baryons = 0.045+/-0.004 ~ (1/6) matter Coronal & diffuse IG gas~0.037 Cluster IGM~0.002 Stars ~ 0.003 Cold Gas ~ 0.0008 (~2/3 atomic) HI is a piffling.
ASKAP Continuum Surveys of Local Galaxies Michael Brown ARC Future Fellow Monash University.
Transient Science with the Allen Telescope Array Geoff Bower Berkeley.
Recent Results and the Future of Radio Afterglow Observations Alexander van der Horst Astronomical Institute Anton Pannekoek University of Amsterdam.
The Turbulent Interstellar Medium
ALMA Science WorkshopMay 14, 2004 Present and Future Thomas W. Folkers Arizona Radio Observatory.
ALFALFA:
Wide-Field HI Galaxy Surveys The Arecibo Legacy Fast ALFA (ALFALFA) Survey and its Predictions for Future Surveys Martha Haynes Cornell University STScI.
Molecular Gas at High Redshift
Radio `source’
The Arecibo Legacy Fast ALFA Extragalactic HI Survey: (The Search for Low-Mass, Gas-Rich Halos) Martha Haynes (Cornell University) for the ALFALFA team.
