Photometric Redshifts in the Hawaii-Hubble Deep Field-North (H-HDF-N)
G. Yang, Y. Q. Xue, B. Luo, W. N. Brandt, D. M. Alexander, F. E., Bauer, W. Cui, X. Kong, B. D. Lehmer, J.-X. Wang, X.-B. Wu, F. Yuan, Y.-F., Yuan, H. Y. Zhou

TL;DR
This paper presents a comprehensive catalog of photometric redshifts for over 130,000 sources in the Hawaii-Hubble Deep Field-North, utilizing multi-band photometry and improved methods for accuracy and classification.
Contribution
The study provides an extensive, high-quality photometric redshift catalog with improved accuracy, classification, and matching to X-ray data, covering the entire H-HDF-N field.
Findings
Achieved a normalized median absolute deviation of 0.029 for photometric redshifts.
Reduced outlier fraction to 5.5% for non-X-ray sources.
Enhanced redshift accuracy for X-ray sources by incorporating additional AGN templates.
Abstract
We derive photometric redshifts (\zp) for sources in the entire ( deg) Hawaii-Hubble Deep Field-North (\hdfn) field with the EAzY code, based on point spread function-matched photometry of 15 broad bands from the ultraviolet (\bandu~band) to mid-infrared (IRAC 4.5 m). Our catalog consists of a total of 131,678 sources. We evaluate the \zp~quality by comparing \zp~with spectroscopic redshifts (\zs) when available, and find a value of normalized median absolute deviation \sigm0.029 and an outlier fraction of 5.5\% (outliers are defined as sources having ) for non-X-ray sources. More specifically, we obtain \sigm with 2.7\% outliers for sources brighter than ~mag, \sigm with 7.4\% outliers for sources fainter than ~mag, \sigm0.026 with 3.9\% outliers for sources having , and \sigm0.034 with 9.0\%…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Astronomical Observations and Instrumentation · Stellar, planetary, and galactic studies
