Figure 16 from Mid-infrared Outbursts in Nearby Galaxies (MIRONG). I. Sample Selection and Characterization

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Mid-infrared Outbursts in Nearby Galaxies (MIRONG). I. Sample Selection and Characterization

Authors: Ning Jiang, Tinggui Wang, Liming Dou, Xinwen Shu, Xueyang Hu, Hui Liu, Yibo Wang, Lin Yan, Zhenfeng Sheng, Chenwei Yang, Luming Sun, and Hongyan Zhou

2021 The Astrophysical Journal Supplement Series 252 32.

Provider: AAS Journals

Caption: Figure 16.

Time-resolved W2 magnitudes with date zero-point set as the time of first MIR excess. Our sample has been plotted in solid gray circles with the radio-loud sources and SNe highlighted in blue and red, respectively. We have also overplotted other IR-luminous SNe (orange squares), which are among the brightest known to us, for comparison. The Ia-CSM light curve (green triangles) is drawn from Fox et al. (2013).

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