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

Open Access

Table B.1

Linear ranges and coarseness of the grids explored to infer physical parameters.

Parameter	Start	Stop	Step	Final precision
T_e [K]	10	5000	10	1
n_e [cm⁻³]	0.01	1	0.01	0.001
T₀ [K]	100	5000	500	100
υ_t [km s⁻¹]	1	20	1	0.1
L [pc]	L_min ^(a)	L_max ^(a)	1	0.5

Notes. The left column indicates the parameters of the broad initial grid, the columns marked ’start’ and ’stop’ define the range, while ’step’ defines the coarseness and the last column gives the precision of the finest grid.

^(a) The edges of the exploratory range are determined through cloud identification as L_min = L_prior - 10 pc and L_max = L_prior + 10 pc

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