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No Evidence for Enhanced [O III] 88 μm Emission in a z ∼ 6 Quasar Compared to Its Companion Starbursting Galaxy

  • Authors: Fabian Walter, Dominik Riechers, Mladen Novak, Roberto Decarli, Carl Ferkinhoff, Bram Venemans, Eduardo Bañados, Frank Bertoldi, Chris Carilli, Xiaohui Fan, Emanuele Farina, Chiara Mazzucchelli, Marcel Neeleman, Hans-Walter Rix, Michael Strauss, Bade Uzgil, and Ran Wang

2018 The Astrophysical Journal Letters 869 L22.

  • Provider: AAS Journals

Caption: Figure 3.

[O III]88 emission after continuum subtraction in J2100–Q (top panel) and J2100–SB (bottom panel), integrated over a velocity range of 1.2× FWHM, respectively. Logarithmically spaced contours are shown at ±2, 4, 8σ, with σ = 0.17 mJy beam−1 for J2100–Q and σ = 0.16 mJy beam−1 for J2100–SB. The beam size of 0.″73 × 0.″57 (position angle: 87.°3) is shown in the bottom-left corner.

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