Radiative rates for forbidden M1 and E2 transitions of astrophysical interest in doubly ionized iron-peak elements

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Table A.9

Comparison of transition probabilities for M1 and E2 lines from our calculations (HFR and AUTOS) and previous works in Sc III. A[B] denotes A × 10^B.

Lower level	Upper level	λ (nm)	A(M1+E2) (s^-1)
			Type	HFR	AUTOS	Others


3d ²D_3/2	3d ²D_5/2	50 597.04	M1+E2	8.36[–05]	8.33[–05]	8.32[–05]^a, 8.32[-05]^b,
						8.24[–05]^c,8.33[–05]^d
3d ²D_3/2	4s ²S_1/2	391.55	M1+E2	7.67	8.71	8.21^a, 7.95^b,
						7.86^c, 7.83^d
3d ²D_5/2	4s ²S_1/2	394.61	E2	11.07	12.56	11.9^a, 11.5^b,
						11.41^c, 11.40^d

Reference. and

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