Excavations at Tas-Silg, 1996

For the first time ever, the Department of Classics and Archaeology of the University of Malta conducted its own excavations at the site of Tas-Silg which is located at Marsaxlokk in the south-east of the island of Malta. These excavations were directed by the authors, who would like to thank Mr Simon Mason and Mr Nicholas Vella who were responsible for the field supervision. We would also like to thank the area supervisors, namely Mr Andrew Appleyard, Ms Carmen Michelle 'Buhagiar, Ms Aloisia de Trafford, Mr Joseph Magro Conti, Mr Paul C. Saliba as well as Mr Andre Corrado; the latter agreed to act as an area supervisor for a while when the need arose. Obviously, we do also appreciate very much all the hard work of the "diggers" who were in fact students from.the aforementioned Department of Classics and Archaeology, the foreign and local students who formed part of the first Summer School in Archaeology which was organized by the International Office of the University of Malta, and some very eager and hard-working volunteers.peer-reviewe

Excavations at Tas-Silg, Malta : a preliminary report on the 1996-1998 campaigns conducted by the Department of Classics and Archaeology of the University of Malta

The area known as Tas-Silg is situated in the south-eastern part of the island of Malta, close to Marsaxlokk harbour. In reality the place name refers to the small church dedicated to Our Lady of the Snows (hence Tas-Silg) situated at the point where the narrow · road from Zejtun forks out in two directions: to Delimara and Xrobb il-Ghagin due south-east and to Marsaxlokk village due south-west. A British-period fort occupying the highest point of the elongated hill further south along· the first road also carries the same place name. The lower and more compact hill on which the excavations have been conducted is called 'Ta' Berikka' , but since it is so close to the above-mentioned church (only 50 m to the north) the tradition of calling it Tas-Silg is now well established and there is no sense in changing it. The site has a commanding view of the Marsaxlokk harbour to the south and overlooks two other bays, Marsascala and St Thomas's bay, to the north-east. On all sides the slope is broken up by man-made terraced fields There is no doubt that the topography of the site must have been a determining factor in its choice for the establishment of a religious centre in the Temple period of Maltese pehistory (3000--2500 BC), though one must keep in mind that close to Tas-Silg there are three other prehistoric temple sites. each one with a completely different topography. The Temple people were quite introverted in their cultural isolation and do not seem to have been much interested in seafaring and in the outside world. The situation changed radically in the following age, the Bronze Age. when the island was occupied by people who set up villages on naturally defensible hilltops, occasionally fortifying them with artificial ramparts. The Tas-Silg hill with its temple ruins was occupied by these people, but it is not as yet clear for what purpose. The scenario changed again in historical times when the central and western Mediterranean started to be parcelled out among the commercial powers originating in the eastern Mediterranean. The Greeks do not seem to have even tried 10 colonize Malta as they did in neighbouring Sicily. The Phoenicians, however, did occupy the island, apparently through a slow process of peaceful penetration and eventual political and cultural assimi lation. It was in this period that the ruins of the megalithic temple were transformed into a Phoenician extraurban shrine dedicated to Astarte, which in time expanded into a full y-fledged sanctuary with an international reputation. The last chapter in the millennia- long history of the site was written when the colonnaded courtyard in front of the old temple was transformed into an early Christian church. Any use made of the site in the following Arab period is, once again, poorly understood.peer-reviewe

Optical Synoptic Telescopes: New Science Frontiers

Over the past decade, sky surveys such as the Sloan Digital Sky Survey have proven the power of large data sets for answering fundamental astrophysical questions. This observational progress, based on a synergy of advances in telescope construction, detectors, and information technology, has had a dramatic impact on nearly all fields of astronomy, and areas of fundamental physics. The next-generation instruments, and the surveys that will be made with them, will maintain this revolutionary progress. The hardware and computational technical challenges and the exciting science opportunities are attracting scientists and engineers from astronomy, optics, low-light-level detectors, high-energy physics, statistics, and computer science. The history of astronomy has taught us repeatedly that there are surprises whenever we view the sky in a new way. This will be particularly true of discoveries emerging from a new generation of sky surveys. Imaging data from large ground-based active optics telescopes with sufficient etendue can address many scientific missions simultaneously. These new investigations will rely on the statistical precision obtainable with billions of objects. For the first time, the full sky will be surveyed deep and fast, opening a new window on a universe of faint moving and distant exploding objects as well as unraveling the mystery of dark energy.Comment: 12 pages, 7 figure

Critique [of Institutional Racism]

As Deloria indicates in the opening lines of his essay, the dominant paradigm of racism in the 1960s reflected the popularly held belief that racism was an individual phenomena. Consequently. if racist individuals were confronted and curtailed or converted, the argument concluded, then discrimination would come to an end. However, history has shown us that we can have racist institutions without having racist individuals. For instance, our education institutions perpetuate racial, as well as sex, inequality. Yet it is possible for every member of such an institution to be non-racist, as well as non-sexist

Heavy Ion e+ e- Pairs to All Orders in Z alpha

The heavy ion cross section for continuum e+ e- pair production has been calculated to all orders in Z alpha. Comparison is made with available CERN SPS and RHIC STAR data. Computed cross sections are found to be reduced from perturbation theory with increasing charge of the colliding heavy ions and for all energy and momentum regions investigated. Au or Pb total cross sections are reduced by 28% (SPS), 17% (RHIC),and 11% (LHC). For very high energy (E_e+, E_e- > 3 GeV) forward pairs at LHC the reduction from perturbation theory is a bit larger (17%). Use of zero degree calorimeter triggering (and thus small impact parameter weighting) makes impact parameter representation of exact pair production useful. Preliminary exact calculations in the zero impact parameter limit show a much larger reduction from perturbation theory (about 40%) at both RHIC and LHC.Comment: 4 pages, poster proceedings from Quark Matter 200