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[O II] as a tracer of current star formation
Rolf A. Jansen, Marijn Franx, Daniel Fabricant
[O II] lambda 3727 Angstrom is often used as a tracer of star formation at intermediate redshifts (z > 0.4), where Halpha is not easily observed. We use the spectrophotometric data…
Weak lensing study of low mass galaxy groups: implications for Omega_m
H. Hoekstra, M. Franx, K. Kuijken +8
We report on the first measurement of the average mass and mass-to-light ratio of galaxy groups by analysing the weak lensing signal induced by these systems. The groups, which hav…
Evolution of Cluster Early-Type Galaxies
P. G. van Dokkum, M. Franx, D. D. Kelson +2
The slow evolution of the M/L ratios, colors, and line strengths of cluster early-type galaxies to z=1 suggests that their stars were formed at very high redshift. At the same time…
Lessons from lensed Lyman break galaxies: can dusty Lyman break galaxies produce the submillimetre counts and background?
Paul P. van der Werf, Kirsten Kraiberg Knudsen, Ivo Labb'e +1
Can the submillimetre counts and background be produced by applying a locally derived extinction correction to the population of Lyman break galaxies? We investigate the submillime…
Can dusty Lyman break galaxies produce the submillimeter counts and background? Lessons from lensed Lyman break galaxies
Paul P. van der Werf, Kirsten Kraiberg Knudsen, Ivo Labbe +1
Can the submillimeter counts and background be produced by applying a locally derived extinction correction to the population of Lyman break galaxies? We investigate the submillime…
Formation and Evolution of E and S0 Galaxies from HST and Keck Studies of z~0.3-1 Clusters
Garth Illingworth, Daniel Kelson, Pieter van Dokkum +1
We have witnessed a dramatic increase over the last five years in results on distant galaxies, in large part because of the high resolution imaging capability of HST, and the multi…