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...
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PublicationTransmission- to Reflection-dominated Transition in Seyfert 2 Galaxies: the XMM-Newton View
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PublicationTransportable 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...
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PublicationTransportable 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...
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PublicationTransverse Oscillations in Coronal Loops
During last years, direct evidence about oscillations in different coronal structures has been obtained thanks to the detailed observations made by SoHO and...
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PublicationTrends for Outer Disk Profiles
The surface-brightness profiles of galaxy disks fall into three main classes, based on whether they are simple exponentials (Type I), bend down at large radii...
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PublicationTriaxiality can Explain the Alleged Dark Matter Deficiency in some Dwarf Galaxies
Dark Matter (DM) is an ingredient essential to the current cosmological concordance model. It provides the gravitational pull needed for the baryons to form...
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PublicationTriaxiality in the bulges of spirals: dynamical implications
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PublicationTriggered Star Formation Along the Spiral Arms of M51
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PublicationTriggered Star Formation on Galactic Scales
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