Figure 12 from UV-to-FIR Analysis of Spitzer/IRAC Sources in the Extended Groth Strip. I. Multi-wavelength Photometry and Spectral Energy Distributions

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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 12.

Same as Figure 11 for irac164462, an LBG at z = 2.8. 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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