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Two more, bright, z > 6 quasars from VST ATLAS and WISE

MPS-Authors

Chehade,  B.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Carnall,  A. C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Shanks,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Diener,  C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Fumagalli,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Findlay,  J. R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Metcalfe,  N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hennawi,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Leibler,  C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Murphy,  D. N. A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Prochaska,  J. X.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Irwin,  M. J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Gonzalez-Solares,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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Citation

Chehade, B., Carnall, A. C., Shanks, T., Diener, C., Fumagalli, M., Findlay, J. R., et al. (2018). Two more, bright, z > 6 quasars from VST ATLAS and WISE. Monthly Notices of the Royal Astronomical Society, 478, 1649-1659.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CE76-F
Abstract
Recently, Carnall et al. discovered two bright high-redshift quasars using the combination of the Very Large Telescope (VLT) Survey Telescope (VST) ATLAS and Wide-field Infrared Survey Explorer (WISE) surveys. The technique involved using the 3D colour plane i-z : z-W1 : W1-W2 with the WISE W1 (3.4 micron) and W2 (4.5 micron) bands taking the place of the usual NIR J band to help decrease stellar dwarf contamination. Here, we report on our continued search for 5.7 < z < 6.4 quasars over an ≈2 × larger area of ≈3577 deg2 of the Southern Hemisphere. We have found two further z > 6 quasars, VST-ATLAS J158.6938-14.4211 at z = 6.07 and J332.8017-32.1036 at z = 6.32 with magnitudes of zAB = 19.4 and 19.7 mag, respectively. J158.6938-14.4211 was confirmed by Keck LRIS observations and J332.8017-32.1036 was confirmed by ESO NTT EFOSC-2 observations. Here, we present VLT X-shooter visible and NIR spectra for the four ATLAS quasars. We have further independently rediscovered two z > 5.7 quasars previously found by the VIKING/KiDS and PanSTARRS surveys. This means that in ATLAS we have now discovered a total of six quasars in our target 5.7 < z < 6.4 redshift range. Making approximate corrections for incompleteness, we find that our quasar space density agrees with the Sloan Digital Sky Survey results of Jiang et al. at M1450 Å ≈ -27. Preliminary virial mass estimates based on the C IV and Mg II emission lines give black hole masses in the range MBH ≈ 1-6 × 109 M for the four ATLAS quasars.