Observational constraints on the neutron star mass distribution

Radio observations of neutron star binary pulsar systems have constrained strongly the masses of eight neutron stars. Assuming neutron star masses are uniformly distributed between lower and upper bounds $m_l$ and $m_u$, the observations determine with 95\% confidence that $1.01 < m_l/\text{M}_\odot < 1.34$ and $1.43 < m_u/\text{M}_\odot < 1.64$. These limits give observational support to neutron star formation scenarios that suggest that masses should fall predominantly in the range $1.3<m/\text{M}_\odot<1.6$, and will also be important in the interpretation of binary inspiral observations by the Laser Interferometer Gravitational-wave Observatory.Comment: Postscript, 4 pages, NU-GR-

Prevention of chemotherapy and radiotherapy-induced emesis: Results of the Perugia consensus Conference

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Deliberative Mapping: a novel analytic-deliberative methodology to support contested science-policy decisions

This paper discusses the methodological development of Deliberative Mapping (DM), a participatory, multi-criteria, option appraisal process that combines a novel approach to the use of quantitative decision analysis techniques with some significant innovations in the field of participatory deliberation. DM is a symmetrical process, engaging "specialists" and "citizens" in the same appraisal process, providing for consistency of framing, mutual inter-linkage and interrogation, and substantial opportunities for face-to-face discussion. Through a detailed case study of organ transplantation options, the paper discusses the steps in DM. The analysis shows that DM is able to elicit and document consensual judgments as well as divergent views by integrating analytic and deliberative components in a transparent, auditable process that creates many opportunities for personal learning, and provides a robust decision-support tool for contested science-policy issues