Galaxy formation and evolution

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THE EFFECTS OF SEEING ON THE PHOTOMETRIC PROPERTIES OF ELLIPTIC GALAXIES

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 264:4 (1993) 961-974

Authors:

RP SAGLIA, E BERTSCHINGER, G BAGGLEY, D BURSTEIN, M COLLESS, RL DAVIES, RK MCMAHAN, G WEGNER
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A CRITICAL-REVIEW OF SELECTED TECHNIQUES FOR MEASURING EXTRAGALACTIC DISTANCES

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 104:678 (1992) 599-662

Authors:

GH JACOBY, D BRANCH, R CIARDULLO, RL DAVIES, WE HARRIS, MJ PIERCE, CJ PRITCHET, JL TONRY, DL WELCH
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OPTIMAL ANTENNA CONFIGURATIONS FOR THE BIMA ARRAY

19 (1991) 457-463

Authors:

N THATTE, WMJ WELCH
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THE STELLAR LUMINOSITY FUNCTION IN THE BULGE OF M31

ASTRONOMICAL JOURNAL 102:5 (1991) 1729-1733

Authors:

RL DAVIES, JA FROGEL, DM TERNDRUP
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Technical description of the U.K. large telescope

Proceedings of SPIE - The International Society for Optical Engineering 1236 pt 1 (1990) 26-40

Authors:

RL Davies, K Raybould

Abstract:

The UK is currently developing an 8m optical/infrared telescope in a Phase A program which started in October 1988. The design studies will be completed in September 1990 when a report will be submitted to the Science and Engineering Research Council for approval. This paper describes the telecope facility and briefly outlines the Phase A design studies. The technical effort during the Phase A has concentrated on aspects that require design efforts to prove technical feasibility, and on design areas that have a potentially high impact on the cost. The UK Large Telescope project is a national endeavour co-ordinated by the project team based at Oxford University and includes significant contributions from the Royal Greenwich Observatory, the Royal Observatory Edinburgh, the Rutherford Appleton Laboratory, the Council Works Unit, and several University groups.
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