The capabilities of Eddington for the detection and analysis of extrasolar planets are outlined. The primary goal of the PF (Planet finding) part of the mission...
EDiFiSE: equalized and diffraction-limited field spectrograph experiment
We present EDiFiSE, a prototype instrument for the observation of high-contrast systems, combining an adaptive optics (AO) system and an equalized integral...
Cosmoeduca is an educational project set up by the Canaries Astrophysics Institute (IAC), with the support of the Spanish Ministry of Science and Technology...
Educational Project with Robotic Telescopes (PETeR): robots looking to the future
The ``Proyecto Educativo con Telescopios Robóticos'' (PETeR) of the Instituto de Astrofísica de Canarias is an online inquiry-based laboratory that allows...
EELT-HIRES the high-resolution spectrograph for the E-ELT
The first generation of E-ELT instruments will include an optic-infrared High Resolution Spectrograph, conventionally indicated as EELT-HIRES, which will be...
Effect of atmospheric extinction on solar radial velocity measurements
Effects of differential extinction across the Earth's atmosphere on astronomical photometry are reviewed. Under the same circumstances when a rotating extended...
Effect of Fast Rotation on L and T eff Determination and Seismology of delta Scuti Stars
For a decade now, d Scuti stars are considered as very good candidates for asteroseismology and a lot of efforts have been made to fit the increasing number of...
Effect of line-of-sight inclinations on the observation of solar activity cycle: Lessons for CoRoT & Kepler
CoRoT and Kepler missions are collecting data of solar-like oscillating stars of unprecedented quality. Moreover, thanks to the length of the time series, we...