AKARI Spectroscopic Study of the Rest-frame Optical Spectra of Quasars at 3 < z < 5

  • Jun, Hyun-Sung (CEOU/Dept. of Physics and Astronomy, Seoul National University) ;
  • Im, Myung-Shin (CEOU/Dept. of Physics and Astronomy, Seoul National University) ;
  • Lee, Hyung-Mok (CEOU/Dept. of Physics and Astronomy, Seoul National University) ;
  • QSONG team, QSONG team (CEOU/Dept. of Physics and Astronomy, Seoul National University)
  • Published : 2010.04.06

Abstract

We present the initial results of rest-frame optical spectroscopy of quasars at 3 < z < 5 from the AKARI space telescope mission program QSONG (Quasar Spectroscopic Observation with NIR Grism). QSONG is an AKARI phase-3 mission program which utilizes the unique capability of spectroscopy at 2.5-5 microns, and is adequate for detecting redshifted Balmer lines. We focus on how to overcome the noise induced from instrumental degradation, and report our measurements of supermassive black hole (SMBH) masses with well calibrated optical mass estimators.

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