FIT ALL PHOTOMETRIC AND GRISM SPECTROSCOPIC DATA FOR QUIESCENT GALAXIES IN 3D-HST SURVEYS. STUDY THE AGE-DUST DEGENERACY BY CONNECTING THE STAR-FORMATION TIMESCALES TO OTHER OBSERVATIONAL PARAMETERS THAT ARE GENERALLY EASIER TO MEASURE.
$120,367FY2020National Aeronautics and Space AdministrationNASA
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