1ES0647+250 Analysis with lstchain v0.9.12 E. Pons
Contents
1ES 0647+250 Analysis with lstchain v0.9.12 E. Pons
General information
- Name of the source: 1ES 0647+250
- Brief description of the source:
- Object type : AGN
- Redshift (z) : 0.41
- HBL
- RA: 6 50 46.49 (hh mm ss), Dec: +25 2 59.62 (dd mm ss)
- RA, Dec in deg (ICRS): 102.69370933, 25.04989555
- Analysis by Estelle Pons (LAPP - estelle.pons@lapp.in2p3.fr)
Dataset (< 2022-05-24)
- Number of selected observations : 28
- Runs: 3281 - 3364
- Date range: 2020-12-16 to 2020-12-21
obsids:
[3281 3282 3283 3284 3285 3287 3288 3331 3332 3333 3334 3335 3341 3342 3343 3344 3345 3346 3347 3348 3357 3358 3359 3360 3361 3362 3363 3364]
DL1 data
DL1 files produced by LSTOSA (lstchain v0.9)
- original real DL1a data
/fefs/aswg/data/real/DL1/{Date}/v0.9/tailcut84/
DL1 to DL2
- Random Forest
Standard ‘un-tuned’ production for processing standard AGN data, with lstchain v0.9.12 standard settings (az instead of sin(az) in training features).
/fefs/aswg/data/models/AllSky/20230127_v0.9.12_base_prod_az_tel/dec_2276
- DL2 data
/fefs/aswg/workspace/estelle.pons/1ES0647/DL2/{Date}/v0.9.12/tailcut84
NB: The lstchain config file from the RF production is specified for lstchain_dl1_to_dl2
Example:
lstchain_dl1_to_dl2 -f /fefs/aswg/data/real//DL1/20201219/v0.9/tailcut84/dl1_LST-1.Run03348.0012.h5 --output-dir /fefs/aswg/workspace/estelle.pons/1ES0647//DL2/20201219/v0.9.12/tailcut84/ --path-models /fefs/aswg/data/models/AllSky/20230127_v0.9.12_base_prod_az_tel/dec_2276/ --config /fefs/aswg/data/models/AllSky/20230127_v0.9.12_base_prod_az_tel/dec_2276/lstchain_config.json
DL2 to DL3
- DL3 cuts: source-independent analysis & global cuts:
- gh_cut = 0.7
- theta_cut = 0.2
- MC DL2 files used to produce IRF
/fefs/aswg/data/mc/DL2/AllSky/20230414_v0.9.13_dec_931_az_tel/TestingDataset/dec_931
The closest node compared to the telescope pointing position is then selected for each run to create the corresponding IRF.
Example:
lstchain_create_irf_files -g /fefs/aswg/data/mc/DL2/AllSky/20230414_v0.9.13_dec_931_az_tel/TestingDataset/dec_931/node_theta_32.059_az_248.099_/dl2_20230414_v0.9.13_dec_931_az_tel_node_theta_32.059_az_248.099__merged.h5 -o /fefs/aswg/workspace/estelle.pons/PG1553/IRF/allsky/irf_20230414_v0.9.13_dec_931_az_tel_dec_931_node_theta_32.059_az_248.099_ghcut0.7_run8787.fits.gz --point-like --global-theta-cut 0.2 --global-gh-cut 0.7
- DL3 data
/fefs/aswg/workspace/estelle.pons/PG1553/DL3/lstchain/v0.9.13/point_like/offset0.4/ghcut0.7/{Date}
Example:
lstchain_create_dl3_file -d /fefs/aswg/workspace/estelle.pons/PG1553//DL2/20220617/v0.9.13/tailcut84/dl2_LST-1.Run08787.h5 -o /fefs/aswg/workspace/estelle.pons/PG1553/DL3/lstchain/v0.9.13/point_like/offset0.4/ghcut0.7/20220617 --input-irf /fefs/aswg/workspace/estelle.pons/PG1553/IRF/allsky/irf_20230414_v0.9.13_dec_931_az_tel_dec_931_node_theta_32.059_az_248.099_ghcut0.7_run8787.fits.gz --source-name PG1553+113 --source-ra " 238.92935002022deg" --source-dec " 11.19010156943deg" --global-gh-cut 0.7 --gzip
gammapy analysis parameters
- gammapy version v1.0.1
- DL4 datasets
- on_radius = 0.2 deg / exclusion_radius = 0.35 deg
- Reflected Regions Background method
- Safe Energy mask:
- MapDataset: methods=["offset-max"], offset_max=4 deg
- SpectrumDataset: NO safe mask
- Energy axes:
- True: 10 GeV to 10 TeV with 5 bins per decade
- Reco: 10 GeV to 40 TeV with 10 bins per decade
- DL5 datasets
- Spectral analysis
- Joint fit
- Energy axes Flux Points: 10 GeV to 10 TeV with 5 bins per decade
- Reference energy: pivot energy from a power-law fit = 0.12 TeV
- SED fitting: best fit between power-law + EBL (Dominguez), log-parabol + EBL, exponantial cutoff power-law + EBL
- Spectral analysis
Analysis Results
Livetime : 8.17 h
Significance : 7.33 sigma
Excess : 1711.1
S/B : 0.040
Rate : 3.49 per min
Fluxes (for spectral model PL+EBL)
Energy flux (0.01 TeV-10.0 TeV) = 7.740e-11 pm 3.602e-11 TeV / (cm2 s) Integral flux (0.01 TeV-10.0 TeV) = 3.489e-09 pm 2.099e-09 1 / (cm2 s) Integral flux (100 GeV-10.0 TeV) = 5.376e-11 pm 9.360e-12 1 / (cm2 s)
Count Map
Theta2 plot
SED
- power-law + EBL = best fit
- log-parabola & log-parabola + EBL