Exploring molecular complexity with ALMA (EMoCA): Detection of three new hot cores in Sagittarius B2(N)

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Table 5

Statistics of the lines detected toward the three new hot cores.

Source	N_l ^a	n_l ^b	N_species ^c	N_iso ^c	N_exc ^c	U-lines^d
		(GHz^-1)				(%)

N3	714	31	23	20	19	9
N4	249	11	22	13	9	11
N5	508	22	25	16	12	7

Notes.

^(a)

Total number of emission lines detected above the 7σ level (rms ~ 3 mJy/beam) excluding setup 3.

^(b)

Line density above 7σ, excluding setup 3.

^(c)

Number of identified molecules, less abundant isotopologs, and vibrationally excited states.

^(d)

Fraction of remaining unidentified lines above 7σ.

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