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Total MACS at 30keV:

1333

±

133

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	1333 ± 133	-	-
0.0	1320 ± 84	-	-

(Version 0.0 corresponds to Bao et al.)

New rec. value is value from JaK95 (using gamma-line intensities of NDS12) and renormalized with recent evaluations of endfb71 and jendl40. Uncertainty is 9.6 % as in JaK95 plus deviation of both evaluations.
Last review: September 2013

original	renorm.	year	type	Comment	Ref
1320 ± 84	1333 ± 133	1995,2013	r	VdG, Act., 1/v(kT), Au:RaK88; gamma intensities from NDS12; energy dep. from endfb71 and jendl40	JaK95
1320 ± 84		1995	c	VdG, Act., 1/v(kT), Au:RaK88	JaK95
1136		2011	e	ENDF/B-VII.1	endfb71
1264		2011	e	JENDL-4.0	jendl40
1339		2004	e	JEFF-3.1	jeff31
1141		2002	e	JENDL-3.3	jendl33
1107		2005	t	MOST 2005	Gor05
1452		2002	t	MOST 2002	Gor02
1374		2000	t	NON-SMOKER	RaT99
2088		1981	t		Har81
1730		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:

r	Recalculated for kT = 30keV with the code described in Ref. 2 after renormalizing the original data to updated standard cross sections
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	4258 ± 684	-	2649 ± 347	2044 ± 232	1711 ± 176	1492 ± 144	1333 ± 133	1109 ± 114	954 ± 99	839 ± 87	676 ± 70	566 ± 58
Xfactor	1.00	1.00	1.00	0.99	0.97	0.94	0.89	0.79	0.70	0.61	0.47	0.38
SEF	1.00	1.00	1.00	1.00	1.00	0.99	0.98	0.97	0.95	0.93	0.91	0.89
Rate	2.53	-	2.22	2.10	2.02	1.96	1.91	1.80	1.69	1.61	1.45	1.34

MACS:
Reference: JaK95,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 10⁸ cm³/mole/s, including SEF

	155Tb 5.32 d β+ 156Tb 5.35 d β+ 157Tb 71.01 a β+ 158Tb 179.99 a β+ 159Tb 100 1580 mb 154Gd 2.18 1028 mb 155Gd 14.8 2648 mb 156Gd 20.47 615 mb 157Gd 15.65 1369 mb 158Gd 24.84 324 mb 153Eu 52.19 2780 mb 154Eu 8.59 a 4420 mb, β- 155Eu 4.75 a 1320 mb, β- 156Eu 15.19 d β- 157Eu 15.18 h β- 152Sm 26.75 473 mb 153Sm 1.93 d 1095 mb, β- 154Sm 22.75 206 mb 155Sm 22.30 m β- 156Sm 9.40 h β- 151Pm 1.18 d β- 152Pm 4.12 m β- 153Pm 5.25 m β- 154Pm 2.68 m β- 155Pm 41.50 s β-

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