コード例 #1
0
/***********************************************************************//**
 * @brief Set sky directions and solid angles of events cube.
 *
 * @exception GCTAException::no_sky
 *            No sky pixels found in event cube.
 *
 * This method computes the sky directions and solid angles for all event
 * cube pixels. Sky directions are stored in an array of GCTAInstDir objects
 * while solid angles are stored in units of sr in an array of double
 * precision variables.
 *
 * A kluge has been introduced that handles invalid pixels. Invalid pixels
 * may occur if a Hammer-Aitoff projection is used. In this case, pixels may
 * lie outside the valid sky region. As invalid pixels lead to exceptions
 * in the WCS classes, we simply need to catch the exceptions here. Invalid
 * pixels are signaled by setting the solid angle of the pixel to 0.
 ***************************************************************************/
void GCTAEventCube::set_directions(void)
{
    // Throw an error if we have no sky pixels
    if (npix() < 1) {
        throw GCTAException::no_sky(G_SET_DIRECTIONS, "Every CTA event cube"
                                   " needs a definition of the sky pixels.");
    }

    // Clear old pixel directions and solid angle
    m_dirs.clear();
    m_solidangle.clear();

    // Reserve space for pixel directions and solid angles
    m_dirs.reserve(npix());
    m_solidangle.reserve(npix());

    // Set pixel directions and solid angles
    for (int iy = 0; iy < ny(); ++iy) {
        for (int ix = 0; ix < nx(); ++ix) {
            try {
                GSkyPixel pixel = GSkyPixel(double(ix), double(iy));
                m_dirs.push_back(GCTAInstDir(m_map.pix2dir(pixel)));
                m_solidangle.push_back(m_map.solidangle(pixel));
            }
            catch (GException::wcs_invalid_x_y& e) {
                m_dirs.push_back(GCTAInstDir());
                m_solidangle.push_back(0.0);
            }
        }
    }

    // Return
    return;
}
コード例 #2
0
/***********************************************************************//**
 * @brief Return simulated list of events
 *
 * @param[in] obs Observation.
 * @param[in] ran Random number generator.
 * @return Pointer to list of simulated events (needs to be de-allocated by
 *         client)
 *
 * @exception GException::invalid_argument
 *            No CTA event list found in observation.
 *
 * Draws a sample of events from the background model using a Monte
 * Carlo simulation. The pointing information, the energy boundaries and the
 * good time interval for the sampling will be extracted from the observation
 * argument that is passed to the method. The method also requires a random
 * number generator of type GRan which is passed by reference, hence the
 * state of the random number generator will be changed by the method.
 *
 * The method also applies a deadtime correction using a Monte Carlo process,
 * taking into account temporal deadtime variations. For this purpose, the
 * method makes use of the time dependent GObservation::deadc method.
 ***************************************************************************/
GCTAEventList* GCTAModelBackground::mc(const GObservation& obs, GRan& ran) const
{
    // Initialise new event list
    GCTAEventList* list = new GCTAEventList;

    // Continue only if model is valid)
    if (valid_model()) {

        // Extract event list to access the ROI, energy boundaries and GTIs
        const GCTAEventList* events = dynamic_cast<const GCTAEventList*>(obs.events());
        if (events == NULL) {
            std::string msg = "No CTA event list found in observation.\n" +
                              obs.print();
            throw GException::invalid_argument(G_MC, msg);
        }

        // Get simulation region
        const GCTARoi&  roi     = events->roi();
        const GEbounds& ebounds = events->ebounds();
        const GGti&     gti     = events->gti();

        // Set simulation region for result event list
        list->roi(roi);
        list->ebounds(ebounds);
        list->gti(gti);

        // Loop over all energy boundaries
        for (int ieng = 0; ieng < ebounds.size(); ++ieng) {

            // Initialise de-allocation flag
            bool free_spectral = false;

            // Set pointer to spectral model
            GModelSpectral* spectral = m_spectral;

            // If the spectral model is a diffuse cube then create a node
            // function spectral model that is the product of the diffuse
            // cube node function and the spectral model evaluated at the
            // energies of the node function
            GModelSpatialDiffuseCube* cube =
                dynamic_cast<GModelSpatialDiffuseCube*>(m_spatial);
            if (cube != NULL) {

			   // Set MC simulation cone based on ROI
			   cube->set_mc_cone(roi.centre().dir(), roi.radius());

			   // Allocate node function to replace the spectral component
			   GModelSpectralNodes* nodes = new GModelSpectralNodes(cube->spectrum());
			   for (int i = 0; i < nodes->nodes(); ++i) {
				   GEnergy energy    = nodes->energy(i);
				   double  intensity = nodes->intensity(i);
				   double  norm      = m_spectral->eval(energy, events->tstart());
				   nodes->intensity(i, norm*intensity);
			   }

			   // Signal that node function needs to be de-allocated later
			   free_spectral = true;

			   // Set the spectral model pointer to the node function
			   spectral = nodes;

            } // endif: spatial model was a diffuse cube

            // Compute the background rate in model within the energy boundaries
            // from spectral component (units: cts/s).
            // Note that the time here is ontime. Deadtime correction will be done
            // later.
            double rate = spectral->flux(ebounds.emin(ieng), ebounds.emax(ieng));

            // Debug option: dump rate
            #if defined(G_DUMP_MC)
            std::cout << "GCTAModelBackground::mc(\"" << name() << "\": ";
            std::cout << "rate=" << rate << " cts/s)" << std::endl;
            #endif

            // Loop over all good time intervals
            for (int itime = 0; itime < gti.size(); ++itime) {

                // Get Monte Carlo event arrival times from temporal model
                GTimes times = m_temporal->mc(rate,
                                              gti.tstart(itime),
                                              gti.tstop(itime),
                                              ran);

                // Get number of events
                int n_events = times.size();

                // Reserve space for events
                if (n_events > 0) {
                    list->reserve(n_events);
                }

                // Loop over events
                for (int i = 0; i < n_events; ++i) {

                    // Apply deadtime correction
                    double deadc = obs.deadc(times[i]);
                    if (deadc < 1.0) {
                        if (ran.uniform() > deadc) {
                            continue;
                        }
                    }

                    // Get Monte Carlo event energy from spectral model
                    GEnergy energy = spectral->mc(ebounds.emin(ieng),
                                                  ebounds.emax(ieng),
                                                  times[i],
                                                  ran);

                    // Get Monte Carlo event direction from spatial model
                    GSkyDir dir = spatial()->mc(energy, times[i], ran);

                    // Allocate event
                    GCTAEventAtom event;

                    // Set event attributes
                    event.dir(GCTAInstDir(dir));
                    event.energy(energy);
                    event.time(times[i]);

                    // Append event to list if it falls in ROI
                    if (events->roi().contains(event)) {
                        list->append(event);
                    }

                } // endfor: looped over all events

            } // endfor: looped over all GTIs

            // Free spectral model if required
            if (free_spectral) delete spectral;

        } // endfor: looped over all energy boundaries

    } // endif: model was valid

    // Return
    return list;
}