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Total MACS at 30keV:

532

±

16

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
0.0	532 ± 16	-	-

(Version 0.0 corresponds to Bao et al.)

Recommended value is from KSW93. MACS vs. kT table normalized to average of recent evaluations (endfb71,jendl40). Uncertainty is deviation between both evaluations plus 3 % uncertainty from KSW93.
Last review: July 2013

original	renorm.	year	type	Comment	Ref
532 ± 16		1993	c	VdG, Act., 1/v(kT), Au:RaK88	KSW93
1096 ± 165 E(n)= 24 (5) keV		1968	c	VdG, Act., 7Li(p,n), 235U(n,f)	TKK68
492.2		2011	e	ENDF/B-VII.1	endfb71
519.8		2011	e	JENDL-4.0	jendl40
522.1		2004	e	JEFF-3.1	jeff31
522.1		2002	e	JENDL-3.3	jendl33
740 ± 100		1971	e		AGM71
417		2005	t	MOST 2005	Gor05
523		2002	t	MOST 2002	Gor02
697		2000	t	NON-SMOKER	RaT99
603		1981	t		Har81
837		1976	t		HWF76
Partial cross section to 122gSb:
1035 ± 100 E(n)= 25 (5) keV		1972	c	Sb-Be, Act., 1/v(E), 127I:832mb(24keV)	LRR72
Partial cross section to 122mSb:
2.0 ± 0.3 E(n)= 25 (5) keV		1972	c	Sb-Be, Act., 1/v(E), 127I:832mb(24keV)	LRR72

Original:MACS [<σ v>/v_T] (mb) for kT=30 keV, based on the published cross sections except where indicated otherwise.
Renorm:MACS [<σ v>/v_T] (mb) for kT=30 keV for which the reference or standard cross section was meanwhile improved.
Type: The letters and numbers in the column labelled 'type' give information on how the cross section has been obtained:

c	Directly quoted from the reference itself
e	Evaluated value taken directly from the reference
t	Theoretical value

Energy	5keV	8keV	10keV	15keV	20keV	25keV	30keV	40keV	50keV	60keV	80keV	100keV
MACS	1320 ± 198	-	998 ± 88	812 ± 58	686 ± 47	597 ± 38	532 ± 16	445 ± 17	389 ± 17	349 ± 22	298 ± 28	266 ± 31
Xfactor	1.00	0.98	0.97	0.90	0.83	0.77	0.72	0.65	0.61	0.57	0.53	0.50
SEF	1.00	1.00	1.00	1.00	1.00	0.99	1.00	1.00	1.01	1.01	1.03	1.04
Rate	7.84	-	8.38	8.33	8.11	7.89	7.71	7.48	7.36	7.29	7.28	7.36

MACS:
Reference: KSW93,endfb71,jendl40
Procedure: 'e+t' (The MACS from kT=5 keV to 100 keV are derived from calculated cross sections, which are then normalized to experimental data, e.g. to the values at kT=25 keV obtained in activation measurements. In these cases the uncertainties should be linearly increased below 25 and above 30 keV to reach about 30% at the extreme kT values.)
Year: 2013

X-factor:
Reference: Rau12
Year: 2012

SEF (Stellar enhancement factor):
Reference: Rau09
Year: 2009
Comment:

Rate:
Reaction rate N_A<σv> given in 10⁷ cm³/mole/s, including SEF

	121I 2.12 h β+ 122I 3.63 m β+ 123I 13.23 h β+ 124I 4.18 d β+ 125I 59.40 d β+ 120Te 0.09 538 mb 121Te 19.16 d β+ 122Te 2.55 295 mb 123Te 0.89 832 mb 124Te 4.74 155 mb 119Sb 1.59 d β+ 120Sb 15.89 m β+ 121Sb 57.21 532 mb 122Sb 2.72 d 894 mb, β- 123Sb 42.79 303 mb 118Sn 24.22 62.1 mb 119Sn 8.59 180 mb 120Sn 32.58 36 mb 121Sn 1.13 d 167 mb, β- 122Sn 4.63 21.9 mb 117In 43.20 m β- 118In 5.00 s β- 119In 2.40 m β- 120In 3.08 s β- 121In 23.10 s β-

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