Velocity Field of the Optical Nebula at the Center of the Perseus Cluster Jeremy Lim (University of Hong Kong) *Jeffrey Chan (University of Hong Kong)
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.
Spectral Line Observing I
Ninth Synthesis Imaging Summer School Socorro, June 15-22, 2004 Spectral Line Observing I Michael P. Rupen NRAO/Socorro.
ALFALFA:
Wide-Field HI Galaxy Surveys The Arecibo Legacy Fast ALFA (ALFALFA) Survey and its Predictions for Future Surveys Martha Haynes Cornell University STScI.
ESAC report Rebaselining Time Allocation procedure Other items ARC, EU-FP6: see T. Wilson.
Analyzing Spectral Cubes
The Arecibo Legacy Fast ALFA Extragalactic HI Survey: (The Search for Low-Mass, Gas-Rich Halos) Martha Haynes (Cornell University) for the ALFALFA team.
Velocity Field of the Optical Nebula at the Center of the Perseus Cluster
