ALMA, the Atacama Large Millimeter Array, was formally dedicated on March 13, 2013. After an overview of the highlights of ALMA: Science drivers, characteristic...
ALMA is a submillimetre/millimetre telescope located at 5000m in the Atacama desert in Chile designed to observe at 0.32–9.5 mm (31–950 GHz), and it is expected...
An infrared and sub-mm view of AGN obscuration and feedback
In the past 10-15 years our view of AGN has significantly evolved thanks to the combination of new observations and models. X-ray, infrared and sub-mm data have...
I will present a multiwavelength study of a large MIPS selected galaxies and satisfy a certain IRAC color criterion. Stellar population modeling and IRS spectra...
And the sky fell on our heads: all about the Chelyabinsk event
On February 15, while we were preparing to observe the close approach of the potentially hazardous asteroid (PHA) 2012 DA14 another small asteroid entered the...
Andromeda II: a merger remnant or a product of tidal stirring
I will present an evolutionary model for the origin of Andromeda II, a dSph satellite of M31, involving a merger between two disky dwarf galaxies than explains...
Arch Filament Systems and their evolution through the layers of the solar atmosphere
Emerging flux regions (EFRs) are seen as magnetic concentrations in the photosphere of the Sun. From a theoretical point of view, the EFRs are formed in the...
Fossil groups are an unusual type of galaxy system with an overluminous central galaxy more than 2 magnitudes brighter than their brightest sate llite. To...
The World Health Organization’s International Agency for Research on Cancer (IARC) on May 31st 2011 classified mobile phone use and other radio-frequency...