Erratum : On the diversity of superluminous supernovae: ejected mass as the dominant factor (vol 452, pg 3869, 2015)

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 (vol 452, pg 3869, 2015)

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

Department of Particle Physics and Astrophysics

Weizmann Institute of Science

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

Abstract

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
Early online date	11 Feb 2016
DOIs	https://doi.org/10.1093/mnras/stw160
State	Published - 11 Apr 2016

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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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 (vol 452, pg 3869, 2015). MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 457(3), 2514-2515. Article stw124. https://doi.org/10.1093/mnras/stw160

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title = "Erratum : On the diversity of superluminous supernovae: ejected mass as the dominant factor (vol 452, pg 3869, 2015)",

abstract = "We have noticed that some of the supernova peak magnitudes in Table 1 are given in the wrong rows. The error affected the rows {\textquoteleft}PS1-11ap{\textquoteright} to {\textquoteleft}PS1-10ky{\textquoteright}, 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 {\textquoteleft}Gold{\textquoteright} coverage group. This does not affect any of the other tables, figures, or analysis in the paper.",

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 \{Della Valle\}, M. and N. Elias-Rosa and U. Feindt and L. Galbany and E. Hadjiyska and \{Le Guillou\}, L. 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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doi = "10.1093/mnras/stw160",

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Nicholl, M, Smartt, SJ, Jerkstrand, A, Inserra, C, Sim, SA, Chen, T-W, 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, M-T, Childress, M, Dennefeld, M, Della Valle, M, 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, BP, Schulze, S, Sollerman, J, Taddia, F & Yuan, F 2016, 'Erratum : On the diversity of superluminous supernovae: ejected mass as the dominant factor (vol 452, pg 3869, 2015)', 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 : On the diversity of superluminous supernovae: ejected mass as the dominant factor (vol 452, pg 3869, 2015)

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 - Della Valle, M.

AU - Elias-Rosa, N.

AU - Feindt, U.

AU - Galbany, L.

AU - Hadjiyska, E.

AU - Le Guillou, L.

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.

N1 - NA

PY - 2016/4/11

Y1 - 2016/4/11

N2 - 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 - 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.

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U2 - 10.1093/mnras/stw160

DO - 10.1093/mnras/stw160

M3 - تعليقَ / نقاش

SN - 0035-8711

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EP - 2515

JO - MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

JF - MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

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M1 - stw124

ER -

Erratum : On the diversity of superluminous supernovae: ejected mass as the dominant factor (vol 452, pg 3869, 2015)

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