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A New Framework for Multiline Analysis Combined Kernel Principal Component Analysis and Kernel Shapley Additive Explanations: A Case of NGC 1068 ALMA Band 3 Data

  • Authors: Hiroma Okubo, Tsutomu T. Takeuchi, Shotaro Akaho, Toshiki Saito, Yasuhiko Igarashi, Nario Kuno, Nanase Harada, Akio Taniguchi, Shuro Takano, Taku Nakajima

Hiroma Okubo et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

The integrated intensity maps of NGC 1068. The left panel presents the 13CO(J = 1–0) integrated intensity map. The crosses indicate the positions of the SSC, SHC, and Paα regions defined in F. Rico-Villas et al. (2021). Note that the circle marking the starburst ring is not a strict definition, but only shows its approximate location. The middle and right panels show the CS(J = 2–1) and HNC(J = 1–0) integrated intensity maps, respectively. The central circle indicates the field of view (FoV) of the [C I] data. The region outlined with dotted arrows marks the direction of the molecular outflow (T. Saito et al. 2022a, 2022b). The diameter of the circle is 1 kpc.

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