GEPI, Obs. Paris: F. Hammer, H. Flores, & C. Balkowski LAM : P. Amram MPE, Garching : M. Lehnert Stockholm Obs. : G. Östlin, T. Marquart Galaxy kinematics.
ADASS XVII Sep 2007The NOAO Pipeline Applications Francisco Valdes (NOAO) Robert Swaters (UMd) Derec Scott (NOAO) Mark Dickinson (NOAO)
CCD Mosaics at CTIO and SOAR. Abstract: Mosaics based on 2K x 4K CCDs are briefly reviewed. An 8Kx8K mosaic of SITe002A CCDs is in use at the 4m Blanco.
HETDEX Spectrographs R&D for DESpec Jennifer Marshall Texas A&M University.
The University of Wyoming GRB Afterglow Follow-Up Program S. L. Savage 1,2, M. Pierce 1, R. Canterna 1, A. S. Kutyrev 2, J. P. Norris 2 1 University of.
Some Thoughts on Ground Layer Adaptive Optics & Adaptive Secondary Mirrors for Keck
VLST workshop; STScI February 2004 1 UV astronomy in the post- GALEX era Noah Brosch Wise Observatory Tel Aviv University Israel.
Triggering radio galaxies at 0
IGRINS Immersion GRating INfrared Spectrograph: Current Design
The Thüringer Landessternwarte Tautenburg
25 Nov 20091 Triggering radio galaxies at 0
Future instrumentation for high-energy solar physics a partial and partial survey David Smith.
