Difference between revisions of "Crab Pulsar analysis v0.9.12 AlvaroMas"
(→Systematics tests) |
(→Phaseogram) |
||
(28 intermediate revisions by the same user not shown) | |||
Line 5: | Line 5: | ||
:- RA, Dec in deg (ICRS): 83.63, 22.01 | :- RA, Dec in deg (ICRS): 83.63, 22.01 | ||
+ | ==People involved in this analysis (LST-1 and new Fermi-LAT analysis)== | ||
+ | * Álvaro Mas-Aguilar | ||
+ | * Marcos López-Moya | ||
==Run selection== | ==Run selection== | ||
Line 295: | Line 298: | ||
* Evolution of the signal in time (without zd cut): | * Evolution of the signal in time (without zd cut): | ||
− | [[File: | + | [[File:time_evolution_lst.png|1000px]] |
* Fitting results | * Fitting results | ||
Line 321: | Line 324: | ||
[[File:fitting_sed_p2.png|800px]] | [[File:fitting_sed_p2.png|800px]] | ||
− | === LST-1 + Fermi-LAT joint fit === | + | === P1 LST-1 + Fermi-LAT joint fit === |
+ | |||
+ | ** Using a SubExponentialCutOffPL model: | ||
+ | |||
+ | [[File:P1_exponential_model_3.png|500px]] | ||
+ | [[File:Exponential_result_fit_P1.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 32.56''' | ||
+ | |||
+ | ** Using a SmoothBrokenPowerLaw model | ||
+ | [[File:SmoothBrokenPL_P1_2.png|500px]] | ||
+ | [[File:SmoothBPL_results_fit_P1.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 24.44''' | ||
+ | |||
+ | *P1 for E>10 GeV: | ||
+ | |||
+ | ** Using a LogParabola model | ||
+ | [[File:P1_logParabolaModel_2.png|500px]] | ||
+ | [[File:LogParabola_results_fit_P1.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 7.34''' | ||
+ | |||
+ | ** Using a PowerLaw model | ||
+ | [[File:P1_PLmodel_2.png|500px]] | ||
+ | [[File:PL_results_fit_P1.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 7.83''' | ||
+ | |||
+ | === P2 LST-1 + Fermi-LAT joint fit === | ||
+ | |||
+ | ** Using a SubExponentialCutOffPL model: | ||
+ | |||
+ | [[File:P2_Exponential_model.png|500px]] | ||
+ | [[File:Exponential_results_fit_P2.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 51.40''' | ||
+ | |||
+ | ** Using a SmoothBrokenPowerLaw model | ||
+ | [[File:SmoothBrokenPL_P2.png|500px]] | ||
+ | [[File:SmoothBPL_results_fit_P2.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 34.74''' | ||
+ | |||
+ | |||
+ | *P2 for E>10 GeV: | ||
+ | |||
+ | ** Using a LogParabola model | ||
+ | [[File:P2_logParabolaModel.png|500px]] | ||
+ | [[File:LogParabola_results_fit_P2.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 17.85''' | ||
+ | |||
+ | ** Using a PowerLaw model | ||
+ | [[File:P2_PLmodel.png|500px]] | ||
+ | [[File:PL_results_fit_P2.png|500px]] | ||
+ | |||
+ | '''Total stat: -2logL = 19.35''' | ||
=== LST-1+ Fermi-LAT energy calibration === | === LST-1+ Fermi-LAT energy calibration === | ||
Line 327: | Line 387: | ||
*P1 in left and P2 in right (Using SmoothBrokenPowerLaw model in all energy range) | *P1 in left and P2 in right (Using SmoothBrokenPowerLaw model in all energy range) | ||
− | [[File: | + | [[File:energy_factor_fermi_LST_P1_3.png|500px]] |
− | [[File: | + | [[File:energy_factor_LST_fermi_P2_3.png|500px]] |
*P1 in left and P2 in right (Using PowerLaw model at E>10 GeV) | *P1 in left and P2 in right (Using PowerLaw model at E>10 GeV) | ||
− | [[File: | + | [[File:energy_factor_fermi_LST_P1_PL_3.png|500px]] |
− | [[File: | + | [[File:energy_factor_LST_fermi_P2_PL_3.png|500px]] |
