Editing NGC1068 LST1 analysis Cycle I DanielMorcuende

=Analysis of LST-1 NGC 1068 data from observation cycle I=


==General information==
* '''Name of the source''': NGC 1068
* '''Brief description of the source''': 
** Object type : AGN, Seyfert II galaxy
** Redshift (z) : 0.0037
** Other relevant information 
** RA: XX XX XX.XX (hh mm ss), Dec: +/-YY YY YY.YY (dd mm ss)
** RA, Dec in deg (ICRS): XX.XX, YY.YY

* Analysis by Name (Institute - email)
** Daniel Morcuende (IAA-CSIC, dmorcuende@iaa.es)
** José Manuel Gavilán (IAA-CSIC)

==Data-taking information==
* '''Dates of data-taking''': 
** Date (time of observation h)
***ZD range (deg): Zenith Range
***AZ range (deg): Azimuth Range
***Runs: 

==Analysis information==
* lstchain v0.10
* source-independent analysis
* Gammapy v1.1

==Monte Carlo information==

Closest declination line towards La Palma latitude (28.8 deg)

 20240131_allsky_v0.10.5_all_dec_base/dec_931

==DL1 data==

Standard DL1b files produced by LSTOSA (lstchain v0.10, tailcut 8-4 with cleaning based on pedestal RMS, dynamic cleaning)

 /fefs/aswg/data/real/DL1/YYYYMMDD/v0.10/tailcut84/dl1_LST-1.Run?????.h5

==Random forest==

Please include your specific .json files used in producing your RFs and for which source analysis (source dependent or independent), and variables used in the RF.  


==DL3 data selection==
Files: 
 /fefs/aswg/workspace/daniel.morcuende/data/real/DL3/NGC1068/20240131_allsky_v0.10.5_all_dec_base/dec_931/gh_eff_0.7_th_cont_0.7

* intensity > 50 p.e.
* gammaness energy-dependent cuts with 70% efficiency
* theta energy-dependent cuts 70% efficiency


==High-level analysis==

* Science Tool: Gammapy 1.1
* point-like IRF, 1D analysis

==Analysis Results==

=== Theta2 plot ===

=== Significance map ===

=== Excess map ===

=== Spectral results ===