Returns
-------
obs : `gammapy.data.Observation`
"""
from .data_store import CalDBIRF
irf_loc = CalDBIRF("CTA", caldb, irf)
filename = irf_loc.file_dir + irf_loc.file_name
irfs = load_cta_irfs(filename)
return cls.create(
pointing=pointing,
obs_id=obs_id,
livetime=livetime,
tstart=tstart,
tstop=tstop,
irfs=irfs,
deadtime_fraction=deadtime_fraction,
)
@property
def tstart(self):
"""Observation start time (`~astropy.time.Time`)."""
return self.gti.time_start[0]
@property
def tstop(self):
"""Observation stop time (`~astropy.time.Time`)."""
return self.gti.time_stop[0]
@property
def observation_time_duration(self):
"""Observation time duration in seconds (`~astropy.units.Quantity`).
The wall time, including dead-time.
"""
return self.gti.time_sum
@property
def observation_live_time_duration(self):
"""Live-time duration in seconds (`~astropy.units.Quantity`).
The dead-time-corrected observation time.
Computed as ``t_live = t_observation * (1 - f_dead)``
where ``f_dead`` is the dead-time fraction.
"""
return self.observation_time_duration * (
1 - self.observation_dead_time_fraction
)
@property
def observation_dead_time_fraction(self):
"""Dead-time fraction (float).
Defined as dead-time over observation time.
Dead-time is defined as the time during the observation
where the detector didn't record events:
https://en.wikipedia.org/wiki/Dead_time
https://ui.adsabs.harvard.edu/abs/2004APh....22..285F
The dead-time fraction is used in the live-time computation,
which in turn is used in the exposure and flux computation.
"""
return 1 - self.obs_info["DEADC"]
@property
def pointing_radec(self):
"""Pointing RA / DEC sky coordinates (`~astropy.coordinates.SkyCoord`)."""
lon, lat = (
self.obs_info.get("RA_PNT", np.nan),
self.obs_info.get("DEC_PNT", np.nan),
)
return SkyCoord(lon, lat, unit="deg", frame="icrs")
@property
def pointing_altaz(self):
"""Pointing ALT / AZ sky coordinates (`~astropy.coordinates.SkyCoord`)."""
alt, az = (
self.obs_info.get("ALT_PNT", np.nan),
self.obs_info.get("AZ_PNT", np.nan),
)
return SkyCoord(az, alt, unit="deg", frame="altaz")
@property
def pointing_zen(self):
"""Pointing zenith angle sky (`~astropy.units.Quantity`)."""
return Quantity(self.obs_info.get("ZEN_PNT", np.nan), unit="deg")
@property
def fixed_pointing_info(self):
"""Fixed pointing info for this observation (`FixedPointingInfo`)."""
return FixedPointingInfo(self.events.table.meta)
@property
def target_radec(self):
"""Target RA / DEC sky coordinates (`~astropy.coordinates.SkyCoord`)."""
lon, lat = (
self.obs_info.get("RA_OBJ", np.nan),
self.obs_info.get("DEC_OBJ", np.nan),
)
return SkyCoord(lon, lat, unit="deg", frame="icrs")
@property
def observatory_earth_location(self):
"""Observatory location (`~astropy.coordinates.EarthLocation`)."""
return earth_location_from_dict(self.obs_info)
@property
def muoneff(self):
"""Observation muon efficiency."""
return self.obs_info.get("MUONEFF", 1)
def __str__(self):
ra = self.pointing_radec.ra.deg
dec = self.pointing_radec.dec.deg
pointing = f"{ra:.1f} deg, {dec:.1f} deg\n"
# TODO: Which target was observed?
# TODO: print info about available HDUs for this observation ...
return (
f"{self.__class__.__name__}\n\n"
f"\tobs id : {self.obs_id} \n "
f"\ttstart : {self.tstart.mjd:.2f}\n"
f"\ttstop : {self.tstop.mjd:.2f}\n"
f"\tduration : {self.observation_time_duration:.2f}\n"
f"\tpointing (icrs) : {pointing}\n"
f"\tdeadtime fraction : {self.observation_dead_time_fraction:.1%}\n"
)
[docs] def check(self, checks="all"):
"""Run checks.
