Figure 10 from FLASH SPECTROSCOPY: EMISSION LINES FROM THE IONIZED CIRCUMSTELLAR MATERIAL AROUND <10-DAY-OLD TYPE II SUPERNOVAE

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FLASH SPECTROSCOPY: EMISSION LINES FROM THE IONIZED CIRCUMSTELLAR MATERIAL AROUND <10-DAY-OLD TYPE II SUPERNOVAE

Authors: D. Khazov, O. Yaron, A. Gal-Yam, I. Manulis, A. Rubin, S. R. Kulkarni, I. Arcavi, M. M. Kasliwal, E. O. Ofek, Y. Cao, D. Perley, J. Sollerman, A. Horesh, M. Sullivan, A. V. Filippenko, P. E. Nugent, D. A. Howell, S. B. Cenko, J. M. Silverman, H. Ebeling, F. Taddia, J. Johansson, R. R. Laher, J. Surace, U. D. Rebbapragada, P. R. Wozniak, and T. Matheson

2016 The Astrophysical Journal 818 3.

Provider: AAS Journals

Caption: Figure 10.

Time between the first spectrum and the estimated explosion time vs. the redshift. The error bars are between the times of the first detection and the pre-explosion limit (which is the same as the estimated explosion time for the SNe with fitted rise time). Note the lack of distant SNe that are not classified as BF or FI events.

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