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Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). VI. Black Hole Mass Measurements of Six Quasars at 6.1 ≤ z ≤ 6.7

  • Authors: Masafusa Onoue, Nobunari Kashikawa, Yoshiki Matsuoka, Nanako Kato, Takuma Izumi, Tohru Nagao, Michael A. Strauss, Yuichi Harikane, Masatoshi Imanishi, Kei Ito, Kazushi Iwasawa, Toshihiro Kawaguchi, Chien-Hsiu Lee, Akatoki Noboriguchi, Hyewon Suh, Masayuki Tanaka, and Yoshiki Toba

2019 The Astrophysical Journal 880 77.

  • Provider: AAS Journals

Caption: Figure 1.

Optical-to-NIR spectra of the six HSC quasars in this paper. The top three panels show the X-Shooter spectra of J1205−0000, J0859+0022, and J1152+0059. The next three show the GNIRS spectra of J2239+0207, J1208−0200, and J2216−0016, while their optical data (λobs ≲ 1 μm) are from the discovery spectra (Matsuoka et al. 2016, 2018b). The bottom panel shows the atmospheric transmission at Maunakea retrieved from the Gemini Observatory (Lord 1992). The vertical lines indicate the central wavelength of broad emission lines expected from the systemic redshift (Mg II redshift for J1205−0000 and [C II] redshift from Izumi et al. 2018, 2019 for the others). In each panel, the noise spectra are shown in gray, and the best-fit power-law continuum models are shown in blue.

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