The Transiting Exoplanet Survey Satellite (TESS) will search for planets transiting bright and nearby stars. TESS has been selected by NASA for launch in 2017...
Transits against Fainter Stars: The Power of Image Deconvolution
Compared to bright star searches, surveys for transiting planets against fainter (V = 12 18) stars have the advantage of much higher sky densities of dwarf star...
Gaia, an ESA cornerstone mission, will obtain of the order of 100 high-precision photometric observations over five years for tens of millions of stars with V ...
Transmission Spectroscopy of HAT-P-32Ab with GTC/OSIRIS
I will present one of the latest results of our GTC exoplanet transit spectroscopy survey. Over the last years our group has obtained ground-based optical (538...
Transmission- to Reflection-dominated Transition in Seyfert 2 Galaxies: the XMM-Newton View
In this paper we present the current status of a XMM-Newton program to observe an optically-defined, complete and unbiased sample of Compton-thick Seyfert 2...
Transportable ground station for QKD using adaptive optics
This article summarizes the results of a system engineering approach to the design of a Transportable Optical Ground Station (TOGS) intended to be used for...
Transportable optical ground station for QKD using adaptive optics with a plenoptic wavefront sensor
The Institute of Astrophysics of the Canary Islands, IAC, and specifically its technology transfer division IACTEC, has a long history of participation in free...
During last years, direct evidence about oscillations in different coronal structures has been obtained thanks to the detailed observations made by SoHO and...