tipa -- 7/5/2012

A filament of dark matter between two clusters of galaxies

• Jörg P. Dietrich (1), Norbert Werner (2), Douglas Clowe (3), Alexis Finoguenov (4), Tom Kitching (5), Lance Miller (6), Aurora Simionescu (2) ((1) Physics Dept., University of Michigan, (2) KIPAC, Stanford, (3) Dept. of Physics & Astronomy, Ohio University, (4) MPE, (5) Institute for Astronomy, The University of Edinburgh, (6) Department of Physics, University of Oxford)

The influence of rotation on optical emission profiles of O stars

• D. John Hillier, Jean-Claude Bouret, Thierry Lanz, Joseph R. Busche

The unusual smoothness of the extragalactic unresolved radio background

• Gilbert Holder

Stellar Intensity Interferometry: Prospects for sub-milliarcsecond optical imaging

• Dainis Dravins (Lund Observatory), Stephan LeBohec (University of Utah), Hannes Jensen (Lund Observatory and Stockholm University), Paul D. Nuñez (University of Utah)

Use of event-level neutrino telescope data in global fits for theories of new physics

• P. Scott, C. Savage, J. Edsjö, the IceCube Collaboration