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UV-to-FIR Analysis of Spitzer/IRAC Sources in the Extended Groth Strip. I. Multi-wavelength Photometry and Spectral Energy Distributions

  • Authors: Guillermo Barro, P. G. Pérez-González, J. Gallego, M. L. N. Ashby, M. Kajisawa, S. Miyazaki, V. Villar, T. Yamada, and J. Zamorano

Barro et al. 2011 The Astrophysical Journal Supplement Series 193 13.

  • Provider: AAS Journals

Caption: Figure 8.

Example of two of the stellarity criteria used in this paper to separate galaxies from stars. Left: B- z vs. z- K for all sources in the catalog. The dashed line depicts the BzK criteria of Daddi et al. (2004) to isolate stars. The solid lines delimit the regions where high-redshift galaxies are located. The red dots indicate sources satisfying three or more stellarity criteria. Right: comparison of the magnitude in a 3'' radius aperture ([3.6] 3'') and SExtractor MagAuto ([3.6] auto), i.e., the concentration parameter, vs. [3.6] auto for all sources in the catalog. The criterion of Eisenhardt et al. (2004) identifies stars with −0.25 < [3.6] 3'' − [3.6] auto < 0.2 and [3.6] auto < 17.80.

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