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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 11.

Same as Figure  9 for irac129479, an IR-bright galaxy at z = 1.8. This galaxy corresponds to source EGS11 in the paper of Huang et al. (2009). Band labels in red in the gray-scale postage stamps indicate non-detections. For each of these bands, σ sky is depicted in the UV-to-FIR SED as red arrow. Band labels in green indicate forced photometric measurements (see Section 4.2). These bands are shown as green stars in the SED plot.

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