Commit 65bcb4a1f4064dd13dffa06495713d5229b4a8bd
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Add some more known issues related to El Capitan and the elliptical Gaussian model.
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doc/source/issues.rst
| @@ -5,11 +5,68 @@ Known issues | @@ -5,11 +5,68 @@ Known issues | ||
| 5 | 5 | ||
| 6 | Below you will find a list of known issues. | 6 | Below you will find a list of known issues. |
| 7 | 7 | ||
| 8 | +**Installation issues** | ||
| 9 | + | ||
| 10 | +- :ref:`Certificate problem when cloning from Git <issue_ssl>` | ||
| 11 | +- :ref:`Python unit test fail on El Capitan <issue_elcapitan>` | ||
| 12 | + | ||
| 13 | +**Analysis issues** | ||
| 14 | + | ||
| 15 | +- :ref:`Binned analysis is biased for coarse binning <issue_binned>` | ||
| 16 | + | ||
| 17 | +**Model fitting issues** | ||
| 18 | + | ||
| 8 | - :ref:`Broken power law has unreliable errors <issue_bplaw>` | 19 | - :ref:`Broken power law has unreliable errors <issue_bplaw>` |
| 9 | - :ref:`Errors become unreliable when fitting the pivot energy <issue_pivot>` | 20 | - :ref:`Errors become unreliable when fitting the pivot energy <issue_pivot>` |
| 10 | -- :ref:`Binned analysis is biased when using coarse binning <issue_binned>` | ||
| 11 | - :ref:`Shell model is biased when width is comparable to angular resolution <issue_shell>` | 21 | - :ref:`Shell model is biased when width is comparable to angular resolution <issue_shell>` |
| 22 | +- :ref:`Elliptical Gaussian model fit converges slowly <issue_egauss>` | ||
| 23 | + | ||
| 24 | + | ||
| 25 | +Installation issues | ||
| 26 | +^^^^^^^^^^^^^^^^^^^ | ||
| 27 | + | ||
| 28 | +.. _issue_ssl: | ||
| 29 | + | ||
| 30 | +.. topic:: Certificate problem when cloning from Git | ||
| 31 | + | ||
| 32 | + When cloning ctools from git you may encounter an SSL certificate | ||
| 33 | + problem. This is related to the usage of the https protocol and can | ||
| 34 | + be resolved by setting the ``GIT_SSL_NO_VERIFY`` environment variable | ||
| 35 | + to true: | ||
| 36 | + | ||
| 37 | + .. code-block:: bash | ||
| 12 | 38 | ||
| 39 | + export GIT_SSL_NO_VERIFY=true | ||
| 40 | + | ||
| 41 | +.. _issue_elcapitan: | ||
| 42 | + | ||
| 43 | +.. topic:: Python unit test fail on El Capitan | ||
| 44 | + | ||
| 45 | + On Mac OS X 10.11 (El Capitan) the Python unit tests fail when ctools | ||
| 46 | + are not installed due to the way the ``DYLD_LIBRARY_PATH`` environment | ||
| 47 | + variable is handled by the operating system. A (not very elegant) | ||
| 48 | + workaround is to install the ctools before running the unit test using | ||
| 49 | + ``make check``. | ||
| 50 | + | ||
| 51 | + | ||
| 52 | +Analysis issues | ||
| 53 | +^^^^^^^^^^^^^^^ | ||
| 54 | + | ||
| 55 | +.. _issue_binned: | ||
| 56 | + | ||
| 57 | +.. topic:: Binned analysis is biased for coarse binning | ||
| 58 | + | ||
| 59 | + When performing a binned or stacked analysis you should make sure | ||
| 60 | + that the spatial and spectral binning is sufficiently fine grained. | ||
| 61 | + The spatial binning should be better than the best angular resolution | ||
| 62 | + over the energy range of interest. Use a typical value of 0.02 degrees | ||
| 63 | + per pixel for the spatial binning and 10 bins per decade for the | ||
| 64 | + spectral binning. If the binning is too coarse, the spectral parameters | ||
| 65 | + that are fitted will be biased. | ||
| 66 | + | ||
| 67 | + | ||
| 68 | +Model fitting issues | ||
| 69 | +^^^^^^^^^^^^^^^^^^^^ | ||
| 13 | 70 | ||
| 14 | .. _issue_bplaw: | 71 | .. _issue_bplaw: |
| 15 | 72 | ||
| @@ -35,18 +92,6 @@ Below you will find a list of known issues. | @@ -35,18 +92,6 @@ Below you will find a list of known issues. | ||
| 35 | parameters of the model to assure non-degeneracy of the free | 92 | parameters of the model to assure non-degeneracy of the free |
| 36 | parameters. | 93 | parameters. |
| 37 | 94 | ||
| 38 | -.. _issue_binned: | ||
| 39 | - | ||
| 40 | -.. topic:: Binned analysis is biased when using coarse binning | ||
| 41 | - | ||
| 42 | - When performing a binned or stacked analysis you should make sure | ||
| 43 | - that the spatial and spectral binning is sufficiently fine grained. | ||
| 44 | - The spatial binning should be better than the best angular resolution | ||
| 45 | - over the energy range of interest. Use a typical value of 0.02 degrees | ||
| 46 | - per pixel for the spatial binning and 10 bins per decade for the | ||
| 47 | - spectral binning. If the binning is too coarse, the spectral parameters | ||
| 48 | - that are fitted will be biased. | ||
| 49 | - | ||
| 50 | .. _issue_shell: | 95 | .. _issue_shell: |
| 51 | 96 | ||
| 52 | .. topic:: Shell model is biased when width is comparable to angular resolution | 97 | .. topic:: Shell model is biased when width is comparable to angular resolution |
| @@ -57,3 +102,11 @@ Below you will find a list of known issues. | @@ -57,3 +102,11 @@ Below you will find a list of known issues. | ||
| 57 | The fitted shell width and radius should thus not be overinterpreted | 102 | The fitted shell width and radius should thus not be overinterpreted |
| 58 | when the width is close to the angular resolution of CTA. | 103 | when the width is close to the angular resolution of CTA. |
| 59 | 104 | ||
| 105 | +.. _issue_egauss: | ||
| 106 | + | ||
| 107 | +.. topic:: Elliptical Gaussian model fit converges slowly | ||
| 108 | + | ||
| 109 | + The convergence of the elliptical Gaussian model can be slow and | ||
| 110 | + in some situations requires of the order of 20 iterations before | ||
| 111 | + the fit terminates. Nevertheless, the numerical accuracy of the model | ||
| 112 | + fitting results are satisfactory. |