'''In all the cases the energy factor that minimize the chi2 value is below 5%''' | '''In all the cases the energy factor that minimize the chi2 value is below 5%''' | ||
Line 343: | Line 403: | ||
=== Systematics tests === | === Systematics tests === | ||
− | * Phaseogram and SED | + | ==== Phaseogram and SED for different samples ==== |
− | [[File: | + | |
+ | |||
+ | |||
+ | *Phaseogram Before August 2021 | ||
+ | [[File:histo_preAug.png|600px]] | ||
+ | |||
+ | |||
+ | '''sign(P1)/sqrt(Tobs) = 0.856 h^(-1/2)''' | ||
+ | |||
+ | '''sign(P2)/sqrt(Tobs) = 1.059 h^(-1/2)''' | ||
+ | |||
+ | |||
+ | *Phaseogram After August 2021 | ||
+ | [[File:histo_posAug.png|600px]] | ||
+ | |||
+ | '''sign(P1)/sqrt(Tobs) = 1.063 h^(-1/2)''' | ||
+ | |||
+ | '''sign(P2)/sqrt(Tobs) = 1.183 h^(-1/2)''' | ||
+ | |||
+ | *SED for P1: | ||
+ | [[File:spectra_P1_bothsamples.png|600px]] | ||
+ | |||
+ | '''Difference in spectral index of ~10% and flux 60% (lacking some statistics for first sample)''' | ||
+ | |||
+ | |||
+ | *SED for P2: | ||
+ | [[File:spectra_P2_bothsamples.png|600px]] | ||
+ | |||
+ | '''Difference in spectral index of ~2% and flux of 15%''' | ||
+ | ==== Phaseogram and SED with different efficiencies ==== | ||
+ | [[File:phaseogram_different_efficiencies.png|1000px]] | ||
− | * SED | + | * P1 SED: |
+ | [[File:SED_different_efficiencies.png|1000px]] | ||
+ | '''Relative maximum error of 3.07% in spectral index and 35.4% in flux.''' | ||
− | * Effect on SED due to shift on MC true energy | + | * P1 SED: |
+ | [[File:SED_different_efficiencies_P2.png|1000px]] | ||
+ | '''Relative maximum error of 7.36% in spectral index and 29.2% in flux.''' | ||
+ | |||
+ | ==== Effect on SED due to shift on MC true energy ===== | ||
** P1: | ** P1: | ||
− | [[File: | + | [[File:P1_energy_factor_SED_2.png|1000px]] |
+ | |||
+ | '''Relative maximum error of 1.01% in spectral index and 24.9% in flux.''' | ||
+ | |||
+ | **P2: | ||
+ | |||
+ | [[File:energy_factor_LST_P2.png|1000px]] | ||
+ | |||
+ | '''Relative maximum error of 0.45% in spectral index and 16.4% in flux.''' | ||
+ | |||
+ | ==== Final uncertainties ==== | ||
+ | |||
+ | **P1: | ||
+ | [[File:relative_error_index_P1.png|300px]] | ||
+ | [[File:relative_error_flux_P1.png|300px]] | ||
+ | [[File:total_uncertainty_P1.png|500px]] | ||
− | + | **P2: | |
+ | [[File:relative_error_index_P2.png|300px]] | ||
+ | [[File:relative_error_flux_P2.png|300px]] | ||
+ | [[File:total_uncertainty_P2.png|500px]] |
Latest revision as of 10:54, 23 February 2023
Contents
- 1 General information
- 2 People involved in this analysis (LST-1 and new Fermi-LAT analysis)
- 3 Run selection
- 4 MC information
- 5 DL1 data
- 6 DL2 data
- 7 DL3 data
- 8 DL3 pulsar data
- 9 High-level analysis
- 10 Results
General information[edit]
- Name of the source: Crab Pulsar
- Brief description of the source:
- - Object type : Pulsar
- - RA, Dec in deg (ICRS): 83.63, 22.01
People involved in this analysis (LST-1 and new Fermi-LAT analysis)[edit]
- Álvaro Mas-Aguilar
- Marcos López-Moya
Run selection[edit]
- Run selection with the use of the notebook from Abelardo Moralejo [1]
- Atmospheric transmission extracted from ELOG
- In total 403 runs selected, obstime 113.1 hours
- Summary of selection cuts:
- - Zenith < 60 deg
- - elapsed_time > 2 min
- - transmission_cut > 0.60
- - pedestal charge std dev < 1.9 p.e.
