Statistics – Methodology
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21520209m&link_type=abstract
American Astronomical Society, AAS Meeting #215, #202.09; Bulletin of the American Astronomical Society, Vol. 42, p.294
Statistics
Methodology
Scientific paper
Using infrared photometry from the Spitzer Space Telescope, we perform the first inventory of aromatic feature emission for a large unbiased sample of galaxies in the local volume. The photometric methodology involved is calibrated and demonstrated to recover the aromatic fraction of the IRAC 8 micron flux with a standard deviation of 6% using a training set of 40 SINGS galaxies for which both equivalent photometry and suitable mid-infrared Spitzer IRS spectra were available. The resulting technique is then applied to the 258 galaxies from the Local Volume Legacy (LVL) survey, a large sample dominated by low-luminosity dwarf galaxies for which obtaining comparable MIR spectroscopy is not feasible. We find the total LVL luminosity due to five strong aromatic features in the 8 micron complex to be 2.47E10 solar luminosities with a mean volume density of 8.8E6 solar luminosities per cubic Mpc. Correspondingly, the same values for all mid-infrared aromatic features in the wavelength range 5.5-20 microns are approximately 1.9 times larger. Using oxygen abundances compiled from the literature, we report a correlation between aromatic feature strength and metallicity, albeit one with significant scatter.
LVL Team
Marble Andrew
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