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Erratum: On the diversity of superluminous supernovae: ejected mass as the dominant factor

Nicholl, M., Smartt, S. J., Jerkstrand, A., Inserra, C., Sim, S. A., Chen, T.-W., Benetti, S., Fraser, M., Gal-Yam, A., Kankare, E., Maguire, K., Smith, K., Sullivan, M., Valenti, S., Young, D. R., Baltay, C., Bauer, F. E., Baumont, S., Bersier, D., Botticella, M.-T., Childress, M., Dennefeld, M., Valle, M. Della, Elias-Rosa, N., Feindt, U., Galbany, L., Hadjiyska, E., Le Guillou, L., Leloudas, G., Mazzali, P., McKinnon, R., Polshaw, J., Rabinowitz, D., Rostami, S., Scalzo, R., Schmidt, B. P., Schulze, S., Sollerman, J., Taddia, F. and Yuan, F. 2016. Erratum: On the diversity of superluminous supernovae: ejected mass as the dominant factor. Monthly Notices of the Royal Astronomical Society 457 (3) , pp. 2514-2515. 10.1093/mnras/stw160

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Abstract

This is an erratum to the paper ‘On the diversity of superluminous supernovae: ejected mass as the dominant factor’, published in MNRAS, 2015, 452. We have noticed that some of the supernova peak magnitudes in Table 1 are given in the wrong rows. The error affected the rows ‘PS1-11ap’ to ‘PS1-10ky’, with each magnitude displaced downwards by one cell. The nature of this error is purely typographic. Originally, the objects were grouped into high- and low-redshift bins, rather than by wavelength coverage; the error occurred when moving PS1-11ap from the high-z group into the ‘Gold’ coverage group. This does not affect any of the other tables, figures, or analysis in the paper.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Publisher: Oxford University Press
ISSN: 0035-8711
Date of First Compliant Deposit: 23 January 2019
Date of Acceptance: 15 January 2016
Last Modified: 31 Jan 2019 11:28
URI: http://orca.cf.ac.uk/id/eprint/118731

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