Image Details

Choose export citation format:

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 5.

Multi-band images of an IRAC-selected source (irac096525) in the [3.6], R, I, and i 814 bands (from left to right and top to bottom). The size of the frames is 15'' ×15''. In the three optical bands, the flux is measured in elliptical apertures (red) whose parameters are determined in the R-band image. Note that, despite the different image resolutions (and multiple HST counterparts), the accurate WCS re-centering (rms < 0 farcs15) allows to place the aperture correctly, recovering the flux of all sources. For the IRAC bands, we use fixed circular apertures of 2'' radius (blue) and we apply a correction to the total magnitude.

Other Images in This Article

Show More

Copyright and Terms & Conditions