X-ray binaries are excellent laboratories to study the physics of relativistic stars. On the one hand, they provide robust evidence for the existence of black holes (BHs), the pinnacle of extreme gravity. On the other, they allow investigations on neutron stars (NS) the densest form of matter known. In addition, accretion on matter (provided by the
Economic information: Grants
To see the Grants awarded by the IAC (Access the National Subsidy Advertising System) select "Convocatorias", Admon. del Estado: select: Ministerio de Ciencia, Innovación e Universidades; Organo: select: Instituto de Astrofísica de Canarias
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Unveiling the missing populations of X-ray binaries: dormant black holes and ultra-compact systemsJorgeCasares VelázquezIn force dateNot in force
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Unveiling the Properties of Stellar Fosils in the Local Group Environment
The main objective of this project is the study of the primeval star formation in nearby systems. In particular, we will address this research in three fundamental types: (1) the Local Group dwarf galaxies; (2) the Milky Way (MW) bulge and old disk populations; and (3) the Milky Way globular clusters. This kind of investigation is mandatory in
AntonioAparicio JuanIn force dateNot in force -
Using machine-learning techniques to drag galaxies from the noise in deep imaging
We propose to extend our current lead in the area of deep astronomical imaging to decipher the secrets of galaxy formation and evolution. In particular, we will prepare for the imaging from the Large Synoptic Survey Telescope (LSST) to which we will soon have privileged access. The LSST project is truly a 'Big Data' project in astrophysics, which
Johan HendrikKnapen KoelstraIn force dateNot in force -
UV-sensitive detection system for the OSIRIS instrument in the GTCJorgeCepa NogueIn force dateNot in force
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Vacuum equipment, cryogenics and automatic safety control in cryogenic infrastructures
We propose the acquisition of specific technological equipment for the adaptation and safety control of the IAC infrastructures dedicated to the realization of tests in cryogenics and high vacuum of large scientific instrumentation. The increase in the diameter of the telescopes implies a significant increase in the size of their instruments. The
EvencioMediavilla GradolphIn force dateNot in force -
Verifying the FWHM-K2 correlation for erupting Black HolesJorgeCasares VelázquezIn force dateNot in force