- - Cosmic rate > 3000 ev/s
- - Cosmic rate( > 10 p.e.) > 25-15 ev/s (depends on zd)
- - Cosmic rate( > 30 p.e.) > 3-4 ev/s (depends on zd)
- List of selected runs:
1 : 2020-09-18 : [2759] 2 : 2020-11-17 : [2914, 2919] 3 : 2020-11-18 : [2922, 2923, 2924, 2925, 2929, 2930, 2931, 2932, 2933, 2934] 4 : 2020-11-19 : [2949, 2950, 2959, 2961] 5 : 2020-11-20 : [2965, 2966, 2967, 2968, 2969, 2970, 2971, 2972, 2973, 2974, 2975, 2976, 2977] 6 : 2020-11-21 : [2988, 2989, 2990, 2991, 2992] 7 : 2020-11-22 : [3004, 3005, 3006, 3007, 3008, 3009, 3010, 3011, 3012] 8 : 2020-12-06 : [3087, 3088, 3089, 3090] 9 : 2020-12-07 : [3093, 3094, 3095, 3096] 10 : 2020-12-10 : [3143] 11 : 2020-12-11 : [3169, 3170, 3171] 12 : 2020-12-13 : [3231, 3232, 3233, 3234, 3235, 3236, 3237] 13 : 2020-12-14 : [3243, 3244, 3245] 14 : 2020-12-15 : [3264, 3265, 3266, 3267, 3268, 3269, 3270, 3271, 3272, 3273, 3274, 3275, 3276, 3277, 3278, 3279] 15 : 2020-12-17 : [3318, 3319, 3320, 3321] 16 : 2020-12-18 : [3328, 3329, 3330] 17 : 2020-12-19 : [3338, 3339, 3340] 18 : 2020-12-20 : [3355, 3356] 19 : 2020-12-21 : [3373] 20 : 2020-12-22 : [3382, 3383, 3384, 3385] 21 : 2021-02-11 : [3598, 3599, 3600, 3601] 22 : 2021-02-12 : [3615] 23 : 2021-02-13 : [3632, 3633, 3634, 3635, 3636, 3637, 3638, 3639] 24 : 2021-02-15 : [3672, 3673, 3674, 3675, 3676, 3677] 25 : 2021-02-16 : [3706, 3707, 3708, 3711, 3712] 26 : 2021-03-09 : [3925] 27 : 2021-03-11 : [3961] 28 : 2021-03-12 : [3980] 29 : 2021-03-13 : [4007, 4008] 30 : 2021-03-14 : [4031, 4032, 4033, 4034] 31 : 2021-03-15 : [4067, 4068, 4069, 4070, 4071, 4073, 4074] 32 : 2021-03-16 : [4086, 4087, 4088, 4089, 4090, 4091, 4092] 33 : 2021-03-17 : [4125, 4126] 34 : 2021-09-03 : [6012, 6013, 6014, 6016] 35 : 2021-09-04 : [6041, 6042, 6043, 6044, 6045] 36 : 2021-09-05 : [6069, 6070, 6071, 6072, 6073] 37 : 2021-09-13 : [6279] 38 : 2021-09-14 : [6301, 6302, 6304] 39 : 2022-02-04 : [6872, 6873, 6874, 6875] 40 : 2022-02-05 : [6892, 6893, 6894, 6895, 6896, 6897, 6898] 41 : 2022-02-23 : [7097, 7098, 7099, 7100, 7101, 7102, 7105, 7106] 42 : 2022-02-28 : [7133, 7136, 7137, 7138, 7139, 7140] 43 : 2022-03-01 : [7161, 7168, 7169, 7170, 7171, 7172] 44 : 2022-03-02 : [7195, 7196, 7197, 7199, 7200, 7201] 45 : 2022-03-03 : [7227, 7228, 7231, 7232, 7233, 7234, 7235, 7236, 7237, 7238] 46 : 2022-03-04 : [7253, 7254, 7255, 7256] 47 : 2022-03-05 : [7274, 7275, 7276, 7277, 7278, 7279, 7280, 7281] 48 : 2022-03-06 : [7301, 7302, 7303, 7304, 7305] 49 : 2022-03-25 : [7465] 50 : 2022-09-21 : [9274] 51 : 2022-09-29 : [9434, 9435, 9436, 9437, 9438] 52 : 2022-10-05 : [9596] 53 : 2022-10-25 : [9903, 9904, 9905, 