From e40e2904c2efea83dd788cfc346a91cff8da61a0 Mon Sep 17 00:00:00 2001 From: Jürgen Knödlseder Date: Fri, 12 Feb 2021 11:12:40 +0100 Subject: [PATCH] Correct energy dispersion tutorial --- doc/source/users/tutorials/quickstart/energy_dispersion.rst | 24 ++++++++++++------------ 1 file changed, 12 insertions(+), 12 deletions(-) diff --git a/doc/source/users/tutorials/quickstart/energy_dispersion.rst b/doc/source/users/tutorials/quickstart/energy_dispersion.rst index 917713e..4421928 100755 --- a/doc/source/users/tutorials/quickstart/energy_dispersion.rst +++ b/doc/source/users/tutorials/quickstart/energy_dispersion.rst @@ -33,9 +33,9 @@ To simulate events taking the energy dispersion into account you run the Dec of pointing (degrees) (-90-90) [22.51] Radius of FOV (degrees) (0-180) [5.0] Start time (UTC string, JD, MJD or MET in seconds) [2020-01-01T00:00:00] - Stop time (UTC string, JD, MJD or MET in seconds) [2020-01-01T00:30:00] 2020-01-01T01:00:00 - Lower energy limit (TeV) [0.1] 0.03 - Upper energy limit (TeV) [100.0] 150.0 + Stop time (UTC string, JD, MJD or MET in seconds) [2020-01-01T01:00:00] + Lower energy limit (TeV) [0.03] + Upper energy limit (TeV) [150.0] Calibration database [prod2] Instrument response function [South_0.5h] Input model definition XML file [$CTOOLS/share/models/crab.xml] @@ -48,10 +48,10 @@ You then select events from the simulated data as before using the $ ctselect Input event list or observation definition XML file [events.fits] events_edisp.fits - Radius of ROI around pointing or specified RA/DEC (degrees) (0-180) [3.0] - Start time (UTC string, JD, MJD or MET in seconds) [NONE] 2020-01-01T00:10:00 - Stop time (UTC string, JD, MJD or MET in seconds) [NONE] 2020-01-01T00:40:00 - Lower energy limit (TeV) [0.1] + Radius of ROI around pointing or specified RA/DEC (degrees) (0-180) [NONE] 3.0 + Start time (UTC string, JD, MJD or MET in seconds) [2020-01-01T00:10:00] + Stop time (UTC string, JD, MJD or MET in seconds) [2020-01-01T00:40:00] + Lower energy limit (TeV) [NONE] 0.1 Upper energy limit (TeV) [100.0] Output event list or observation definition XML file [selected_events.fits] selected_events_edisp.fits @@ -61,7 +61,7 @@ Then you bin as before the selected events into a counts cube using the .. code-block:: bash $ ctbin - Input event list or observation definition XML file [events.fits] selected_events_edisp.fits + Input event list or observation definition XML file [selected_events.fits] selected_events_edisp.fits Coordinate system (CEL - celestial, GAL - galactic) (CEL|GAL) [CEL] Projection method (AIT|AZP|CAR|GLS|MER|MOL|SFL|SIN|STG|TAN) [CAR] First coordinate of image center in degrees (RA or galactic l) (0-360) [83.63] @@ -107,10 +107,10 @@ energy dispersion cube: .. code-block:: bash $ ctlike edisp=yes - Input event list, counts cube or observation definition XML file [events.fits] cntcube_edisp.fits - Input exposure cube file [NONE] expcube.fits - Input PSF cube file [NONE] psfcube.fits - Input background cube file [NONE] bkgcube.fits + Input event list, counts cube or observation definition XML file [selected_events.fits] cntcube_edisp.fits + Input exposure cube file [expcube.fits] + Input PSF cube file [psfcube.fits] + Input background cube file [bkgcube.fits] Input energy dispersion cube file [NONE] edispcube.fits Input model definition XML file [$CTOOLS/share/models/crab.xml] models.xml Output model definition XML file [crab_results.xml] crab_results_edisp.xml -- libgit2 0.21.4