Details on DARWIN and the Search for Extrasolar Planets

It is consistent with this rule for the nominating committee to choose one or more of the currently open positions that share responsibilities with other positions

At any time, at least 20 members of the IETF community, who are qualified to be voting members of a nominating committee, may request by signed petition (email

In this work we consider the general question: for a given algebraic formal power series with coefficients in a finite field, what kind of regularity (if any) can be expected for

Methods of calibration and moni- toring using LED and laser systems, and also Cherenkov events from muon rings and arcs are presented here..

We present the detection of a warm Neptune orbiting the M dwarf Gl 378, using radial velocity measurements obtained with the SOPHIE spectrograph at the Observatoire de

by the AO system, and the resulting higher single-mode cou- pling efficiency. The improvement level, however, is lower than the predictions given in Fig. This may be explained by

Second from top panel: GLS of radial velocities after zero-point correction and removal of secular acceleration term, that is the residuals of the k0d0 model shown in the top

Periodogram of: (top) the radial velocities calculated with template-matching for Gl617A from the SOPHIE + measurements, cor- rected from the zero-point drift; (middle) the