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astro-ph200586 cited

Orbital X-Ray Variability of the Microquasar LS 5039

V. Bosch-Ramon, J. M. Paredes, M. Ribo +3

The properties of the orbit and the donor star in the high mass X-ray binary microquasar LS 5039 indicate that accretion processes should mainly occur via a radiatively driven wind…

astro-ph2005

Optimization of time data codification and transmission schemes: Application to Gaia

Jordi Portell, Enrique Garcia-Berro, Xavier Luri

Gaia is an ambitious space observatory devoted to obtain the largest and most precise astrometric catalogue of astronomical objects from our Galaxy and beyond. On-board processing…

astro-ph2004

Microquasars as high-energy gamma-ray sources

Josep M. Paredes

Galactic microquasars are certainly one of the most recent additions to the field of high energy astrophysics and have attracted increasing interest over the last decade. However,…

astro-ph20041 cited

Application of fast CCD drift scanning to speckle imaging of binary stars

O. Fors, E. P. Horch, J. Nunez

A new application of a fast CCD drift scanning technique that allows us to perform speckle imaging of binary stars is presented. For each observation, an arbitrary number of speckl…

astro-ph20047 cited

Multiresolution approach for period determination on unevenly sampled data

X. Otazu, M. Ribo, J. M. Paredes +2

In this paper we present a multiresolution-based method for period determination that is able to deal with unevenly sampled data. This method allows us to detect superimposed perio…

astro-ph20047 cited

Infrared and visual lunar occultations measurements of stellar diameters and new binary stars detections at the Calar Alto 1.5m telescope

O. Fors, A. Richichi, J. Nunez +1

We present a program of routine lunar occultations, at optical and near-IR wavelengths, recently started at the 1.5m Spanish telescope at the Calar Alto Observatory. Both a CCD and…