PI: David W. Atlee, National Optical Astronomy Observatory, email@example.com
Address: NOAO, 950 N. Cherry Ave, Tucson, AZ 85719, United States of America
CoI: Janine Pforr, National Optical Astronomy Observatory
Title: A Spectroscopic Study of the Contribution of TP-AGB Stars to Integrated NIR Starlight
Abstract: The interpretation of galaxy spectral energy distributions to determine parameters such as stellar masses and star formation rates is one of the most ubiquitous problems in extragalactic astronomy. This problem is usually solved by the use of stellar population synthesis models. However, this process suffers from several systematic uncertainties, including the luminosity of stars ascending the thermally- pulsating asymptotic giant branch (TP-AGB). We propose NIR spectroscopy of post-starburst galaxies with GNIRS and FLAMINGOS. We will measure the strong molecular features expected due to the significant contribution of TP-AGB stars in stellar populations with ages of ~ 300 Myr and determine the contribution of TP-AGB stars to the integrated starlight. Our proposal is part of a multi-wavelength suite of observations that will measure both the direct and re-processed emission of TP-AGB stars to constrain their contribution to integrated stellar populations as a function of age.
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