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doc/source/users/tutorials/1dc/classical_analysis.rst
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| 1 | +.. _classical_analysis: | |
| 2 | + | |
| 3 | +Performing a classical analysis | |
| 4 | +-------------------------------- | |
| 5 | + | |
| 6 | + .. admonition:: What you will learn | |
| 7 | + | |
| 8 | + You will learn how to perform a *classical* atmospheric Cherenkov analysis | |
| 9 | + of a source. In thys type of analysis you do not need to have a 3D (spatial | |
| 10 | + and spectral) model of the residual hadronic background. First you create a | |
| 11 | + skymap to identify a source region. Then, you extract the measured counts | |
| 12 | + from the source region and from one or more background regions, and perform | |
| 13 | + a 1D maximum likelihood analysis to derive the source's spectrum. | |
| 14 | + | |
| 15 | +We will assume that you have selected the observations available around your | |
| 16 | +source of interest. You can do this using the :ref:`csobsselect` script. | |
| 17 | + | |
| 18 | +We will derive the spectrum of a source with known position, i.e., the supernova | |
| 19 | +remnants Cassiopeia A. First, you want to create a skymap to identify the source | |
| 20 | +region. You can do this using the :ref:`ctskymap` tool. | |
| 21 | + | |
| 22 | +.. code-block:: bash | |
| 23 | + | |
| 24 | +In the spirit of the classical analysis we have chosen to derive the background | |
| 25 | +using the RING method. You need to choose inner/outer radii such that you avoid | |
| 26 | +emission from a source when deriving the background. This means that the inner | |
| 27 | +radius must be larger than the source's size, or the instrument PSF for a | |
| 28 | +pointlike source. This has produced a FITS file ``skymap.fits`` that contains | |
| 29 | +three images of the region around the source. The primary image shows the excess | |
| 30 | +counts, i.e., the total number of counts minus the estimated background counts. | |
| 31 | +The BACKGROUND image shows the number of estimated background counts. Finally, | |
| 32 | +the SIGNIFICANCE image shows the significance of the excess, calculated | |
| 33 | +according to Li&Ma | ... | ... |