We describe the user-access and analysis possible for a robotic telescope (the Liverpool Telescope) that can be used for educational and other use. Robotic telescopes operate with no staff on-site and the observations are remotely scheduled each night.

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This is the written account of the second of two panel discussions, on Reconciling observations and modeling of star formation at high redshifts. The chair of the panel was Pavel Kroupa, and panel members were Marc Balcells, John Beckman, Christopher Conselice, and Joseph Silk. After a short introduction by each of the panelists, panel and audience

This is the written account of the first of two panel discussions, on Star formation in galaxies: how do we continue? The chair of the panel was Phil James, and panel members were John Beckman, Torsten Böker, Daniela Calzetti, Angeles Díaz, and Rob Kennicutt. The panel and audience discussed the following four questions: 1) What are the most

In this work we investigate p-mode power variation with solar atmosphere. To this aim, we use THÉMIS observations of the Na D1 (λ5896 Å) and K (λ7699 Å) spectral lines. While the formation heights of the K spectral line are essentially located in the photospheric layer, the formation heights of the Na D1 line span a much wider region: from