Luminous efficiency of meteors derived from ablation model after assessment of its range of validity

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Table E.1

τ of the simulated light curves based on the four events listed in Table 1.

Event	Data included in%	τ in%

		Missing end	Missing beginning	Missing beginning and end
1 Dec. 2016 (faint and slow)	100	0.68	0.68	0.68
	95	0.69	0.27	0.46
	90	0.71	1.80	0.46
	85	0.74	1.40	0.49
	80	0.72	1.80	0.50
	75	0.67	1.20	0.54
	70	0.58	0.91	0.55
	60	0.47	0.71	0.63
	50	0.41	0.67	0.70
21 Sep. 2017 (bright and fast)	100	35.65	35.65	35.65
	95	35.99	23.05	15.96
	90	39.99	37.06	15.69
	85	35.88	52.92	16.30
	80	25.09	43.53	17.04
	75	22.69	38.46	17.43
	70	20.59	35.77	18.45
	60	16.17	34.82	20.87
	50	14.21	34.85	22.74
18 Aug. 2018 (faint and fast)	100	0.42	0.42	0.42
	95	0.42	0.26	0.73
	90	0.42	0.35	0.35
	85	0.41	0.38	0.35
	80	0.40	0.44	0.34
	75	0.38	0.43	0.35
	70	0.37	0.40	0.35
	60	0.34	0.39	0.36
	50	0.33	0.40	0.37
16 Oct. 2019 (bright and slow)	100	0.73	0.73	0.73
	95	0.73	4.39	1.76
	90	0.73	0.75	0.82
	85	0.72	0.58	0.80
	80	0.71	0.77	0.77
	75	0.69	0.70	0.75
	70	0.68	0.62	0.73
	60	0.76	0.56	0.71
	50	1.63	0.65	0.71

Notes. The values are also visualized in Fig. E.1 (missing end), Fig. E.2 (missing beginning), and Fig. E.3 (missing beginning and end). The percentage of the light curve that is included in the simulated data is given (100%, 95%, 90%, 85%, 80%, 75%, 70%, 60%, and 50%, respectively) for three cases: Missing parts at the end of the trajectory, missing parts at the beginning of the trajectory, as well as missing parts at the beginning and end of the trajectory.

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