S4N: A Spectroscopic Survey of Stars in the Solar Neighborhood
We are using the McDonald 2.7m and ESO 1.52m telescopes to obtain spectra of nearby stars at high-resolution, high S/N, and with complete optical coverage. The...
SABIO: new system for telescope full scheduling and queue operation to be implemented at the Observatorio de EL Teide
SABIO is currently at the beginning of the specification phase at the Instituto de Astrofisica de Canarias (IAC). This system is aimed at providing full control...
SAFIR: testing the coexistence of AGN and star formation activity and the nature of the dusty torus in the local Universe
We present the Seyfert and star formation Activity in the Far-InfraRed (SAFIR) project, a small (15.1 h) Herschel guaranteed time proposal performing PACS and...
Sampling and Characterization of the Turbulence Vertical Distribution. Statistics of SCIDAR Profiling
Unlike the trial procedures, a reliable characterization of the vertical turbulence distribution on a site should be based in unbiased statistical sample...
The Observatorio Astronomico Nacional at San Pedro Martir is situated on the summit of the San Pedro Martir Sierra in the Baja California peninsula of Mexico...