Uv-to-fir analysis of spitzer/irac sources in the extended groth strip i: Multi-wavelength photometry and spectral energy distributions
Guillermo Barro, P.G. Perez-Gonzalez, J. Gallego, M. L. N. Ashby, M., Kajisawa, S. Miyazaki, V.Villar, T. Yamada, J. Zamorano

TL;DR
This paper presents a comprehensive multi-wavelength catalog of sources in the Extended Groth Strip, including photometry from UV to FIR, and describes the methodology for constructing spectral energy distributions for these sources.
Contribution
It introduces a new IRAC-selected catalog with detailed multi-wavelength photometry and robust SED construction for over 76,000 sources in the EGS.
Findings
Catalog contains 76,936 sources with extensive photometry.
Most sources are detected in optical and near-infrared bands.
The data enables detailed analysis of stellar parameters and galaxy properties.
Abstract
We present an IRAC 3.6+4.5 microns selected catalog in the Extended Groth Strip (EGS) containing photometry from the ultraviolet to the far-infrared and stellar parameters derived from the analysis of the multi-wavelength data. In this paper, we describe the method used to build coherent spectral energy distributions (SEDs) for all the sources. In a companion paper, we analyze those SEDs to obtain robust estimations of stellar parameters such as photometric redshifts, stellar masses, and star formation rates. The catalog comprises 76,936 sources with [3.6]<23.75 mag (85% completeness level of the IRAC survey in the EGS) over 0.48 square degrees. For approximately 16% of this sample, we are able to deconvolve the IRAC data to obtain robust fluxes for the multiple counterparts found in ground-based optical images. Typically, the SEDs of the IRAC sources in our catalog count with more than…
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