9907] 54 : 2022-10-29 : [9996, 9997, 9998, 9999, 10001, 10002] 55 : 2022-11-19 : [10880, 10881, 10882, 10883] 56 : 2022-11-20 : [10909, 10910, 10911, 10912, 10913, 10914, 10915, 10916, 10917, 10918, 10919] 57 : 2022-11-21 : [10946, 10947, 10948, 10949, 10950] 58 : 2022-11-22 : [10981, 10982, 10983, 10984, 10985, 10986, 10987, 10988, 10989] 59 : 2022-11-24 : [11014, 11015, 11016, 11017, 11018, 11019] 60 : 2022-11-26 : [11087, 11088, 11089, 11090, 11091, 11092, 11093, 11094, 11095] 61 : 2022-11-27 : [11117, 11118, 11119, 11120, 11121, 11122, 11123, 11124, 11125] 62 : 2022-12-15 : [11373, 11374] 63 : 2022-12-16 : [11402] 64 : 2022-12-17 : [11427, 11428, 11429, 11430, 11431, 11432, 11433] 65 : 2022-12-18 : [11463, 11464, 11465, 11466, 11467, 11468, 11469, 11470, 11471, 11472, 11473] 66 : 2022-12-19 : [11486, 11487, 11488, 11489, 11490, 11491, 11492, 11493, 11510, 11511, 11512, 11513] 67 : 2022-12-21 : [11560, 11561, 11562, 11563] 68 : 2022-12-22 : [11575, 11576, 11577, 11578, 11579] 69 : 2022-12-23 : [11603, 11604, 11605, 11606] 70 : 2023-01-13 : [11625, 11626, 11627, 11628, 11630, 11631] 71 : 2023-01-15 : [11667, 11668, 11669, 11670, 11671, 11673, 11674, 11675, 11676] 72 : 2023-01-16 : [11681, 11682, 11683, 11684, 11685] 73 : 2023-01-17 : [11699, 11700, 11701, 11702, 11703, 11708, 11709] 74 : 2023-01-20 : [11738, 11739, 11740, 11741, 11742, 11743, 11744, 11745, 11746] 75 : 2023-01-21 : [11763, 11764, 11765, 11766, 11767, 11768, 11769, 11770] 76 : 2023-01-24 : [11828, 11829, 11830, 11831] 77 : 2023-01-26 : [11890, 11891, 11892, 11893] 78 : 2023-01-27 : [11923, 11926, 11927, 11928]
MC information[edit]
- - 20221027_v0.9.9_crab_tuned
- - AllSky MC using different test nodes for different runs depending on sky location.
- PSF and NSB tuned:
"image_modifier": { "increase_nsb": true, "extra_noise_in_dim_pixels": 1.27, "extra_bias_in_dim_pixels": 0.665, "transition_charge": 8, "extra_noise_in_bright_pixels": 2.08, "increase_psf": false, "smeared_light_fraction": 0 },
- Tuned DL1b MC:
- - Training sample: /fefs/aswg/data/mc/DL1/AllSky/20221027_v0.9.9_crab_tuned/TrainingDataset/
- - Testing sample (AllSky MC): /fefs/aswg/data/mc/DL1/AllSky/20221027_v0.9.9_crab_tuned/TestingDataset/
- Random Forests - Source Dependent:
- - General path: /fefs/aswg/workspace/seiya.nozaki/Crab_performance_paper/20221027_v0.9.9_crab_tuned/std/RF/trained_models/
- - Configuration file: /fefs/aswg/workspace/seiya.nozaki/Crab_performance_paper/20221027_v0.9.9_crab_tuned/std/DL2/lstchain_src_dep_config.json
- DL2 MC (testing only):
- - Souce-dependent
- - AllSky MC depending on the sky location.
