Difference between revisions of "BLLac2022flare"

From my_wiki
Jump to: navigation, search
(→‎DL1 data)
Line 59: Line 59:
 
==DL1 data==
 
==DL1 data==
  
−
Please include your settings to produce your DL1a and DL1b files.  This includes whether you use LSTOSA, specific versions of lstchain, dllab scripts, cleaning levels, and calibration information.
 
  
 
'''Dark data''' :  
 
'''Dark data''' :  
  
−
Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)
+
'''Moon data''' :
 +
 
 +
Moon data reprocessed to produce the DL1b files with the optimal cleaning for moon analysis as calculated with lstchain_dvr_pixselector -f "/fefs/aswg/data/real/DL1/2022XXXX/v0.9/tailcut84/dl1_LST-1.RunXXXXX'.*.h5"
 +
Reprocessed using DL1a files produced by LSTOSA (lstchain v0.10.XX) and dl1ab script (v0.7.5)
  
 
* original DL1a files
 
* original DL1a files
Line 70: Line 72:
 
  /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/
 
  /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
+
SPECIFY THE CONFIGURATION FOR OPTIMIZING THE CLEANING
−
* 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
 
* Produced DL1b files
Line 92: Line 78:
 
  /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/data/
 
  /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
 
  /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 variabules used in the RF. 
 
−
 
−
'''Example'''
 
−
 
−
* lstchain-0.7.6.dev242+g2086cb9
 
−
 
−
* source-indep (diffuse gamma, src_r<3deg, disp_norm)
 
−
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/RF/lstchain_standard_config.json
 
−
 
−
 
−
* source-dep
 
−
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/RF/lstchain_src_dep_config.json
 
−
 
−
==DL2 data==
 
−
 
−
Information about your DL2 data and settings such as: specific versions of lstchain, specific .json version used.
 
−
 
−
'''Example''':
 
−
 
−
* lstchain-0.7.6.dev242+g2086cb9
 
−
 
−
* 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
 
−
 
−
* source-dep
 
−
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/DL2/data/
 
−
/fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcdep/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
 
−
**fixed_gh_cut: 0.3
 
−
**fixed_theta_cut: 0.2
 
−
 
−
* source-dep
 
−
**fixed_gh_cut: 0.7
 
−
**fixed_alpha_cut: 10
 
  
 
==High-level analysis==
 
==High-level analysis==

Revision as of 09:59, 6 June 2024

BL Lacertae 2022 flare project

General information

  • Name of the source: BL Lacertae
  • Brief description of the source:
- Object type : Blazar
- RA: 22 02 43.3 (hh mm ss), Dec: +42 16 40 (dd mm ss)
  • Analysis by:
    • Jorge Otero Santos (IAA-CSIC, joteros@iaa.es)
    • Daniel Morcuende (IAA-CSIC, dmorcuende@iaa.es)

Data-taking information

  • Dates of data-taking:
    • Date: 16/09/2022-25/11/2022 (53 h before cuts)
      • ZD range (deg): 15-60 deg
      • AZ range (deg): 0-60 and 300-360 deg
      • Joint observations with MAGIC? : No
      • Runs:
1 : 2022-09-16 : 9228 to 9232
2 : 2022-09-21 : 9262 to 9268
3 : 2022-09-22 : 9347 to 9350
4: 2022-10-01: 9453 to 9461
5: 2022-10-03: 9544 to 9555
6: 2022-10-15: 9631 to 9635
7: 2022-10-16: 9648
8: 2022-10-17: 9678 to 9685
9: 2022-10-18: 9697 to 9706
10: 2022-10-19: 9729 to 9739
11: 2022-10-20: 9753 to 9761
12: 2022-10-21: 9808 to 9815
13: 2022-10-23: 9836 to 9848
14: 2022-10-24: 9864 to 9873
15: 2022-10-25: 9892 to 9900
16: 2022-10-26: 9921 to 9924
17: 2022-10-27: 9940 to 9944
18: 2022-10-28: 9969 to 9973
19: 2022-10-29: 9993 to 9995
20: 2022-10-31: 10022 to 10029
21: 2022-11-01: 10069 to 10076
22: 2022-11-02: 10193 to 10204
23: 2022-11-13: 10508 to 10512
24: 2022-11-14: 10521 to 10523
25: 2022-11-15: 10586 to 10588
26: 2022-11-16: 10616 to 10620
27: 2022-11-17: 10652 to 10655
28: 2022-11-18: 10827 to 10830
29: 2022-11-19: 10870 to 10872
30: 2022-11-25: 11033 to 11037

Monte Carlo information

  • Link to MC files used:
    • Dark data: /fefs/aswg/data/mc/DL2/AllSky/20230925_v0.10.4_src3_dec3476_4822_tuned/TestingDataset/dec_3476/
    • Moon data: /fefs/aswg/data/mc/DL2/AllSky/20240426_v0.10.9_src3_dec3476_4822_tunedNSB/TestingDataset/dec_3476/ (tuned NSBs and cleaning to match that needed for the real data)

DL1 data

Dark data :

Moon data :

Moon data reprocessed to produce the DL1b files with the optimal cleaning for moon analysis as calculated with lstchain_dvr_pixselector -f "/fefs/aswg/data/real/DL1/2022XXXX/v0.9/tailcut84/dl1_LST-1.RunXXXXX'.*.h5" Reprocessed using DL1a files produced by LSTOSA (lstchain v0.10.XX) 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/

SPECIFY THE CONFIGURATION FOR OPTIMIZING THE CLEANING

  • 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

High-level analysis

Please put any information about the production of higher level analysis here.

Example

  • lstchain to generate source-dep IRF, DL3
  • Science Tool: gammapy 0.18.2
  • 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

Retrieved from "https://www.lst1.iac.es/wiki/index.php?title=BLLac2022flare&oldid=10383"