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Total MACS at 30keV:

0.0139

±

0.0019

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	0.0139 ± 0.0019	-	-
0.0	0.00886 ± 0.00080	-	-

(Version 0.0 corresponds to Bao et al.)

Fit to all existing high-energy data (OIN08, MSG96, Vau68) including optimized resonance parameters and normalized p-wave DRC. p-wave DRC parameterized as sigma(p)= 44.86*sqrt(E) - 9.7*E^1.2 (E in keV and sigma in micro-barn). Average uncertainty from OIN08, MSG96 is 14 % which was taken also for the recommended value.
Last review: Jan. 4th, 2013

original	renorm.	year	type	Comment	Ref
0.0085-0.0119 E(n,av.)= 42-64 keV		2008	c	Pelletron, TOF, Au:ENDF/B-VI and MaG67b	OIN08
0.00793 ± 0.00070 kT= 25 keV		1996	c	VdG, Act., 86Kr(n,gamma): Bee91,BRV91	MSG96
0.0138-0.096 E(n,av.)= 129-370 keV		1996	c	VdG, Act., Au:RaK88	MSG96
0.0153		1996	t	DRC calculations plus resonances	MSG96
0.0145	0.0116	2012	t	norm. p-wave DRC calc.: sigma(p)= 44.86*sqrt(E) - 9.7*E^1.2	MSG96
0.0029		2003	t	JEFF3.0/A; missing res. at 152 keV	jeff30A
2.74		2002	t	MOST 2002	Gor02
2.35		2005	t	MOST 2005	Gor05

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
t	Theoretical value

Energy	5keV	8keV	10keV	15keV	20keV	25keV	30keV	40keV	50keV	60keV	80keV	100keV
MACS	0.0057	-	0.0078	0.0094	0.0109	0.0124	0.0139 ± 0.0012	0.017	0.0207	0.0252	0.0362	0.0481
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	3.46	-	6.70	9.89	13.24	16.85	20.69	29.21	39.77	53.03	87.97	130.69

MACS:
Reference: MSG96,OIN08,Vau68
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: 2012

X-factor:
Please note: X-factors for this element have not been calculated but are expected to be close to 1.

SEF (Stellar enhancement factor):
Reference: Rau09
Year: 2009
Comment:
Please note: SEF for this element have not been calculated but are expected to be close to 1.

Rate:
Reaction rate N_A<σv> given in 10² cm³/mole/s, including SEF

	18Ne 1.67 s β+ 19Ne 17.22 s β+ 20Ne 90.48 0.119 mb 21Ne 0.27 1.5 mb 22Ne 9.25 0.059 mb 17F 1.07 m β+ 18F 1.83 h β+ 19F 100 5.8 mb 20F 11.07 s β- 21F 4.16 s β- 16O 99.762 0.038 mb 17O 0.038 18O 0.2 0.00886 mb 19O 26.88 s β- 20O 13.51 s β- 15N 0.366 0.0058 mb 16N 7.13 s β- 17N 4.17 s β- 18N 624.00 ms β- 19N 271.00 ms β- 14C 5.70 ka 0.00848 mb, β- 15C 2.45 s β- 16C 747.00 ms β- 17C 193.00 ms β- 18C 92.00 ms β-

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