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R. Silberberg, C.H. Tsao, Astrophys. J. Suppl. 220 (I) 25
1973
Earlier work this paper cites.
T.W. Armstrong, K.C. Chandler, J. Barish, J. Geophys. Res. 78
1973
Earlier work this paper cites.

Similar

R. Silberberg, and C. H. Tsao, Astrophys. J. 501
1998
Cited alongside, same era.
J. F. Ziegler, IBM Journal of Research and Development 42
1998
Cited alongside, same era.
M. Yeh et al
Cited in the paper.
V. Lozza and J. Petzoldt (in preparation)
Cited in the paper.
http://www.talys.eu
Cited in the paper.
B. Wang (these proceedings)
Cited in the paper.
M. Yeh et al
Original
Cited in the paper.

Then

J. J. Back, Y. A. Ramachers, ACTIVIA:Calculation of isotope production cross-sections and yields
2008
Later among the works it cites.
S. Biller and M. Chen, SNO+ internal report #1532-v1 (Aug, 2012)
2012
Later among the works it cites.

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2014

SNO+ with Tellurium

Biller, Steven

Understand

The SNO+ experiment, currently undergoing commissioning, will be a large scale liquid scintillator detector capable of studying a variety of physics topics, with the highest priority being a sensitive search for neutrinoless double beta decay.

The collaboration has recently decided to use 130Te as the candidate isotope for this search, having developed a new approach to the purification and loading of tellurium into liquid scintillator.
An initial Phase I demonstrator with a 0.3% Te loading is expected to reach sensitivities to Majorana neutrino masses approaching the top of the inverted neutrino mass hierarchy.
If successful, there is significant scope for further enhancements that could lead to measurements covering the vast majority of the inverted hierarchy range with high sensitivity.