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1
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78349231920
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note
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This paper is a commentary from the lecture given at ESOR XII, Haifa, September 2009 and is based on the work of reference [29]; since the intended focus is to present the flow of events choronologically, there are some differences in presentation. (a) Putative structures are introduced in a different order; however, to avoid any confusion we have chosen to maintain the previous ordering and, as a consequence, putative structures do not appear in numerical order here. Also, structure 2 was incorrectly drawn in reference [29] and has been corrected here (we thank a Referee for pointing this out). (b) Keppler's compound, which is not an isomer of arsenicin A (2 in reference [29]) is named 13 here. (c) Computational details are only briefly listed below, as follows (see reference [29] for details). The structure of each species was optimized at the B3LYP/6-311G(2d,2p) level. NMR parameters were computed with several methods; the results reported in Figs 1 and 2 include shieldings calculated including relativistic corrections by means of the Zero-Order Regular Approximation (ZORA) up to spin-orbit coupling (ZSO) with the Becke88-Perdew86 GGA functional (BP) and a double-zeta, twice-polarized Slater basis set (TZ2P); coupling constants with the B3LYP functional and a mixed basis set comprising pcJ-2 for O, C, and H, and cc-pVTZ for As.
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