The Chandra Deep Protocluster Survey: Evidence for an Enhancement in the AGN Activity in the SSA22 Protocluster at z = 3 09

These two models are then used to calculate the number of SLSNe-I, in bins of ∆z = 0.5 width, centred on multiples of z = 0.5 up to z = 3.5 which is consistent with the highest

Government policy varies between nations and this guidance sets out the need for balanced decision-making about ways of working, and the ongoing safety considerations

 The expansionary monetary policy measures have had a negative impact on net interest margins both via the reduction in interest rates and –less powerfully- the flattening of the

Recent observations of the bulge display a gradient of the mean metallicity and of [Ƚ/Fe] with distance from galactic plane.. Bulge regions away from the plane are less

The spatially-resolved information provided by these observations are allowing us to test and extend the previous body of results from small-sample studies, while at the same time

Relationship between the total cluster stellar mass and the photometric blue fraction for the ALHAMBRA cluster and group sample stacked into different redshift bins. The galaxy

(hundreds of kHz). Resolution problems are directly related to the resulting accuracy of the computation, as it was seen in [18], so 32-bit floating point may not be appropriate

Una vez el Modelo Flyback está en funcionamiento es el momento de obtener los datos de salida con el fin de enviarlos a la memoria DDR para que se puedan transmitir a la