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                  <mods:namePart>Takahashi, A.</mods:namePart>
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                  <mods:namePart>Matsuoka, Y.</mods:namePart>
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                  <mods:namePart>Onoue, M.</mods:namePart>
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                  <mods:namePart>Strauss, M. A.</mods:namePart>
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                  <mods:namePart>Kashikawa, N.</mods:namePart>
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                  <mods:namePart>Toba, Y.</mods:namePart>
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                  <mods:namePart>Iwasawa, Kazushi</mods:namePart>
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                  <mods:namePart>Imanishi, M.</mods:namePart>
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                  <mods:namePart>Akiyama, M.</mods:namePart>
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                  <mods:namePart>Kawaguchi, T.</mods:namePart>
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                  <mods:namePart>Noboriguchi, A.</mods:namePart>
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                  <mods:namePart>Lee, C.-H.</mods:namePart>
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                  <mods:dateIssued encoding="iso8601">2025-01-30T17:14:27Z2025-01-30T17:14:27Z20242025-01-30T17:14:27Z</mods:dateIssued>
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               <mods:abstract>We report the distribution of black hole (BH) masses and Eddingont ratios estimated for a sample of 131 low luminosity quasars in the early cosmic epoch (5.6 &lt; z &lt; 7.0). Our work is based on the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, which has constructed a low luminosity quasar sample down to M1450 ∼ − 21 mag, exploiting the survey data of Hyper Suprime-Cam installed on Subaru Telescope. The discovery spectra of these quasars are limited to the rest-frame wavelengths of ∼1200–1400 Å, which contain no emission lines that can be used as BH mass estimators. In order to overcome this problem, we made use of low-z counterpart spectra from the Sloan Digital Sky Survey, which are spectrally matched to the high-z spectra in overlapping wavelengths. We then combined the C iv emission line widths of the counterparts with the continuum luminosity from the SHELLQs data to estimate BH masses. The resulting BH mass distribution has a range of ∼107–10M⊙, with most of the quasars having BH masses ∼108M⊙ with sub-Eddington accretion. The present study provides not only a new insight into normal quasars in the reionization epoch, but also a new promising way to estimate BH masses of high-z quasars without near-infrared spectroscopy.</mods:abstract>
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               <mods:accessCondition type="useAndReproduction">(c) American Astronomical Society, 2024 info:eu-repo/semantics/openAccess</mods:accessCondition>
               <mods:subject>
                  <mods:topic>Forats negres (Astronomia)</mods:topic>
               </mods:subject>
               <mods:subject>
                  <mods:topic>Galàxies</mods:topic>
               </mods:subject>
               <mods:subject>
                  <mods:topic>Quàsars</mods:topic>
               </mods:subject>
               <mods:subject>
                  <mods:topic>Black holes (Astronomy)</mods:topic>
               </mods:subject>
               <mods:subject>
                  <mods:topic>Galaxies</mods:topic>
               </mods:subject>
               <mods:subject>
                  <mods:topic>Quasars</mods:topic>
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                  <mods:title>Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at z 6 Estimated via Spectral Comparison with Low-z Quasars</mods:title>
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