This is a generator that yields a list of dicts.
"""
checker = ObservationChecker(self)
return checker.run(checks=checks)
[docs] def peek(self, figsize=(12, 10)):
"""Quick-look plots in a few panels.
Parameters
----------
figszie : tuple
Figure size
"""
import matplotlib.pyplot as plt
fig, ((ax_aeff, ax_bkg), (ax_psf, ax_edisp)) = plt.subplots(
nrows=2,
ncols=2,
figsize=figsize,
gridspec_kw={"wspace": 0.25, "hspace": 0.25},
)
self.aeff.plot(ax=ax_aeff)
try:
if isinstance(self.bkg, Background3D):
bkg = self.bkg.to_2d()
else:
bkg = self.bkg
bkg.plot(ax=ax_bkg)
except IndexError:
logging.warning(f"No background model found for obs {self.obs_id}.")
self.psf.plot_containment_vs_energy(ax=ax_psf)
self.edisp.plot_bias(ax=ax_edisp, add_cbar=True)
ax_aeff.set_title("Effective area")
ax_bkg.set_title("Background rate")
ax_psf.set_title("Point spread function")
ax_edisp.set_title("Energy dispersion")
[docs] def select_time(self, time_interval):
"""Select a time interval of the observation.
Parameters
----------
time_interval : `astropy.time.Time`
Start and stop time of the selected time interval.
For now we only support a single time interval.
Returns
-------
new_obs : `~gammapy.data.Observation`
A new observation instance of the specified time interval
"""
new_obs_filter = self.obs_filter.copy()
new_obs_filter.time_filter = time_interval
obs = copy.deepcopy(self)
obs.obs_filter = new_obs_filter
return obs
[docs]class Observations(collections.abc.MutableSequence):
"""Container class that holds a list of observations.
Parameters
----------
observations : list
A list of `~gammapy.data.Observation`
"""
def __init__(self, observations=None):
self._observations = observations or []
def __getitem__(self, key):
return self._observations[self.index(key)]
def __delitem__(self, key):
del self._observations[self.index(key)]
def __setitem__(self, key, obs):
if isinstance(obs, Observation):
self._observations[self.index(key)] = obs
else:
raise TypeError(f"Invalid type: {type(obs)!r}")
[docs] def insert(self, idx, obs):
if isinstance(obs, Observation):
self._observations.insert(idx, obs)
else:
raise TypeError(f"Invalid type: {type(obs)!r}")
def __len__(self):
return len(self._observations)
def __str__(self):
s = self.__class__.__name__ + "\n"
s += "Number of observations: {}\n".format(len(self))
for obs in self:
s += str(obs)
return s
[docs] def index(self, key):
if isinstance(key, (int, slice)):
return key
elif isinstance(key, str):
return self.ids.index(key)
elif isinstance(key, Observation):
return self._observations.index(key)
else:
raise TypeError(f"Invalid type: {type(key)!r}")
@property
def ids(self):
"""List of obs IDs (`list`)"""
return [str(obs.obs_id) for obs in self]
[docs] def select_time(self, time_intervals):
"""Select a time interval of the observations.
Parameters
----------
time_intervals : `astropy.time.Time` or list of `astropy.time.Time`
list of Start and stop time of the time intervals or one Time interval
Returns
-------
new_observations : `~gammapy.data.Observations`
A new Observations instance of the specified time intervals
"""
new_obs_list = []
if isinstance(time_intervals, Time):
time_intervals = [time_intervals]
for time_interval in time_intervals:
for obs in self:
if (obs.tstart < time_interval[1]) & (obs.tstop > time_interval[0]):
new_obs = obs.select_time(time_interval)
new_obs_list.append(new_obs)
return self.__class__(new_obs_list)
def _ipython_key_completions_(self):
return self.ids
class ObservationChecker(Checker):
"""Check an observation.
