Journal article
The intrinsic far-UV spectrum of the high-redshift quasar B1422 231
M O'Dowd, NF Bate, RL Webster, K Labrie, AL King, SY Yong
Monthly Notices of the Royal Astronomical Society | OXFORD UNIV PRESS | Published : 2018
Abstract
We present new spectroscopy of the z = 3.62 gravitationally lensed quasar B1422+117 from the Gemini North GMOS integral field spectrograph. We observe significant differential magnifications between the broad emission lines and the continuum, as well as across the velocity structure of the Lyman-a line. We take advantage of this differential microlensing to algebraically decompose the quasar spectrum into the absorbed broad emission line and absorbed continuum components.We use the latter to derive the intrinsic Ly α forest absorption spectrum. The proximity effect is clearly detected, with a proximity zone edge of 8.6-17.3Mpc from the quasar, implying (perhaps intermittent) activity over at..
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Awarded by National Science Foundation
Funding Acknowledgements
Based on observations obtained at the Gemini Observatory (Program ID GN-2006A-Q-15, processed using the Gemini IRAF package), which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina), and Ministerio da Ciencia, Tecnologia e Inovacao (Brazil).