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Total MACS at 30keV:

224.7

±

9.1

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	224.7 ± 9.1	-	-
0.0	180 ± 10	-	-

(Version 0.0 corresponds to Bao et al.)

New rec. value is average from recent evaluations (endfb71,jendl40) which fit the data of NIO08 nicely. Uncertainty is from deviation of both evaluations plus 4% as in NIO08.
Last review: June 2013

original	renorm.	year	type	Comment	Ref
235 ± 9 E(n)= 30 (5) keV		2008	c	Pelletron, TOF, Au:ENDF/B-VI and MaG67b	NIO08
194 ± 10	180	1989	r	VdG, TOF, 6Li, Au:B-V+KKP85	TBI89
247 ± 54		1967	c	VdG, TOF, 181Ta:762mb	MaG67a
225.3		2011	e	ENDF/B-VII.1	endfb71
224.8		2011	e	JENDL-4.0	jendl40
224.8		2004	e	JEFF-3.1	jeff31
260 ± 40		1971	e		AGM71
240		2005	t	MOST 2005	Gor05
216		2002	t	MOST 2002	Gor02
222		2000	t	NON-SMOKER	RaT99
263		1981	t		Har81
279		1976	t		HWF76

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
r	Recalculated for kT = 30keV with the code described in Ref. 2 after renormalizing the original data to updated standard cross sections
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	707.9 ± 29.2	-	488.8 ± 21.7	375.8 ± 16.8	305.9 ± 13.3	258.6 ± 10.9	224.7 ± 9.1	179.8 ± 7.8	151.7 ± 7.1	132.7 ± 6.6	109.0 ± 5.9	95.2 ± 5.5
Xfactor	0.98	0.90	0.84	0.69	0.56	0.47	0.39	0.29	0.23	0.19	0.15	0.13
SEF	1.00	1.00	1.01	1.03	1.06	1.11	1.16	1.26	1.34	1.40	1.49	1.56
Rate	4.21	-	4.13	3.97	3.86	3.81	3.80	3.80	3.81	3.82	3.87	3.94

MACS:
Reference: NIO08,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

	119Te 16.05 h β+ 120Te 0.09 538 mb 121Te 19.16 d β+ 122Te 2.55 295 mb 123Te 0.89 832 mb 118Sb 3.60 m β+ 119Sb 1.59 d β+ 120Sb 15.89 m β+ 121Sb 57.21 532 mb 122Sb 2.72 d 894 mb, β- 117Sn 7.68 318.8 mb 118Sn 24.22 62.1 mb 119Sn 8.59 180 mb 120Sn 32.58 36 mb 121Sn 1.13 d 167 mb, β- 116In 14.10 s β- 117In 43.20 m β- 118In 5.00 s β- 119In 2.40 m β- 120In 3.08 s β- 115Cd 2.23 d 601 mb, β- 116Cd 7.49 59 mb 117Cd 2.49 h β- 118Cd 50.30 m β- 119Cd 2.69 m β-

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