The Growth of Stellar Mass at z > 2: Spitzer Imaging of the Gemini Deep Deep Survey Fields

Details The Growth of Stellar Mass at z > 2: Spitzer Imaging of the Gemini Deep Deep Survey Fields The Growth of Stellar Mass at z > 2: Spitzer Imaging of the Gemini Deep Deep Survey Fields

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop.3554m&link_type=abstract

Spitzer Proposal ID #3554

Physics

Scientific paper

We propose to image three of the Gemini Deep Deep Survey fields in the four IRAC bands. We will use the rest-frame 1-3 micron luminosity and our spectroscopic redshifts to measure the stellar mass in galaxies at z ~ 2. Photometric redshifts from the IRAC photometry and our deep 8-band B through K images, as well as on going deep spectroscopy, will allow us to extend our study of stellar masses to higher redshifts and lower masses, thus spanning most of the galaxy assemble epoch. This small program makes maximum use of the unique aspects of Spitzer by building on the deepest redshift survey to date.

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