Southern cosmology survey I Optical cluster detections and predictions for the southern common area millimeter wave experiments

Using ground-based data, meteorological observations, and atmospheric environmental monitoring data, a comparative analysis of the microphysical and optical properties, and

In addition to two learning modes that are articulated in the literature (learning through incident handling practices, and post-incident reflection), the chapter

The luminosity function of the former method is derived by summing membership probabilities of all stars fitted to distribution functions in the vector point diagram, whereas

In the previous sections we have shown how astronomical alignments and solar hierophanies – with a common interest in the solstices − were substantiated in the

In this article, we present a new release of the DANCe- Pleiades catalog including new photometry and updated mem- bership probabilities (Appendix A), as well as a new analysis of

To do that, we have introduced, for both the case of trivial and non-trivial ’t Hooft non-abelian flux, the back- ground symmetric gauge: the gauge in which the stable SU (N )

New generations of researchers have emerged in the field, and some, although responding to an increasing cosmopolitanisation of academies, in a more or less activist way

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