The Evolution of Galaxy Dark Matter and Stellar Mass to z = 1.2 : IRAC Imaging of the Deep Lens Survey Field F2

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Scientific paper

We propose to image 4 square degrees with IRAC (to 120s depth) to carry out a unique project to directly compare the stellar mass content of galaxies with the masses of their dark halos. The IRAC observations will complement a parallel ground-based weak lensing analysis of the same field, currently being undertaken by the Deep Lens Survey (DLS) team. The proposed field is one of five fields comprising the ultradeep BVRz' 20 square degree DLS survey. We will photometrically (and spectroscopically) subdivide galaxies by redshift, luminosity and morphological type, measure average dark matter halos from the full 20 square degrees and average stellar mass for galaxies of the same type from the 4 square degree field. This dataset will allow us to study the evolution of baryons relative to the dark matter to z = 1.2

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