1997
DOI: 10.1023/a:1004246318082
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Cited by 9 publications
(4 citation statements)
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“…Following the same procedure as above, we measure the aperture correction from a composite PSF of 15 unsaturated point sources in each IRAC image. We measure aperture corrections of f tot (λ) / f ap (λ) = 1.49 -1.89, in the 3.6-8.0 µm wave-bands, which are consistent with those estimated by the SWIRE team (Surace et al 2005).…”
Section: Photometrysupporting
confidence: 81%
“…Following the same procedure as above, we measure the aperture correction from a composite PSF of 15 unsaturated point sources in each IRAC image. We measure aperture corrections of f tot (λ) / f ap (λ) = 1.49 -1.89, in the 3.6-8.0 µm wave-bands, which are consistent with those estimated by the SWIRE team (Surace et al 2005).…”
Section: Photometrysupporting
confidence: 81%
“…Both the Spitzer photometry and spectroscopy of high redshift sources capture the light of the entire source, because high redshift sources are unresolved and fall within the entrance slit of the IRS. For local ULIRGs, on the other hand, the IRS entrance slit usually includes most of the MIR flux (Soifer et al 2000;Armus et al 2006;Surace et al 2007), but is much smaller than the near-IR extent (Scoville et al 2000). Therefore, for the local ULIRGs in Fig.…”
Section: The 16 µM Bump Vs Pah Emissionmentioning
confidence: 99%
“…Fazio et al 2004). The SWIRE number counts will be discussed by Shupe et al (2006) and Surace et al (2006). Spectroscopic or photometric redshifts permit a more direct understanding of the properties of galaxies through, the study of luminosity functions (e.g.…”
Section: Introductionmentioning
confidence: 99%