Eclipse timing variation (ETV) analysis of short period binaries is a useful method to detect circumbinary exoplanets.
The satellite Venus Express (2006-2015), together with the Japanese spacecraft Akatsuki (still in orbit) and ground-based campaigns, are unveiling our neighbor planet. At the same time, those new measurements put in evidence the complexity and the high variability of the Venus atmosphere, opening new scientific questions (e.g.
Quasi-Stellar Objects (QSOs) are active galactic nuclei so powerful, that their luminosity can surpass that of the host galaxy, making the observation of the latter extremely difficult or even impossible. Usually QSOs appear on images as point-like sources, what, together with the enormous distances, makes them excellent objects for the materialization of reference systems.
The Euclid space mission will image and obtain NIR spectra of 15,000 deg^2 of the sky outside the Galactic plane.
Gr@v member T. Boekholt visited Tokyo University in Tokyo, Japan. His visit was hosted by Prof. Michiko Fujii, head of the computational astrophysics group at the Astronomy Department. T. Boekholt started a new collaboration on studying planetary dynamics and he presented his recent publication on the Slingshot mechanism in Orion.
"SKA days PT" took place last 6 and 7 of February, at Covilhã and Lisbon, an initiative to promote the Square Kilometer Array (SKA) - the world's largest radio telescope - among the Portuguese scientific and business communities.
SKA project has the participation of 19 countries, in the case of Portugal it is via the infrastructure ENGAGE SKA, which is a consortium composed by the Instituto de Telecomunicações, the Universities of Aveiro (Gr@v), Porto and Évora, and the Polytechnic Institute of Beja.
Greybody factors are frequency dependent quantities that measure the deviation from the perfect black body spectrum of Hawking radiation, and they provide us with valuable information about the near horizon structure of black holes. In
addition, when black holes are perturbed the geometry of spacetime undergoes dumbed oscillations.
DOPPLER (DevelOpment of PaloP knowLEdge in Radioastronomy), coordinated by Dr. Valério Ribeiro of Gr@v (University of Aveiro), is a recently funded FCT and the Aga Khan Development Network project.
The first global meeting of the COST Action ”CA 16104 Gravitational waves, black holes and fundamental physics (GWverse)” took place in Malta, Gravity@Malta2018 (22-25 January 2018). The meeting brought together three normally disjoint communities, namely Gravitational Wave detection and analysis, BH modeling (in both astrophysical and GR contexts), and strong-gravity tests of fundamental physics.
Ema Valente successfully finished her Physics M.Sc. at Aveiro University, on December 20th 2017, by defending a thesis with title "A simple model of exotic compact objects: interaction with a scalar field". This thesis was supervised by Gr@v researcher C. Herdeiro and examined by Prof. Luis Crispino, from the U. Federal do Pará, Brazil. Well done Ema!