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 : Unknown, AGN, SNR, Pulsar, PWN, GRB, etc
** Redshift (z) :
** 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
** José Manuel

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


==Monte Carlo information==
* Link to MC files used:
** Particle types: 
** ZD (deg): Zenith Range
** AZ (deg): Azimuth Range

==DL1 data==


Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)

* original DL1a files

 /fefs/aswg/data/real/DL1/20210808/v0.7.3/tailcut84/dl1_LST-1.Run0XXXX.XXXX.h5
 /fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/XXX/zenith_20deg/south_pointing/20210416_v0.7.3_prod5_trans_80_local_taicut_8_4/

* lstchain v0.7.5
* real data: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning

  /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/lstchain_standard_config.json

* MC: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning, PSF+NSB tuning
  "image_modifier": {
    "increase_nsb": true,
    "extra_noise_in_dim_pixels": 0.74,
    "extra_bias_in_dim_pixels": 0.38,
    "transition_charge": 8,
    "extra_noise_in_bright_pixels": 0.052,
    "increase_psf": true,
    "smeared_light_fraction": 0.125
  },

  /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/lstchain_dl1ab_tune_MC_to_BLLac_config.json

* Produced DL1b files

 /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/data/
 /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/Run0XXXX


==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.  


==DL2 data==


* lstchain-v0.10

* source-indep
 /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/DL2/data/
 /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcindep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5

==DL3 data selection==

Information about your DL3 data selection. 

'''Example'''
*intensity > 50
*r: [0,  1 ]
*wl: [0.1, 1 ]
*leakage_intensity_width_2: [0, 0.2 ]

* source-indep



==High-level analysis==

* lstchain to generate source-dep IRF, DL3
* Science Tool: Gammapy 1.1
* point-like IRF, 1D analysis

==Analysis Results==

Please place higher-level analysis results (Spectra, SkyMaps, Lightcurves, etc) here.

=== Theta2 plot ===

=== Significance map ===

=== Excess map ===

=== Spectral results ===