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Fig. 1

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(a) 1.3 mm continuum image of Orion KL observed with ALMA (#2013.1.00553.S). Contour levels are from 50 mJy−1 beam (5σ) to 950 mJy beam−1 with a 100 mJy beam−1 step. (b) Integrated intensity image of CH318OH (50–40 E) obtained by the ALMA SV. The contour levels are from 4.8 K km s−1 (3σ) to 28.8 K km s−1 with a 4.8 K km s−1 step. The white ellipses in the bottom left corner indicate the synthesized beams. The CH318OH peaks (MeOH1 and MeOH2) are shown by the white squares. The positions of Hot Core (HC), IRc7, and the HCOOCH3 peaks (MF) identified by Favre et al. (2011) are shown by the star, circle, and gray cross marks, respectively. The black cross marks show the positions of dM-1 and dM-3.

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