AsrRoItztETRY oF THE OGLE-III o,łre.'

Dla gwiazd z pól w obłokach Magellana, poza streszczoną wyżej anal'izą gwiazd o naj- większych ruc}rach własnych, sporzą<lzono i przeanalizowano katalog ruchów

Assum ing a hadronic origin of the y-ray emission, the m easurem ent uncertainties are propagated into the interpretation o f the accelerated particle

Indeed, the high velocity of the starburst wind (see HESS12) rather suggests an advection-dominated transport, and therefore a spectrum of γ-rays emitted from the starburst region

Correlation matrix (left panel) and normalized precision matrix (right panel) for galaxy clustering and galaxy-galaxy lensing data in the redshift interval 0.5 <

Among the 1654 objects visible in optical range, we identified a sample of 44 newly selected blazar candidates, including 27 flat spectrum radio quasars and 17 BL Lacs.. We

For clarity, for the remainder of this article, when describing the two main galaxy populations, we will call them red and blue when they have been selected simply according

The γ-ray source associated with Centaurus B is visible in the background-subtracted map. The figure also shows residuals on the Galactic plane. These may be attributed to

Probing the non-thermal energy content of the cluster From the upper limits on the integral VHE gamma-ray flux ob- tained by the presented HESS observations, it is possible to