Difference between revisions of "NGC1068 LST1 analysis Cycle I DanielMorcuende"

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(→‎General information)
(→‎Analysis of LST-1 NGC 1068 data from observation cycle I)
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* '''Name of the source''': NGC 1068
 
* '''Name of the source''': NGC 1068
 
* '''Brief description of the source''':  
 
* '''Brief description of the source''':  
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** Object type : AGN, Seyfert galaxy
+
** Object type : AGN, Seyfert II galaxy
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** Redshift (z) :
+
** Redshift (z) : 0.0037
 
** Other relevant information  
 
** Other relevant information  
 
** RA: XX XX XX.XX (hh mm ss), Dec: +/-YY YY YY.YY (dd mm ss)
 
** RA: XX XX XX.XX (hh mm ss), Dec: +/-YY YY YY.YY (dd mm ss)
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Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)
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Standard DL1b files produced by LSTOSA (lstchain v0.10, tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning)
  
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* original DL1a files
+
  /fefs/aswg/data/real/DL1/YYYYMMDD/v0.10/tailcut84/dl1_LST-1.Run?????.h5
−
 
 
−
  /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/
 
−
 
 
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* lstchain v0.7.5
 
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* 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
 
−
 
 
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* MC: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning, PSF+NSB tuning
 
−
  "image_modifier": {
 
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    "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
 
−
 
 
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* 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
 
  
  

Revision as of 14:00, 24 July 2024

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:


Monte Carlo information

  • Link to MC files used:
    • Particle types:
    • ZD (deg): Zenith Range
    • AZ (deg): Azimuth Range

DL1 data

Standard DL1b files produced by LSTOSA (lstchain v0.10, tailcut8-4 (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.


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

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