- - General path: /fefs/aswg/workspace/seiya.nozaki/Crab_performance_paper/20221027_v0.9.9_crab_tuned/std/DL2_MC/
DL1 data[edit]
- - DL1a files produced by LSTOSA (lstchain v0.9.9)
- - lstchain v0.9 tailcut8-4
- - /fefs/aswg/data/real/DL1/{date}/v0.9/tailcut84/
DL2 data[edit]
- - Data before August 2021: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/DL2_preAug/
- - Data after August 2021: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/DL2_posAug/
IRFs[edit]
- - Point-like
- - IRFs for each MC node and for each intensity cut
- - IRF path before Aug2021: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/IRF/IRF_cut80/eff_0.7/
- - IRF path after Aug2021: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/IRF/IRF_cut50/eff_0.7/
- IRF for different MC efficiency for extra checks: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/IRF/IRF_cut{int_cut}/eff_{eff}/
DL3 data[edit]
- - General path for standard MC efficiency: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/DL3/eff_0.7/
- - General path for different MC efficiency: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/DL3/eff_{eff}/
- - Distribution of runs in AllSKy MC test nodes:
- mc_node = [10,102.199]
[2929,2930,2931,2950,2970,2971,2972,2973,2988,3095,3096,3273,3274,3275,3318,3319,3320,3338,9438,10001, 10002,10880,10909,10981,11087,11120,11121,11374,11463,11464,11491,11492,11576,11577,11625,11626]
- mc_node = [10,248.117]
[2914,2932,2933,2934,2974,2975,2976,2989,2990,2991,3004,3005,3006,3276,3277,3278,3279,3321,3328,3329, 3330,3339,3340,3355,3356,3598,3632,3672,3673,3674,3675,6872,6873,6874,6892,6893,7133,7161,7195,7196, 7197,7227,7228,7253,7274,10881,10882,10910,10911,10946,10947,10948,10982,10983,11014,11088,11089,11122, 11123,11402,11465,11466,11467,11493,11578,11579,11627,11628,11667]
- mc_node = [14.984,175.158]
[9436,9437,9907,9998,9999,10883,10912,10913,10949,10950,10984,10985,11015,11090,11091,11118,11119,11124, 11125,11373,11432,11433,11468,11469,11489,11490,11575,11630,11631,11668,11669,11681,11682,11699]
- mc_node = [23.63,100.758]
[2949,2968,2969,3093,3094,3271,3272,6304, 9434, 9435, 9596, 9905, 9996,9997, 11117,11430,11431,11487,11488]
- mc_node = [23.63,259.265]
[2977,2992,3007,3008,3231,3243,3373,3599,3600,3615,3633,3634,3676,3677,3706,3707,4067,4086,6875,6894,7097, 7098,7099,7199,7231,7254,7255,7256,7275,10914,10915,10986,10987,11016,11017,11092,11093,11470,11471,11560, 11561,11562,11603,11604,11670,11671,11683,11700,11701,11738,11739,11763]
- mc_node = [32.059,102.217]
[2925,2966,2967,3090,3268,3269,3270,6016,6045,6072,6073,6302,9903,9904,11428,11429,11486]
- mc_node=[32.059,248.099]
[2959,3009,3010,3169,3232,3233,3244,3245,3601,3635,3636,3708,4068,4069,4087,4088,6895,6896,7100,7101,7136,7137, 7200,7201,7232,7233,7234,7276,7277,7278,7301,7302,10916,10917,10918,10988,10989,11018,11019,11094,11095,11472, 11473,11563,11605,11606,11673,11674,11684,11685,11702,11703,11740,11741,11742,11764,11765,11766,11923]
- mc_node = [43.197,87.604]
[2923,2924,2965,3088,3089,3266,3267,6043,6044,6071,6279,6301,6070,9274,11427]
- mc_node = [43.197,262.712]
[2919,2961,3011,3012,3143,3170,3171,3234,3382,3383,3384,3637,3638,3639,3711,3925,4007,4008,4031,4032,4070,4071, 4089,4090,6897,7102,7138,7139,7168,7169,7235,7236,7237,7238,7279,7280,7303,7304,7465,10919,11510,11511,11675, 11676,11743,11744,11767,11768,11828,11829,11890,11891,11926]
- mc_node = [52.374,110.312]
[2759,3264,3265,2922,3087,6013,6014,6041,6042,6069]
- mc_node = [52.374,301.217]
[3235,3236,3385,3712,3961,3980,4033,4034,4091,4125,4126,4073,4092,6898,7105,7106,7140,7170,7171,7281,7305,11512,11513, 11708,11709,11745,11746,11769,11770,11830,11831,11892,11893,11927,11928]
- mc_node = [60.528,99.126]
[6012]
- mc_node = [60.528,251.19]
[3237,4074,7172]
- Fixed cuts (before August 2021):
