Example #1
0
def test_wcsndmap_downsample_axis():
    axis = MapAxis.from_edges([1, 2, 3, 4, 5], name="test")
    geom = WcsGeom.create(npix=(4, 4), axes=[axis])
    m = WcsNDMap(geom, unit="m2")
    m.data += 1

    m2 = m.downsample(2, preserve_counts=True, axis_name="test")
    assert m2.data.shape == (2, 4, 4)
Example #2
0
def test_wcsndmap_downsample(npix, binsz, frame, proj, skydir, axes):
    geom = WcsGeom.create(npix=npix, binsz=binsz, proj=proj, frame=frame, axes=axes)
    m = WcsNDMap(geom, unit="m2")
    # Check whether we can downsample
    if np.all(np.mod(geom.npix[0], 2) == 0) and np.all(np.mod(geom.npix[1], 2) == 0):
        m2 = m.downsample(2, preserve_counts=True)
        assert_allclose(np.nansum(m.data), np.nansum(m2.data))
        assert m.unit == m2.unit
Example #3
0
def make_map_background_irf(pointing, ontime, bkg, geom, oversampling=None):
    """Compute background map from background IRFs.

    Parameters
    ----------
    pointing : `~gammapy.data.FixedPointingInfo` or `~astropy.coordinates.SkyCoord`
        Observation pointing

        - If a ``FixedPointingInfo`` is passed, FOV coordinates are properly computed.
        - If a ``SkyCoord`` is passed, FOV frame rotation is not taken into account.
    ontime : `~astropy.units.Quantity`
        Observation ontime. i.e. not corrected for deadtime
        see https://gamma-astro-data-formats.readthedocs.io/en/stable/irfs/full_enclosure/bkg/index.html#notes)
    bkg : `~gammapy.irf.Background3D`
        Background rate model
    geom : `~gammapy.maps.WcsGeom`
        Reference geometry
    oversampling: int
        Oversampling factor in energy, used for the background model evaluation.

    Returns
    -------
    background : `~gammapy.maps.WcsNDMap`
        Background predicted counts sky cube in reco energy
    """
    # TODO:
    #  This implementation can be improved in two ways:
    #  1. Create equal time intervals between TSTART and TSTOP and sum up the
    #  background IRF for each interval. This is instead of multiplying by
    #  the total ontime. This then handles the rotation of the FoV.
    #  2. Use the pointing table (does not currently exist in CTA files) to
    #  obtain the RA DEC and time for each interval. This then considers that
    #  the pointing might change slightly over the observation duration

    # Get altaz coords for map
    if oversampling is not None:
        geom = geom.upsample(factor=oversampling, axis="energy")

    map_coord = geom.to_image().get_coord()
    sky_coord = map_coord.skycoord

    if isinstance(pointing, FixedPointingInfo):
        altaz_coord = sky_coord.transform_to(pointing.altaz_frame)

        # Compute FOV coordinates of map relative to pointing
        fov_lon, fov_lat = sky_to_fov(altaz_coord.az, altaz_coord.alt,
                                      pointing.altaz.az, pointing.altaz.alt)
    else:
        # Create OffsetFrame
        frame = SkyOffsetFrame(origin=pointing)
        pseudo_fov_coord = sky_coord.transform_to(frame)
        fov_lon = pseudo_fov_coord.lon
        fov_lat = pseudo_fov_coord.lat

    energies = geom.get_axis_by_name("energy").edges

    bkg_de = bkg.evaluate_integrate(
        fov_lon=fov_lon,
        fov_lat=fov_lat,
        energy_reco=energies[:, np.newaxis, np.newaxis],
    )

    d_omega = geom.to_image().solid_angle()
    data = (bkg_de * d_omega * ontime).to_value("")
    bkg_map = WcsNDMap(geom, data=data)

    if oversampling is not None:
        bkg_map = bkg_map.downsample(factor=oversampling, axis="energy")

    return bkg_map