Difference between revisions of "NGC1068 LST1 analysis Cycle I DanielMorcuende"
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***Runs: | ***Runs: | ||
| + | ==Analysis information== | ||
| + | * lstchain v0.10 | ||
| + | * source-independent analysis | ||
| + | * Gammapy v1.1 | ||
==Monte Carlo information== | ==Monte Carlo information== | ||
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==DL1 data== | ==DL1 data== | ||
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Standard DL1b files produced by LSTOSA (lstchain v0.10, tailcut 8-4 with cleaning based on pedestal RMS, dynamic cleaning) | Standard DL1b files produced by LSTOSA (lstchain v0.10, tailcut 8-4 with cleaning based on pedestal RMS, dynamic cleaning) | ||
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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. | 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. | ||
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==DL3 data selection== | ==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 | |
| − | *intensity > 50 | ||
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| − | * | ||
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==High-level analysis== | ==High-level analysis== | ||
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* Science Tool: Gammapy 1.1 | * Science Tool: Gammapy 1.1 | ||
* point-like IRF, 1D analysis | * point-like IRF, 1D analysis | ||
==Analysis Results== | ==Analysis Results== | ||
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=== Theta2 plot === | === Theta2 plot === | ||
Revision as of 14:11, 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:
- Date (time of observation h)
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
