Analysis of LIGO data for gravitational waves from binary neutron stars

We report on a search for gravitational waves from coalescing compact binary systems in the Milky Way and the Magellanic Clouds. The analysis uses data taken by two of the three LIGO interferometers during the first LIGO science run and illustrates a method of setting upper limits on inspiral event rates using interferometer data. The analysis pipeline is described with particular attention to data selection and coincidence between the two interferometers. We establish an observational upper limit of $\mathcal{R}<$1.7 \times 10^{2}$per year per Milky Way Equivalent Galaxy (MWEG), with 90coalescence rate of binary systems in which each component has a mass in the range 1--3$M_\odot$.Comment: 17 pages, 9 figure

Political factors in the future of pastoral peoples

In IDL-411

Facteurs politiques déterminant l'avenir des peuples pasteurs

Réunion: Avenir des peuples pasteurs, 4-8 août 1980, Nairobi, KEDans IDL-764

Some remarks on the roles of advisers and advocates

In IDL-411

Quelques observations au sujet du rôle des conseillers et des avocats

Réunion: Avenir des peuples pasteurs, 4-8 août 1980, Nairobi, KEDans IDL-764