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- W2892425478 abstract "We compile multi-wavelength data from ultraviolet to infrared (IR) bands as well as redshift and source-type information, for a large sample of 178 341 sources in the Hawaii-Hubble Deep Field-North field. A total of 145 635 sources among the full sample are classified/treated as galaxies and have redshift information available. We derive physical properties for these sources utilizing the spectral energy distribution fitting code CIGALE that is based on Bayesian analysis. Through various consistency and robustness checks, we find that our stellar-mass and star-formation rate (SFR) estimates are reliable, which is mainly due to two facts. Firstly, we adopt the most up-to-date and accurate redshifts and point spread function-matched photometry; and secondly, we make sensible parameter choices with the CIGALE code and take into account the influences of mid-IR/far-IR data, star-formation history models, and AGN contribution. We release our catalog of galaxy properties publicly (including, e.g., redshift, stellar mass, SFR, age, metallicity, dust attenuation). It is the largest of its kind in this field and should facilitate future relevant studies on the formation and evolution of galaxies." @default.
- W2892425478 created "2018-10-05" @default.
- W2892425478 creator A5033353788 @default.
- W2892425478 creator A5034612131 @default.
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- W2892425478 date "2019-03-01" @default.
- W2892425478 modified "2023-09-25" @default.
- W2892425478 title "Galaxy properties derived with spectral energy distribution fitting in the Hawaii-Hubble Deep Field-North" @default.
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- W2892425478 doi "https://doi.org/10.1088/1674-4527/19/3/39" @default.
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