Erratum: "On the diversity of superluminous supernovae: Ejected mass as the dominant factor" [MNRAS 457, 2514-2515 (2016)]

M. Nicholl; S. J. Smartt; A. Jerkstrand; C. Inserra; S. A. Sim; T. W. Chen; S. Benetti; M. Fraser; A. Gal-Yam; E. Kankare; K. Maguire; K. Smith; M. Sullivan; S. Valenti; D. R. Young; C. Baltay; F. E. Bauer; S. Baumont; D. Bersier; M. T. Botticella; M. Childress; M. Dennefeld; M. Della Valle; N. Elias-Rosa; U. Feindt; L. Galbany; E. Hadjiyska; L. Le Guillou; G. Leloudas; P. Mazzali; R. McKinnon; J. Polshaw; D. Rabinowitz; S. Rostami; R. Scalzo; B. P. Schmidt; S. Schulze; J. Sollerman; F. Taddia; F. Yuan

doi:10.1093/mnras/stw160

Erratum: "On the diversity of superluminous supernovae: Ejected mass as the dominant factor" [MNRAS 457, 2514-2515 (2016)]

M. Nicholl^*, S. J. Smartt, A. Jerkstrand, C. Inserra, S. A. Sim, T. W. Chen, S. Benetti, M. Fraser, A. Gal-Yam, E. Kankare, K. Maguire, K. Smith, M. Sullivan, S. Valenti, D. R. Young, C. Baltay, F. E. Bauer, S. Baumont, D. Bersier, M. T. BotticellaM. Childress, M. Dennefeld, M. Della Valle, N. Elias-Rosa, U. Feindt, L. Galbany, E. Hadjiyska, L. Le Guillou, G. Leloudas, P. Mazzali, R. McKinnon, J. Polshaw, D. Rabinowitz, S. Rostami, R. Scalzo, B. P. Schmidt, S. Schulze, J. Sollerman, F. Taddia, F. Yuan

^*Corresponding author for this work

Research output: Contribution to journal › Comment/debate › peer-review

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.

Original language	English
Article number	stw124
Pages (from-to)	2514-2515
Number of pages	2
Journal	Monthly Notices of the Royal Astronomical Society
Volume	457
Issue number	3
DOIs	https://doi.org/10.1093/mnras/stw160
Publication status	Published - 11 Apr 2016

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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., ... Yuan, F. (2016). Erratum: "On the diversity of superluminous supernovae: Ejected mass as the dominant factor" [MNRAS 457, 2514-2515 (2016)]. Monthly Notices of the Royal Astronomical Society, 457(3), 2514-2515. Article stw124. https://doi.org/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.",

keywords = "Errata, addenda - supernovae, General - supernovae, Individual, LSQ14bdq - supernovae, LSQ14mo -supernovae, SN 2013hx",

author = "M. Nicholl and Smartt, {S. J.} and A. Jerkstrand and C. Inserra and Sim, {S. A.} and Chen, {T. W.} and S. Benetti and M. Fraser and A. Gal-Yam and E. Kankare and K. Maguire and K. Smith and M. Sullivan and S. Valenti and Young, {D. R.} and C. Baltay and Bauer, {F. E.} and S. Baumont and D. Bersier and Botticella, {M. T.} and M. Childress and M. Dennefeld and Valle, {M. Della} and N. Elias-Rosa and U. Feindt and L. Galbany and E. Hadjiyska and Guillou, {L. Le} and G. Leloudas and P. Mazzali and R. McKinnon and J. Polshaw and D. Rabinowitz and S. Rostami and R. Scalzo and Schmidt, {B. P.} and S. Schulze and J. Sollerman and F. Taddia and F. Yuan",

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Nicholl, M, Smartt, SJ, Jerkstrand, A, Inserra, C, Sim, SA, Chen, TW, Benetti, S, Fraser, M, Gal-Yam, A, Kankare, E, Maguire, K, Smith, K, Sullivan, M, Valenti, S, Young, DR, Baltay, C, Bauer, FE, Baumont, S, Bersier, D, Botticella, MT, Childress, M, Dennefeld, M, Valle, MD, Elias-Rosa, N, Feindt, U, Galbany, L, Hadjiyska, E, Guillou, LL, Leloudas, G, Mazzali, P, McKinnon, R, Polshaw, J, Rabinowitz, D, Rostami, S, Scalzo, R, Schmidt, BP, Schulze, S, Sollerman, J, Taddia, F & Yuan, F 2016, 'Erratum: "On the diversity of superluminous supernovae: Ejected mass as the dominant factor" [MNRAS 457, 2514-2515 (2016)]', Monthly Notices of the Royal Astronomical Society, vol. 457, no. 3, stw124, pp. 2514-2515. https://doi.org/10.1093/mnras/stw160

TY - JOUR

T1 - Erratum

T2 - "On the diversity of superluminous supernovae: Ejected mass as the dominant factor" [MNRAS 457, 2514-2515 (2016)]

AU - Nicholl, M.

AU - Smartt, S. J.

AU - Jerkstrand, A.

AU - Inserra, C.

AU - Sim, S. A.

AU - Chen, T. W.

AU - Benetti, S.

AU - Fraser, M.

AU - Gal-Yam, A.

AU - Kankare, E.

AU - Maguire, K.

AU - Smith, K.

AU - Sullivan, M.

AU - Valenti, S.

AU - Young, D. R.

AU - Baltay, C.

AU - Bauer, F. E.

AU - Baumont, S.

AU - Bersier, D.

AU - Botticella, M. T.

AU - Childress, M.

AU - Dennefeld, M.

AU - Valle, M. Della

AU - Elias-Rosa, N.

AU - Feindt, U.

AU - Galbany, L.

AU - Hadjiyska, E.

AU - Guillou, L. Le

AU - Leloudas, G.

AU - Mazzali, P.

AU - McKinnon, R.

AU - Polshaw, J.

AU - Rabinowitz, D.

AU - Rostami, S.

AU - Scalzo, R.

AU - Schmidt, B. P.

AU - Schulze, S.

AU - Sollerman, J.

AU - Taddia, F.

AU - Yuan, F.

PY - 2016/4/11

Y1 - 2016/4/11

N2 - 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.

AB - 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.

KW - Errata, addenda - supernovae

KW - General - supernovae

KW - Individual

KW - LSQ14bdq - supernovae

KW - LSQ14mo -supernovae

KW - SN 2013hx

UR - http://www.scopus.com/inward/record.url?scp=84976866357&partnerID=8YFLogxK

U2 - 10.1093/mnras/stw160

DO - 10.1093/mnras/stw160

M3 - Comment/debate

SN - 0035-8711

VL - 457

SP - 2514

EP - 2515

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

M1 - stw124

ER -

Erratum: "On the diversity of superluminous supernovae: Ejected mass as the dominant factor" [MNRAS 457, 2514-2515 (2016)]

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