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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 11.

The CMD (gr vs. Mr) of the MIRONG sample (blue filled circles). The magnitudes and color are displayed after correction for Galactic dust extinction and k-correction to z = 0.1. We denote the four SN host galaxies in red. Contours show the density of low-redshift (z < 0.2) SDSS DR7 spectroscopic galaxies. The contour lines correspond to 5, 25, 100, 400, 2000, 5000, and 8000 galaxies bin–1 of Δ(gr) = 0.1 and ΔMr = 0.1. The magenta dashed line is the assigned line of demarcation between the blue clouds and red sequence. We have also plotted the optical TDEs (van Velzen et al. 2020) for comparison (green squares), in which the magnitudes are from either SDSS or Pan-STARRS.

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