Perspectives for speckle cameras at the GTC and WHT
I will present a short introduction to speckle imaging and the so-called speckle holography technique. Subsequently, I will present results of speckle...
Planning the WHT future: the WEAVE wide-field massive-multiplex spectrograph
The vision for the use of the WHT in the coming decade is taking shape. A key element is the construction and deployment of WEAVE, a wide-field massive...
Precipitable water vapour at the Roque de los Muchachos Observatory from GPS measurements
There are many parameters accounting for the quality of an astronomical site, namely seeing, cloud cover, ground winds, high-altitude winds, etc. The water...
Precipitable Water Vapour measurements and forecasting at the Observatories.
The precipitable water vapour (PWV) is the main absorber in the Earth's atmosphere at infrared (IR) and microwave wavelengths. In the last years, the IAC Sky...
Luminous high-redshift radio galaxies (HzRGs) are associated with the most massive known galaxies in the early Universe. These galaxies have the properties...
Proposed Operations and Renovation of the JKT by the Southeastern Association for Research In Astronomy
The Southeastern Association for Research in Astronomy (SARA) is a consortium of 11 US universities that currently remotely operates a 0.9 m telescope at Kitt...
Public Surveys and New Instrumentation for Calar Alto Observatory
In this talk I will present the current status of the Calar Alto observatory. I will review the most important highlights published in 2019, as well as the...
QUIJOTE: el estado de la instrumentación CMB en Canarias.
Durante este seminario se hará un recorrido sobre la instrumentación dentro del proyecto QUIJOTE, desde de los instrumentos ya existentes y su problemática...
Response of the solar atmosphere to the photospheric plasma motion
The dynamics of the solar atmosphere is largely controlled by its magnetic coupling to the photosphere of the Sun. Since the solar magnetic field is complex...