ar X iv : a st ro - p h / 03 08 07 9 v 1 5 A ug 2 00 3 THE 2 MS CHANDRA DEEP FIELD - NORTH

ar X iv : a st ro - p h / 04 08 13 5 v 1 9 A ug 2 00 4 A Determination of the Chemical Composition of α Centauri A from Strong Lines

ar X iv : a st ro - p h / 96 08 03 6 v 2 1 2 A ug 1 99 6 TABLE 1 Properties of LMC Double - Mode

ar X iv : a st ro - p h / 96 08 03 6 v 1 8 A ug 1 99 6 TABLE 1 Properties of LMC Double - Mode

ar X iv : a st ro - p h / 06 08 54 9 v 1 2 5 A ug 2 00 6 The Atacama Cosmology Telescope Project : A Progress Report

The Atacama Cosmology Telescope is a project to map the microwave background radiation at arcminute angular resolution and high sensitivity in three frequency bands over substantial sky areas. Cosmological signals driving such an experiment are reviewed, and current progress in hardware construction is summarized. Complementary astronomical observations in other wavebands are also discussed.

ar X iv : a st ro - p h / 99 08 14 0 v 2 1 2 A ug 1 99 9 A Cepheid distance to NGC 4258

#NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000 ∗Department of Astronomy, University of California, Berkeley, CA 94720 †Hubble Fellow, California Institute of Technology, MS 105-24, Pasadena, CA 91125 ‡Dominion Astrophysical Observatory, 5071 W. Saanich Rd., Victoria, B.C., Canada V8X 4M6 §Department of Astronomy, P.O. Box 208101, Yale University, New Haven, CT 06520 ‖Observa...