Checks data format and a bit about the content.
"""
CHECKS = {
"events": "check_events",
"gti": "check_gti",
"aeff": "check_aeff",
"edisp": "check_edisp",
"psf": "check_psf",
}
def __init__(self, observation):
self.observation = observation
def _record(self, level="info", msg=None):
return {"level": level, "obs_id": self.observation.obs_id, "msg": msg}
def check_events(self):
yield self._record(level="debug", msg="Starting events check")
try:
events = self.observation.events
except Exception:
yield self._record(level="warning", msg="Loading events failed")
return
yield from EventListChecker(events).run()
# TODO: split this out into a GTIChecker
def check_gti(self):
yield self._record(level="debug", msg="Starting gti check")
try:
gti = self.observation.gti
except Exception:
yield self._record(level="warning", msg="Loading GTI failed")
return
if len(gti.table) == 0:
yield self._record(level="error", msg="GTI table has zero rows")
columns_required = ["START", "STOP"]
for name in columns_required:
if name not in gti.table.colnames:
yield self._record(level="error", msg=f"Missing table column: {name!r}")
# TODO: Check that header keywords agree with table entries
# TSTART, TSTOP, MJDREFI, MJDREFF
# Check that START and STOP times are consecutive
# times = np.ravel(self.table['START'], self.table['STOP'])
# # TODO: not sure this is correct ... add test with a multi-gti table from Fermi.
# if not np.all(np.diff(times) >= 0):
# yield 'GTIs are not consecutive or sorted.'
# TODO: add reference times for all instruments and check for this
# Use TELESCOP header key to check which instrument it is.
def _check_times(self):
"""Check if various times are consistent.
The headers and tables of the FITS EVENTS and GTI extension
contain various observation and event time information.
"""
# http://fermi.gsfc.nasa.gov/ssc/data/analysis/documentation/Cicerone/Cicerone_Data/Time_in_ScienceTools.html
# https://hess-confluence.desy.de/confluence/display/HESS/HESS+FITS+data+-+References+and+checks#HESSFITSdata-Referencesandchecks-Time
telescope_met_refs = {
"FERMI": Time("2001-01-01T00:00:00"),
"HESS": Time("2001-01-01T00:00:00"),
}
meta = self.dset.event_list.table.meta
telescope = meta["TELESCOP"]
if telescope in telescope_met_refs.keys():
dt = self.time_ref - telescope_met_refs[telescope]
if dt > self.accuracy["time"]:
yield self._record(
level="error", msg="Reference time incorrect for telescope"
)
def check_aeff(self):
yield self._record(level="debug", msg="Starting aeff check")
try:
aeff = self.observation.aeff
except Exception:
yield self._record(level="warning", msg="Loading aeff failed")
return
# Check that thresholds are meaningful for aeff
if (
"LO_THRES" in aeff.meta
and "HI_THRES" in aeff.meta
and aeff.meta["LO_THRES"] >= aeff.meta["HI_THRES"]
):
yield self._record(
level="error", msg="LO_THRES >= HI_THRES in effective area meta data"
)
# Check that data isn't all null
if np.max(aeff.data.data) <= 0:
yield self._record(
level="error", msg="maximum entry of effective area is <= 0"
)
def check_edisp(self):
yield self._record(level="debug", msg="Starting edisp check")
try:
edisp = self.observation.edisp
except Exception:
yield self._record(level="warning", msg="Loading edisp failed")
return
# Check that data isn't all null
if np.max(edisp.data.data) <= 0:
yield self._record(level="error", msg="maximum entry of edisp is <= 0")
def check_psf(self):
yield self._record(level="debug", msg="Starting psf check")
try:
self.observation.psf
except Exception:
yield self._record(level="warning", msg="Loading psf failed")
return
# TODO: implement some basic check
# The following doesn't work, because EnergyDependentMultiGaussPSF
# has no attribute `data`
# Check that data isn't all null
# if np.max(psf.data.data) <= 0:
# yield self._record(
# level="error", msg="maximum entry of psf is <= 0"
# )