Dusty starburst galaxies_in_the_early_universe_as_revealed_by_gravitational_lensing
LYα FOREST TOMOGRAPHY FROM BACKGROUND GALAXIES: THE FIRST MEGAPARSEC-RESOLUTION LARGE-SCALE STRUCTURE MAP AT z > 2
Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen.
Debris Disks around Nearby Stars David J. Wilner (Harvard-Smithsonian CfA ) What are Debris Disks? dust requires replenishment Interest in Resolved Morphologies.
Research in Astronomy Prof. David Cohen Swarthmore College January 30, 2004 Resources and Information for Students Sponsored by SWAP.
The Merger History of Centaurus A: New Evidence from Halo and Group Dynamics
In this toy scenario, metal enriched clouds entrained in galactic winds gives rise to absorption lines in quasar spectra, as illustrated in the above panels.
Joint Analysis of Weak Lensing and SZE data from the Arcminute Microkelvin Imager Natasha Hurley-Walker in collaboration with Farhan Feroz, Jonathan Zwart,
The g iant a rc statistic in the three-year WMAP cosmological model
Weak Lensing
Photometric redshift for clusters through A1689 and simulation studies
Globular Cluster and Satellite Orbits: 2008 Status Dana Casetti-Dinescu - Wesleyan and Yale.
