David Humiston Kelley is a Canadian archaeologist and epigrapher, most noted for his work on the phonetic analysis and major contributions toward the decipherment of the writing system used by the Maya civilization of pre-Columbian Mesoamerica, the Maya script. Eugene Frank Milone received a bachelor's degree from Columbia University in 1961, and a Ph.D. in astronomy from Yale University. After teaching for several years at Gettysburg College he re-located in 1971 to the University of Calgary, where he served as Director of the Rothney Astrophysical Observatory. Milone has published many technical papers in various areas of astronomical research, particularly specializing in variable stars and photometry and archaeoastronomy, and has served on several professional committees.
E.F. Milone received a BA from Columbia and his graduate degrees (MS, PhD) in astronomy from Yale University. Since 1971 he has been in the Physics & Astronomy Department of the University of Calgary, helping to shape and direct activities at that universityï¿½s Rothney Astrophysical Observatory and teaching astronomy and astrophysics courses. He retired from the Directorship in Sept. 2004, and as Professor a year later. Currently he is Professor Emeritus, RAO Director Emeritus, and Faculty Professor in the Physics & Astronomy Department, and continues his observational and analytical research on variable stars, and optical and photometry. He is Vice President of the IAU Commission 25 on Photometry and Polarimetry and Chair of that Commissionï¿½s Infrared Working Group.D.A. Leahy received a B.Sc. in Coop. Applied Physics from U. Waterloo in 1975 and M.Sc. in 1976 and Ph.D. in 1980 in Theoretical Physics from University of British Columbia. After 2 years as N.R.C. Research Associate in Space Science at NASAï¿½s Marshall Space Science Center, he returned to Canada for a 1 year Research Associate at University Calgary before taking a NSERC University Research Fellow/ Assistant Professor position in 1983. Research activities have included observing X-ray binaries and supernova remnants using balloon-borne telescopes, space based telescopes including NASAï¿½s X-ray astronomy satellites (HEAO-1, Einstein, RXTE, Chandra), Japanese satellites (GINGA, TENMA, ASCA), European satellites (EXOSAT, ROSAT, XMM-Newton), and several ground based observatories (DRAO, VLA, NOAOï¿½s Kitt Peak telescopes, and others). Theoretical work includes studies on black hole evaporation, timing analysis methods, neutron star magnetospheres, accretion flows in binaries, and quantum electrodynamics in strong magnetic fields. D.W. Hobill has degrees from Worcester Polytechnic Institute (B.S. 1971), the University of Calgary (M.Sc -1974) and the University of Victoria (Ph.D. -1980). His postdoctoral work I ncludes a NATO Fellowship at the Institut Henri Poincare in Paris, and positions at Stevens Institute of Technology and the University of Illinois where he later became the head of the numerical relativity group at the National Center for Supercomputing Applications.He has been in the Department of Physics and Astronomy at the University of Calgary since 1991 where his research interests are in astrophysical applications of general relativity. Specifically his research is in black hole formation. gravitational wave generation from compact objects, gravitational l lensing as a tool for exploring curved space time and anisotropic cosmologies.