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19 April 2024
 
  » arxiv » 1901.0013

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Near-Infrared Survey and Photometric Redshifts in the Extended GOODS-North field
Li-Ting Hsu ; Lihwai Lin ; Mark Dickinson ; Haojing Yan ; Hsieh Bau-Ching ; Wei-Hao Wang ; Chien-Hsiu Lee ; Chi-Hung Yan ; Douglas Scott ; S. P. Willner ; Masami Ouchi ; Matthew L. N. Ashby ; Yi-Wen Chen ; Emanuele Daddi ; David Elbaz ; Giovanni G. Fazio ; Sebastien Foucaud ; Jiasheng Huang ; David C. Koo ; Glenn Morrison ; Frazer Owen ; Maurilio Pannella ; Alexendra Pope ; Luc Simard ; Shiang-Yu Wang ;
Date 31 Dec 2018
AbstractWe present deep $J$ and $H$-band images in the extended Great Observatories Origins Deep Survey-North (GOODS-N) field covering an area of 0.22 $ m{deg}^{2}$. The observations were taken using WIRCam on the 3.6-m Canada France Hawaii Telescope (CFHT). Together with the reprocessed $K_{ m s}$-band image, the $5sigma$ limiting AB magnitudes (in 2" diameter apertures) are 24.7, 24.2, and 24.4 AB mag in the $J$, $H$, and $K_{ m s}$ bands, respectively. We also release a multi-band photometry and photometric redshift catalog containing 93598 sources. For non-X-ray sources, we obtained a photometric redshift accuracy $sigma_{mathrm{NMAD}}=0.036$ with an outlier fraction $eta = 7.3\%$. For X-ray sources, which are mainly active galactic nuclei (AGNs), we cross-matched our catalog with the updated 2M-CDFN X-ray catalog from Xue et al. (2016) and found that 658 out of 683 X-ray sources have counterparts. $GALEX$ UV data are included in the photometric redshift computation for the X-ray sources to give $sigma_{mathrm{NMAD}} = 0.040$ with $eta=10.5\%$. Our approach yields more accurate photometric redshift estimates compared to previous works in this field. In particular, by adopting AGN-galaxy hybrid templates, our approach delivers photometric redshifts for the X-ray counterparts with fewer outliers compared to the 3D-HST catalog, which fit these sources with galaxy-only templates.
Source arXiv, 1901.0013
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