INT H?

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INT H? imaging (Pérez et al.)
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Atmospheric parameters coverage of different
libraries compared with the parameter coverage of
MILES
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Spectra sample of different spectral types
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A Near-Infrared Stellar Library for Stellar
Population Synthesis
E. Marmol, N. Cardiel, F.J. Gorgas, E. Toloba (UC
Madrid) R.F. Peletier, K. Ganda (Groningen) V.
Ivanov (ESO, Chile) M. Mouhcine (Nottingham,
Liverpool) A. Vazdekis (IAC)
Aim Generate a flux-calibrated stellar library
in the H and K band (1.4-2.4
micron) Summary We take the high-resolution
stellar library of Ivanov et al. (2004)
and obtain low-resolution spectra to
flux-calibrate these. We then make SSP
models using the codes of Vazdekis and
Mouhcine and Lancon.
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Status Dec 06 - 106/210 stars observed with
UKIRT and reduced - 60/210 stars observed with
LIRIS/WHT - 44/210 stars to be done 1 night of
LIRIS allocated in 07A SSP model calculation to
be started
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Stellar Population Work using SAURON
Studies - 18 bright Sb-Sd galaxies. Kinematics
published in Ganda et al. (2006), stellar
population analysis in Ganda et al. (2007) -
Stellar population analysis of 24 early-type
spirals using SAURON (Peletier et al. 2006, to
be submitted)