Empirical aperture corrections for SDSS absorption indices, derived via CALIFA simulations, reach 15% of dynamical range at low redshift and reduce overestimates of old galaxy fractions by up to 10%.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2verdicts
UNVERDICTED 2representative citing papers
Early-type galaxies in dense environments have less dark matter (upper limit 55-75% of dynamical mass) than those in low-density environments.
citing papers explorer
-
Correcting the fiber-aperture bias affecting galaxy stellar populations in the Sloan Digital Sky Survey. Aperture corrections to absorption indices based on CALIFA integral field observations
Empirical aperture corrections for SDSS absorption indices, derived via CALIFA simulations, reach 15% of dynamical range at low redshift and reduce overestimates of old galaxy fractions by up to 10%.
-
The quantity of dark matter in early-type galaxies and its relation to the environment
Early-type galaxies in dense environments have less dark matter (upper limit 55-75% of dynamical mass) than those in low-density environments.