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  1. C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.
  2. First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).
  3. M. G. Ingraham, D. C. Hess, Jr., and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.
  4. H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).
  5. P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I ≧3/2 reported for both odd isotopes.

Brix, P.

P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I ≧3/2 reported for both odd isotopes.

Hayden, R. J.

M. G. Ingraham, D. C. Hess, Jr., and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.

Hess, Jr., D. C.

M. G. Ingraham, D. C. Hess, Jr., and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.

Ingraham, M. G.

M. G. Ingraham, D. C. Hess, Jr., and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.

Keim, C. P.

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

Kopfermann, H.

P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I ≧3/2 reported for both odd isotopes.

Pohl, M.

First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).

Savage, H. W.

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

Schmidt, T.

H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).

Schueler, H.

H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).

von Hevesy, G.

First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).

Weaver, Boyd S.

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

Other (5)

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).

M. G. Ingraham, D. C. Hess, Jr., and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.

H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).

P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I ≧3/2 reported for both odd isotopes.

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