Figure 3 from SDWFS-MT-1: A Self-obscured Luminous Supernova at z ≃ 0.2

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SDWFS-MT-1: A Self-obscured Luminous Supernova at z ≃ 0.2

Authors: Szymon Kozłowski, C. S. Kochanek, D. Stern, J. L. Prieto, K. Z. Stanek, T. A. Thompson, R. J. Assef, A. J. Drake, D. M. Szczygieł, P. R. Woźniak, P. Nugent, M. L. N. Ashby, E. Beshore, M. J. I. Brown, Arjun Dey, R. Griffith, F. Harrison, B. T. Jannuzi, S. Larson, K. Madsen, B. Pilecki, G. Pojmański, J. Skowron, W. T. Vestrand, and J. A. Wren

KOZŁOWSKI et al. 2010 The Astrophysical Journal 722 1624.

Provider: AAS Journals

Caption: Figure 3.

Keck/LRIS rest-frame spectrum (selected parts) of the transient's host galaxy with the major emission lines marked. From the line positions, we find a redshift of z = 0.1907. To derive the metallicity, we measured the fluxes of the [O ii] 3727 Å, [O iii] 4363 Å, [O iii] 4959 Å, [O iii] 5007 Å, and Hβ 4861 Å lines.

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