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A Systematic Study of the Long-term Mid-infrared Color Variations of Seyfert 1 Galaxies

  • Authors: Jiahua Wu, Liming Dou, Zhining Chen, Fupeng Zhang, Luis C. Ho, Yanli Ai, Tinggui Wang, Xinwen Shu, Ning Jiang, Junfeng Wang

Jiahua Wu et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 3.

Correlations between the MCV coefficient ρPearson and MIR variability properties. (a)–(d) ρPearson vs. intrinsic variability amplitude σm in the W1 and W2 bands for NLSy1s and BLSy1s. (e)–(f) ρPearson vs. mean MIR color ﹩\left\langle {\rm{W}}1-{\rm{W}}2\right\rangle ﹩. (g)–(h) ρPearson vs. the host-contamination proxy ﹩r-\left\langle {\rm{W}}1\right\rangle ﹩. Purple and orange points denote RQ NLSy1s and RQ BLSy1s, respectively; red diamonds indicate RL counterparts. Dashed lines represent linear regression fits for the RQ populations.

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