The most extreme electromagnetic radiation that can be observed is known as very high energy gamma rays (VHE, E>100 GeV). It is the last window open to the Universe, thanks to the development of the Cherenkov telescopes. The extragalactic VHE sky is still nowadays vastly unexplored, only composed of around 80 known sources. The great majority of them are classified as blazars, a type of Active Galactic Nuclei (AGN) whose relativistic jets point in the direction of the Earth boosting their emission. While the observation of the gamma-ray emission is crucial to understand the extreme physical

Blazars, Active Galactic Nuclei (AGN) whose relativistic jets point in the direction of the Earth, dominate the VHE (VHE, E>100 GeV) gamma-ray extragalactic sky. One of the most famous archetypical VHE gamma-ray emitters is the blazar Markarian 501 (Mrk 501). During July 2014, the source displayed a strong flare detected across all wavelengths from VHE to the optical band. In particular, it is especially interesting that the source reached the maximum flux and harder spectrum measured in the X-ray band, compatible with the most extreme historical flare from this source. On 2014 July 19

Astronomers from the Agrupación Astrónomica de Sabadell together with the Telescopic Operations Technicians of the Instituto de Astrofísica de Canarias, Marta Puig Subirà and Miguel Rodríguez Alarcón, have detected the transit of the exoplanet WASP-156b, catalogued as a high priority objective by the Exoclock project. The depth of the detected transit was only 6 millimagnitudes and will contribute to improve the ephemerides available for the ARIEL (Atmospheric Remote-sensing Infrared Exoplanet Large-survey) mission of the European Space Agency. Exoclock project: Kokori, A., Tsiaras, A