RT Journal Article
T1 MILES SSP models
A1 Vazdekis, A.
A1 Sánchez Blázquez, Patricia
A1 Falcón Barroso, J.
A1 Cenarro, A. J.
A1 Beasley, M. A.
A1 Cardiel López, Nicolás
A1 Gorgas García, Francisco Javier
A1 Peletier, R.
AB We present SEDs for single-age, single-metallicity stellar populations (SSPs) covering the full optical spectral range at resolution (FWHM = 2.3Å). These SEDs can be regarded as our base models, as we combine scaled-solar isochrones with an empirical stellar spectral library (MILES), which follows the chemical evolution pattern of the solar neighbourhood. The models rely as much as possible on empirical ingredients as also employ extensive photometric libraries. Thanks to the unprecedented parameter coverage of the MILES library we synthesize SSP SEDs from intermediate- to very-old age regimes, and the metallicity from super-solar to [M/H] = −2.3, all for a suite of IMF shapes and slopes. We propose a new Line Index System (LIS), based on flux-calibrated spectra, to avoid the intrinsic uncertainties associated with the Lick/IDS system and provide more appropriate, uniform, spectral resolution.
PB Cambridge Univ. Press
SN 1743-9213
YR 2009
FD 2009-08
LK https://hdl.handle.net/20.500.14352/43007
UL https://hdl.handle.net/20.500.14352/43007
LA eng
NO © International Astronomical Union 2010. Symposium of the International-Astronomical Union (262nd; 2009; Rio de Janeiro, Brazil).
DS Docta Complutense
RD 7 abr 2025