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. Author manuscript; available in PMC: 2019 Jul 19.
Published in final edited form as: Astron Astrophys. 2019 May 29;625:A147. doi: 10.1051/0004-6361/201935164

Fig. 2.

Fig. 2

Overview of the λ 3 mm line survey of L483 covering the frequency range 80-116 GHz. The carriers of the most intense lines are indicated. Negative signals correspond to the artifacts caused by the frequency-switching technique.