Difference between revisions of "Analysis A. Aguasca-Cabot lstchain v0.9.X"
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Latest revision as of 11:28, 29 April 2022
Contents
Overview[edit]
- Source-dependent/independent analysis using LSTCHAIN v0.9.4 (MC production processed with LSTCHAIN v0.9.3, R0 to DL1 process by LSTOSA using LSTCHAIN v0.9.2)
- Cleaning method tail cut 84 and dynamic cleaning. Also, the MC files are tuned to match the NSB in the FoV and the PSF.
- Observations used in the analysis:
Monte Carlo information[edit]
- Link to MC files used:
- - Particle types: gamma off0.4deg, proton
- - ZD (deg): 40
- - AZ (deg): 180
- - Other information: MC production through PR in lstMCpipe Github webpage (https://github.com/cta-observatory/lstmcpipe/pull/185)
- - MC files are tuned to match the NSB in the FoV and the PSF.
DL1 data[edit]
- Processed with LSTOSA using LSTCHAIN v0.9.2.
- - Dynamic cleaning and tail cut cleaning with pedestal threshold applied by the the standard parameters using pipeline LSTOSA.
"dynamic_cleaning": { "apply": true, "threshold": 267, "fraction_cleaning_intensity": 0.03 }
Real data[edit]
- Parameters for the tail cut cleaning with pedestal threshold
"tailcuts_clean_with_pedestal_threshold": { "picture_thresh":8, "boundary_thresh":4, "sigma":2.5, "keep_isolated_pixels":false, "min_number_picture_neighbors":2, "use_only_main_island":false, "delta_time": 2 }
- Original DL1a files (processed up to DL1 by LSTOSA using LSTCHAIN v0.9.2)
/fefs/aswg/data/real/DL1/{}/v0.9/tailcut84/dl1_LST-1.RunXXXXX.XXXX.h5
MC data[edit]
- Tunned NSB
"increase_nsb": true, "extra_noise_in_dim_pixels": 0.6, "extra_bias_in_dim_pixels": 0.269, "transition_charge": 8, "extra_noise_in_bright_pixels": 0.566,
- Tunned PSF
"increase_psf": true, "smeared_light_fraction": 0.175
- Original DL1a files
/fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/{particle}/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1/{}/
Random forest[edit]
- Dispnorm parameterisation
- Source-dependent
- - LSTCHAIN v0.9.4
- - Config file:
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/lstchain_src_dep_tailcut84_config_dispnorm_v0.9.4.json
- - path:
/fefs/aswg/workspace/arnau.aguasca/Analysis/models/20200609_XXXX/srcdep/v0.9.4/
- Source-independent
- - Processed with lstMCpipe using LSTCHAIN v0.9.3.
- - Path:
/fefs/aswg/data/models/20200629_prod5_trans_80/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1/
DL1 to DL2 data[edit]
Real data[edit]
- Source-dependent
- - LSTCHAIN v0.9.4
- - Config file:
//fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.4/lstchain_src_dep_tailcut84_config_dispnorm_v0.9.4.json
- Source-independent
- - LSTCHAIN v0.9.4
- - Config file:
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.4/lstchain_standard_config_tailcut84_dispnorm_v0.9.3.json
MC data[edit]
- Source-dependent
- - LSTCHAIN v0.9.4
- - Config file:
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/analysis_v0.9.4/lstchain_src_dep_tailcut84_config_dispnorm_v0.9.4.json
- Source-independent
- - Processed with lstMCpipe using LSTCHAIN v0.9.3.
- - Config file:
/fefs/aswg/data/mc/analysis_logs/20200629_prod5_trans_80/gamma/zenith_40deg/south_pointing/20220307_v0.9.3_prod5_trans_80_zen40az180_dl1ab_tuned_nsb_src1/off0.4deg/lstchain_config_NSBtuning.json
DL3 data selection[edit]
- Source-dependent
- - Quality cuts
"EventSelector": { "filters": { "intensity": [50, Infinity], "width": [0, Infinity], "length": [0, Infinity], "r": [0, 1], "wl": [0.1, 1], "leakage_intensity_width_2": [0, 0.2] } }, "DL3FixedCuts": { "fixed_gh_cut": 0.8, "fixed_alpha_cut": 15, "allowed_tels": [1] }
- Source-independent
- - Quality cuts
High-level analysis[edit]
- Source-dependent
- - IRF: point-like, single-offset
/fefs/aswg/workspace/arnau.aguasca/scripts/_configs/RSOph/XXXX
- - Produced DL3 files
/fefs/aswg/workspace/arnau.aguasca/XXXX
- Source-independent
Analysis results[edit]
- High level analysis performed with gammapy-v0.19
Alpha plot[edit]
- Filters in EventSelector applied:
"EventSelector": { "filters": { "intensity": [50, Infinity], "width": [0, Infinity], "length": [0, Infinity], "r": [0, 1], "wl": [0.1, 1], "leakage_intensity_width_2": [0, 0.2] } }
See section Crab Check to know more about the justification of the applied cuts. Stacked alpha plots:
Daily alpha plots:
- Energy threshold for the analysis
Theta plot[edit]
Stacked theta plots:
Daily theta plots:
- Energy threshold for the analysis
Spectral results[edit]
- Source-dependent
- Daily SEDs
- HESS and MAGIC comparison
- Daily MAGIC/LST-1 SEDs:
- Source-independent
- Daily SEDs
- HESS and MAGIC comparison
No daily SED can be plotted because the SED from LST-1 using gc=0.6 and tc=0.2 deg are not reliable.
Light curve results[edit]
- Source-dependent
- Source-independent
- - Notice that since the daily SEDs with quality cuts (gc=0.6 and tc=0.2 deg) are not reliable, the daily flux are computed with the stacked SED using data between 20210809-12!!!
- - No comparison with MAGIC light curve is done because the energy threshold using (gc=0.6 and tc=0.2 deg) is higher than 100 GeV.
Crab Check[edit]
Run selection using Crab_data_selection_notebook: https://indico.cta-observatory.org/event/3984/contributions/32878/attachments/20998/29572/Crab_data_selection_notebook.pdf
Threshold for the rate30_mask is set to 4.3. I exclude run 6016 because I obtain a strange SED at low energies.
Data reduction Specifications[edit]
- Source-dependent
Cuts at alpha cut = 15 deg are studied.
- Energy threshold for the analysis
- Source-independent
Cuts at theta cut = 0.2 deg are studied.
- Energy threshold for the analysis
I decide to use only the loose cuts in order to have a low energy threshold.
Spectral results[edit]
- Source-dependent
Conclusions: I decide to apply the following cuts: gammaness cut = 0.8, alpha cut = 15 deg and intensity = 50 p.e.
- Source-independent