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Total MACS at 30keV:	63.8	±	5.3	mb
Partial c.s. to isomer:	4.7	±	0.4	mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	63.8 ± 5.3	-	4.7 ± 0.4
0.0	64.6 ± 5.3	-	4.7 ± 0.4

(Version 0.0 corresponds to Bao et al.)

New rec. value is normalized value (f=1.04) from jendl40. Uncertainty of 8.2 % is from Bee91. The isomeric ratio at kT= 25 keV is IR=0.073, assumed same ratio for kT= 30 keV.
Last review: July 2013

original	renorm.	year	type	Comment	Ref
71.6 ± 5.9 kT= 25 keV	63.8 ± 5.3	1991	c	VdG, Act., 1/v(kT), Au:RaK88; en. dep. from jendl40	Bee91
61 ± 4	60	1983	c	VdG, Act., 1/v(kT), Au:657mb(25keV)	BKR83
47.4		2011	e	ENDF/B-VII.1	endfb71
61.6		2011	e	JENDL-4.0	jendl40
85.0		2004	e	JEFF-3.1	jeff31
52.2		2002	e	JENDL-3.3	jendl33
36		1971	s		AGM71
67.4		2005	t	MOST 2005	Gor05
72.8		2002	t	MOST 2002	Gor02
74		2000	t	NON-SMOKER	RaT99
65		1983	t		BKR83
75		1981	t		Har81
91		1976	t		HWF76
Partial cross section to 133mXe:
4.7 ± 0.4		1991	c	VdG, Act., 1/v(kT), Au:RaK88	Bee91

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
s	Semiempirical estimates given in the reference
t	Theoretical value

Energy	5keV	8keV	10keV	15keV	20keV	25keV	30keV	40keV	50keV	60keV	80keV	100keV
MACS	238.3	-	138.2	101.9	83.1	71.6 ± 5.9	63.8 ± 5.3	53.9	47.9	43.9	38.9	36.0
Xfactor	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	0.99
SEF	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00
Rate	1.41	-	1.16	1.05	0.99	0.95	0.93	0.90	0.90	0.90	0.92	0.96

MACS:
Reference: jendl40,Bee91
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

	132Ba 0.101 397 mb 133Ba 10.52 a β+ 134Ba 2.417 176 mb 135Ba 6.592 455 mb 136Ba 7.854 61.2 mb 131Cs 9.69 d β+ 132Cs 6.48 d β+ 133Cs 100 509 mb 134Cs 2.07 a 664 mb, β- 135Cs 2.30 Ma 198 mb, β- 130Xe 4.071 141 mb 131Xe 21.232 340 mb 132Xe 26.909 64.6 mb 133Xe 5.24 d 127 mb, β- 134Xe 10.436 20.2 mb 129I 15.70 Ma 441 mb, β- 130I 12.36 h β- 131I 8.02 d β- 132I 2.29 h β- 133I 20.80 h β- 128Te 31.74 44.4 mb 129Te 1.16 h β- 130Te 34.08 14.7 mb 131Te 25.00 m β- 132Te 3.20 d β-

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