"intensity": [80, Infinity], "width": [0, Infinity], "length": [0, Infinity], "r": [0, 1], "wl": [0.1, 1], "leakage_intensity_width_2": [0, 1.0], "event_type": [32, 32]
- Fixed cuts (after August 2021):
"intensity": [50, Infinity], "width": [0, Infinity], "length": [0, Infinity], "r": [0, 1], "wl": [0.1, 1], "leakage_intensity_width_2": [0, 1.0], "event_type": [32, 32]
- Global gammaness and alpha cuts optimized on MC gamma efficiency of 70%, point-like source assumption
gh-efficiency 0.7 alpha-containment 0.7
DL3 pulsar data[edit]
- - Add phases using PINT-pulsar tools for LST-1 (https://github.com/alvmas/PulsarTimingAnalysis)
- - Ephemeris file: /home/alvaro.mas/software/Pulsar_analysis/data/all.gro
- - General path for standard MC efficiency: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/DL3_pulsar/eff_0.7/
- - General path for different MC efficiency: /fefs/aswg/workspace/alvaro.mas/data/real/Crab/v0.9.9_final/DL3_pulsar/eff_{eff}/
High-level analysis[edit]
1D Spectral analysis[edit]
- Performed with gammapy-v0.20.1
energy_axis = MapAxis.from_energy_bounds( 0.01, 10, nbin=40, per_decade=False, unit="TeV", name="energy" ) energy_axis_true = MapAxis.from_energy_bounds( 0.05, 100, nbin=100, per_decade=False, unit="TeV", name="energy_true" )
spectral_points_binning e_min, e_max = 0.02, 0.7 nbins = 8 logspace sqrt_ts>1.5
- Phase Regions:
Bkg: [0.52,0.87] P1: [0,0.026,0.983,1] P2: [0.377,0.422] P1+P2: [0,0.026,0.377,0.422, 0.983,1] P3: [0.08,0.24]
- Spectral fitting of stacked LST dataset
- Performed for point-like assumption
- Stacked analysis
- LST-1 data alone: Power-law spectral model
- Fermi + LST-1 data: Power-Law Spectral Model, ExponentialCutOff, LogParabola
Results[edit]
Phaseogram[edit]
- Phaseogram with all data
- Phaseogram with zd<35
- Phaseogram with zd>35
- Phaseogram in different energy bins:
- Evolution of the signal in time (without zd cut):
- Fitting results
- P1/P2 differential ratio (with Fermi-LAT). Until 200 GeV due to large uncertainties
- P1/P2 integral ratio (with Fermi-LAT).
LST-1 only fit and SED (zd<50)[edit]
- P1
- P2
P1 LST-1 + Fermi-LAT joint fit[edit]
- Using a SubExponentialCutOffPL model:
Total stat: -2logL = 32.56
- Using a SmoothBrokenPowerLaw model
Total stat: -2logL = 24.44
- P1 for E>10 GeV:
- Using a LogParabola model
Total stat: -2logL = 7.34
- Using a PowerLaw model
Total stat: -2logL = 7.83
P2 LST-1 + Fermi-LAT joint fit[edit]
- Using a SubExponentialCutOffPL model:
Total stat: -2logL = 51.40
- Using a SmoothBrokenPowerLaw model
Total stat: -2logL = 34.74
- P2 for E>10 GeV:
- Using a LogParabola model
Total stat: -2logL = 17.85
- Using a PowerLaw model
Total stat: -2logL = 19.35
LST-1+ Fermi-LAT energy calibration[edit]
- P1 in left and P2 in right (Using SmoothBrokenPowerLaw model in all energy range)
- P1 in left and P2 in right (Using PowerLaw model at E>10 GeV)
In all the cases the energy factor that minimize the chi2 value is below 5%
Lightcurve[edit]
Systematics tests[edit]
Phaseogram and SED for different samples[edit]
- Phaseogram Before August 2021
sign(P1)/sqrt(Tobs) = 0.856 h^(-1/2)
sign(P2)/sqrt(Tobs) = 1.059 h^(-1/2)
- Phaseogram After August 2021
sign(P1)/sqrt(Tobs) = 1.063 h^(-1/2)
sign(P2)/sqrt(Tobs) = 1.183 h^(-1/2)
- SED for P1:
Difference in spectral index of ~10% and flux 60% (lacking some statistics for first sample)
- SED for P2:
Difference in spectral index of ~2% and flux of 15%
Phaseogram and SED with different efficiencies[edit]
- P1 SED:
Relative maximum error of 3.07% in spectral index and 35.4% in flux.
- P1 SED:
Relative maximum error of 7.36% in spectral index and 29.2% in flux.
Effect on SED due to shift on MC true energy =[edit]
- P1:
Relative maximum error of 1.01% in spectral index and 24.9% in flux.
- P2:
Relative maximum error of 0.45% in spectral index and 16.4% in flux.
Final uncertainties[edit]
- P1:
- P2: