Erratum: Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5 (Astrophysical Journal (2014) 795 (104) DOI: 10.1088/0004-637x/795/2/104)

Katherine E. Whitaker; Marijn Franx; Joel Leja; Pieter G. Van Dokkum; Alaina Henry; Rosalind E. Skelton; Mattia Fumagalli; Ivelina G. Momcheva; Gabriel B. Brammer; Ivo Labbé; Erica J. Nelson; Jane R. Rigby

doi:10.3847/1538-4357/ab98fc

Erratum: Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5 (Astrophysical Journal (2014) 795 (104) DOI: 10.1088/0004-637x/795/2/104)

Katherine E. Whitaker, Marijn Franx, Joel Leja, Pieter G. Van Dokkum, Alaina Henry, Rosalind E. Skelton, Mattia Fumagalli, Ivelina G. Momcheva, Gabriel B. Brammer, Ivo Labbé, Erica J. Nelson, Jane R. Rigby

Astronomy & Astrophysics

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

2 Scopus citations

Abstract

The level of precision of the polynomial coefficients in Table 1 is not adequate to reproduce the best-fit lines accurately in Figures 1 and 2 of the published article. This erratum provides an update to values in Table 1. (Table Presented).

Original language	English (US)
Article number	175
Journal	Astrophysical Journal
Volume	896
Issue number	2
DOIs	https://doi.org/10.3847/1538-4357/ab98fc
State	Published - Jun 20 2020

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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Whitaker, K. E., Franx, M., Leja, J., Van Dokkum, P. G., Henry, A., Skelton, R. E., Fumagalli, M., Momcheva, I. G., Brammer, G. B., Labbé, I., Nelson, E. J., & Rigby, J. R. (2020). Erratum: Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5 (Astrophysical Journal (2014) 795 (104) DOI: 10.1088/0004-637x/795/2/104). Astrophysical Journal, 896(2), Article 175. https://doi.org/10.3847/1538-4357/ab98fc

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abstract = "The level of precision of the polynomial coefficients in Table 1 is not adequate to reproduce the best-fit lines accurately in Figures 1 and 2 of the published article. This erratum provides an update to values in Table 1. (Table Presented).",

author = "Whitaker, {Katherine E.} and Marijn Franx and Joel Leja and {Van Dokkum}, {Pieter G.} and Alaina Henry and Skelton, {Rosalind E.} and Mattia Fumagalli and Momcheva, {Ivelina G.} and Brammer, {Gabriel B.} and Ivo Labb{\'e} and Nelson, {Erica J.} and Rigby, {Jane R.}",

year = "2020",

month = jun,

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doi = "10.3847/1538-4357/ab98fc",

language = "English (US)",

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Whitaker, KE, Franx, M, Leja, J, Van Dokkum, PG, Henry, A, Skelton, RE, Fumagalli, M, Momcheva, IG, Brammer, GB, Labbé, I, Nelson, EJ & Rigby, JR 2020, 'Erratum: Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5 (Astrophysical Journal (2014) 795 (104) DOI: 10.1088/0004-637x/795/2/104)', Astrophysical Journal, vol. 896, no. 2, 175. https://doi.org/10.3847/1538-4357/ab98fc

TY - JOUR

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T2 - Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5 (Astrophysical Journal (2014) 795 (104) DOI: 10.1088/0004-637x/795/2/104)

AU - Whitaker, Katherine E.

AU - Franx, Marijn

AU - Leja, Joel

AU - Van Dokkum, Pieter G.

AU - Henry, Alaina

AU - Skelton, Rosalind E.

AU - Fumagalli, Mattia

AU - Momcheva, Ivelina G.

AU - Brammer, Gabriel B.

AU - Labbé, Ivo

AU - Nelson, Erica J.

AU - Rigby, Jane R.

PY - 2020/6/20

Y1 - 2020/6/20

N2 - The level of precision of the polynomial coefficients in Table 1 is not adequate to reproduce the best-fit lines accurately in Figures 1 and 2 of the published article. This erratum provides an update to values in Table 1. (Table Presented).

AB - The level of precision of the polynomial coefficients in Table 1 is not adequate to reproduce the best-fit lines accurately in Figures 1 and 2 of the published article. This erratum provides an update to values in Table 1. (Table Presented).

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SN - 0004-637X

VL - 896

JO - Astrophysical Journal

JF - Astrophysical Journal

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Erratum: Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5 (Astrophysical Journal (2014) 795 (104) DOI: 10.1088/0004-637x/795/2/104)

Abstract

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