Messenger No144
A Sedna-like body with a perihelion of 80 astronomical units
Combined strong weak_lensing_analysis_from_sloan_giant_arcs_survey
Integral Field Spectroscopy on Gemini Andrew Bunker (IoA, Cambridge) Euro3D Meeting July 2002 GMOS Gemini Multi-Object Spectrograph, optical IFU (Durham)
Jim Kennedy AMPATH Meeting 31 January 2003 The Gemini Observatory: An Application of High-Performance Networks Tools in Modern Astronomy.
Spectroscopy of H 3 + and CO toward the Galactic center Takeshi Oka, Christopher P. Morong, Department of Astronomy And Astrophysics and Department of.
Determining Age on Two Cooling Sequences: Sub-Stellar Brown Dwarfs and Evolved White Dwarfs Sandy Leggett 1, Pierre Bergeron 2, Ben Burningham 3, Mike.
Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center from 140 pc West to 85 pc East of Sgr A* 66th OSU International Symposium, June.
P7: Observing the Universe. Convex / Converging Lenses bring light to a Focus.
Seeing the Distant Universe in Integral Field Spectroscopy at high redshift 3D Andrew Bunker, AAO & Oxford.
Measuring Deflection of the Telescope Mount
Nick Indriolo , 1 Ben McCall, 1 Tom Geballe, 2 & Takeshi Oka 3
