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:

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, 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.

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.