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Traditional database systems hide the recovery process from the user.

The ECONET project is a 3-year large-scale Integrating Project (IP) running from October 2010 to September 2013, co-funded by the European Commission under the 7th Framework Programme.

We have found the CDW in (TaSe(4))(2)I to display a low frequency dielectric relaxation characterized by a distribution of relaxation times.

In the temperature range 450-600C, the title compound (DADBS) deposits silicon dioxide films which have a refractive index of 1.44.

The LSST Instrument is a wide-field optical (0.3 to 1 mum) imager designed to provide a three degree field-of-view with better than 0.2 arcsecond sampling.

MEMS devices are beginning to impact almost every area of science and technology.

We attempt to determine whether the MACHO microlensing source stars are drawn from the average population of the LMC or from a population behind the LMC by examining the Hubble Space Telescope (HST

We have frequency-analyzed 6391 variables classified earlier as fundamental-mode RR Lyrae (RR0) stars in the MACHO database on the Large Magellanic Cloud (LMC).

We present a method for solving the light curve of an eclipsing binary system that contains a Cepheid variable as one of its components as well as the solutions for three eclipsing Cepheids in the

Shapes of RR Lyrae light curves can be described in terms of Fourier coefficients that past research has linked with physical characteristics such as luminosity, mass, and temperature.

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