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METHOD:PUBLISH
BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20110512T000000
DTEND;TZID=Atlantic/Canary:20110512T010000
UID:iactalks-276
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/276
CREATED:2011-05-12T00:00:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Spectral Energy Distributions of Single Stellar Populations in the 
 Infrared range
DESCRIPTION:Spectral Energy Distributions of Single Stellar Populations in 
 the Infrared range\nMiss Sofia Meneses-Goytia\n\nThe present work shows th
 e Spectral Energy Distributions (SEDs) in the near-infrared using the IRTF
  stellar library obtained using the models based on the Single Stellar pop
 ulation Models (SSP) from Vazdekis et al. (1996 - 2010) which work in the 
 optical, and use the CaT and MILES stellar libraries. In this near-infrare
 d research, the isochrones of Marigo et al. (2008) were chosen and which h
 ave a range of metallicity [Fe/H] between -2.27 and 0.019, and ages up to 
 15.85 Gy. Also, they provide the corresponding ?uxes in the IR bands I to 
 M (0.7 to 5.0 microns). The IRTF stellar library contains spectra of 292 s
 tars (F, G, K and M stars) at a resolution of 2000, between 0.8 to 5.2 mic
 rons. The features of the SED (spectrum obtained by the integration of the
  spectra of the stars, at constant metallicity and age) are analysed by co
 mparing to those found on Ivanov et al. (2004) for the IR range. In additi
 on, t he comparison of the models with galaxy observations of early type g
 alaxies by Marmol-Queralto et al. (2009) are presented.
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