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OBSERVATIOSanchez, A. et al.112003
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Observation of enhanced X-ray emission from the CTTS AA Tauri during one transit of an accretion funnel flow
Context: Classical T Tauri stars are young solar-type stars accreting material from their circumstellar disks. Thanks to a favorable inclination of the system, the classical T Tauri star AA Tau exhibits periodic optical eclipses as the warped inner disk edge occults the stellar photosphere. Aims: We intend to observe the X-ray and UV emission of AA
Grosso, N. et al.Fecha de publicación:
112007 -
Observation of Pulsed γ-Rays Above 25 GeV from the Crab Pulsar with MAGIC
One fundamental question about pulsars concerns the mechanism of their pulsed electromagnetic emission. Measuring the high-end region of a pulsar’s spectrum would shed light on this question. By developing a new electronic trigger, we lowered the threshold of the Major Atmospheric γ-ray Imaging Cherenkov (MAGIC) telescope to 25 giga-electron volts
Aliu, E. et al.Fecha de publicación:
112008 -
Observation of VHE γ-rays from Cassiopeia A with the MAGIC telescope
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A Methods: The shell-type supernova remnant Cassiopeia A was observed with the 17 m MAGIC telescope between July 2006 and January 2007 for a total time of 47 h. Results: The source was detected above an energy of 250 GeV with a significance of 5.2σ and
Albert, J. et al.Fecha de publicación:
112007 -
Observational Evidence for Small-Scale Mixture of Weak and Strong Fields in the Quiet Sun
Three different maps of the quiet Sun, observed with the Advanced Stokes Polarimeter (ASP) and the Diffraction-Limited Stokes Polarimeter (DLSP), show evidence of strong (~=1700 G) and weak (
Socas-Navarro, H. et al.Fecha de publicación:
112004 -
Observations and modelling of earth's transmission spectrum through lunar eclipses: A window to transiting exoplanet characterization
Recently we were able to retrieve the Earth's transmission spectrum through lunar eclipse observations. This spectrum showed that the depth of most molecular species was stronger than models had anticipated. The presence of other atmospheric signatures, such as atmospheric dimers, were also present in the spectrum. We have been developing a
Pallé, E. et al.Fecha de publicación:
112011