Observations of carbon radio recombination lines with the NenuFAR telescope - I. Cassiopeia A and Cygnus A

Open Access

Table C.1

Summary of the parameters of the stacking procedure for each source.

Source	Frequency range	Average quantum number	Number of lines in the preselection	Effective number of lines in the stack
	79.11 - 84.41	431	10	7
	73.91 - 79.11	441	10	7
	69.16 - 73.91	451	10	10
	64.81 - 69.16	461	10	7
	60.81 - 64.81	471	10	8
	57.14 - 60.81	481	10	8
	53.76 - 57.14	491	10	8
	50.63 - 53.76	501	10	8
	47.75 - 50.63	511	10	8
	45.08 - 47.75	521	10	7
	42.61 - 45.08	531	10	8
	40.31 - 42.61	541	10	9
	38.18 - 40.31	551	10	9
Cas A	36.19 - 38.18	561	10	6
	34.34 - 36.19	571	10	8
	32.61 - 34.34	581	10	7
	31.00 - 32.61	591	10	8
	29.49 - 31.00	601	10	8
	26.76 - 29.49	616	20	19
	24.35 - 26.76	636	20	18
	22.22 - 24.35	656	20	17
	20.34 - 22.22	676	20	17
	18.66 - 20.34	696	20	16
	16.47 - 18.66	721	30	24
	14.61 - 16.47	751	30	27
	13.02 - 14.61	781	30	29
	11.65 - 13.02	811	30	30
	10.47 - 11.65	841	30	29
	69.16 - 84.41	441	30	30
	57.14 - 69.16	471	30	30
	47.75 - 57.14	501	30	30
	40.31 - 47.75	531	30	27
	34.34 - 40.31	561	30	22
Cyg A	29.49 - 34.34	591	30	26
	24.35 - 29.49	626	40	38
	20.34 - 24.35	666	40	34
	17.16 - 20.34	706	40	35
	14.05 - 17.16	751	50	36
	11.65 - 14.05	801	50	44

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