Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
Utrecht University Repository (Utrecht University)
Abstract
We present a bright galaxy sample with accurate and precise photometric redshifts (photo-zs), selected using $ugriZYJHK_\mathrm{s}$ photometry from the Kilo-Degree Survey (KiDS) Data Release 4 (DR4). The highly pure and complete dataset is flux-limited at $r<20$ mag, covers $\sim1000$ deg$^2$, and contains about 1 million galaxies after artifact masking. We exploit the overlap with Galaxy And Mass Assembly (GAMA) spectroscopy as calibration to determine photo-zs with the supervised machine learning neural network algorithm implemented in the ANNz2 software. The photo-zs have mean error of $|\langle δz \rangle| \sim 5 \times 10^{-4}$ and low scatter (scaled mean absolute deviation of $\sim 0.018(1+z)$), both practically independent of the $r$-band magnitude and photo-z at $0.05 < z_\mathrm{phot} < 0.5$. Combined with the 9-band photometry, these allow us to estimate robust absolute magnitudes and stellar masses for the full sample. As a demonstration of the usefulness of these data we split the dataset into red and blue galaxies, use them as lenses and measure the weak gravitational lensing signal around them for five stellar mass bins. We fit a halo model to these high-precision measurements to constrain the stellar-mass--halo-mass relations for blue and red galaxies. We find that for high stellar mass ($M_\star>5\times 10^{11} M_\odot$), the red galaxies occupy dark matter halos that are much more massive than those occupied by blue galaxies with the same stellar mass. The data presented here are publicly released via the KiDS webpage at http://kids.strw.leidenuniv.nl/DR4/brightsample.php.
Authors 19
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Polish Academy of Sciences (PAN)
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German Centre for Cosmological Lensing
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Leiden University · Leiden Observatory
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Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden, The Netherlands 0000-0001-5434-5942
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Affiliation as printed
German Centre for Cosmological Lensing
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Utrecht University
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Mohammadjavad Vakili Aachen
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Leiden University
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School of Physics and Astronomy
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School of Physics and Astronomy
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University of Edinburgh
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German Centre for Cosmological Lensing
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University of Louisville, Department of Physics and Astronomy, , 102 Natural Sciences Building, Louisville, KY 40292, USA
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Australian Astronomical Optics
Affiliation as printed
Australian Astronomical Optics
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Utrecht University
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Princeton University
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Leiden University · Leiden Observatory
Affiliation as printed
Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden, The Netherlands 0000-0001-5434-5942
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National Centre for Nuclear Research
Affiliation as printed
National Centre for Nuclear Research (NCBJ)
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Shanghai Astronomical Observatory · University of Chinese Academy of Sciences
Affiliation as printed
CAS - Shanghai Astronomical Observatory
UCAS (University of Chinese Academy of Sciences)
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Alessandro Sonnenfeld Aachen
Affiliation as printed
Leiden University
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Affiliation as printed
Astronomy
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