Fig. 1 from Late‐Time Observations of SN 2006gy: Still Going Strong

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Late‐Time Observations of SN 2006gy: Still Going Strong

Authors: Nathan Smith, Ryan J. Foley, Joshua S. Bloom, Weidong Li, Alexei V. Filippenko, Raphaël Gavazzi, Andrea Ghez, Quinn Konopacky, Matthew A. Malkan, Philip J. Marshall, David Pooley, Tommaso Treu, and Jong-Hak Woo

Smith et al. 2008 The Astrophysical Journal 686 485.

Provider: AAS Journals

Caption: Fig. 1.

False‐color IR image of the core of NGC 1260 and SN 2006gy, generated from Keck LGS/NIRC2 H‐band and ﹩K^{\prime }﹩‐band observations on 2007 December 1. SN 2006gy is red and very luminous in the near‐IR, more than a year after explosion.

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