A Point-Source Classification Scheme Using Mid-Infrared Spectra

Details A Point-Source Classification Scheme Using Mid-Infrared Spectra A Point-Source Classification Scheme Using Mid-Infrared Spectra

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21545919w&link_type=abstract

American Astronomical Society, AAS Meeting #215, #459.19; Bulletin of the American Astronomical Society, Vol. 42, p.488

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We have produced a simple but robust classification scheme for point-source targets using mid-infrared spectra. This region of the spectrum is often dominated by dust features, and we utilise these and other spectral features, the overall shape of the spectrum and related information, such as bolometric luminosity and variability, to classify point sources. This scheme has been applied to Spitzer data from the SAGE-Spec project (Kemper et al. 2009) and here we present examples and extend its application to ISO SWS spectra. The classification scheme will also have an application to data from IRAS, Spitzer and the forthcoming MIRI instrument on the JWST.

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