Erratum: SQuIGGLE: Studying Quenching in Intermediate-z Galaxies-Gas, → AnguLar Momentum, and Evolution (ApJ, (2022) 926 (89) DOI: 10.48550/arXiv.2111.14878

Katherine A. Suess; Mariska Kriek; Rachel Bezanson; Jenny E. Greene; David Setton; Justin S. Spilker; Robert Feldmann; Andy D. Goulding; Benjamin D. Johnson; Joel Leja; Desika Narayanan; Khalil Hall-Hooper; Qiana Hunt; Sidney Lower; Margaret Verrico

doi:10.3847/1538-4357/ac6dde

Erratum: SQuIGGLE: Studying Quenching in Intermediate-z Galaxies-Gas, → AnguLar Momentum, and Evolution (ApJ, (2022) 926 (89) DOI: 10.48550/arXiv.2111.14878

Katherine A. Suess, Mariska Kriek, Rachel Bezanson, Jenny E. Greene, David Setton, Justin S. Spilker, Robert Feldmann, Andy D. Goulding, Benjamin D. Johnson, Joel Leja, Desika Narayanan, Khalil Hall-Hooper, Qiana Hunt, Sidney Lower, Margaret Verrico

Astrophysical Sciences

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Abstract

In the published article, we fit all 1300 galaxies in the SQuIGGLE survey using the Prospector stellar population fitting code (Johnson et al. 2021). We reported logM M in Figure 9 and Table 2 as the total mass formed, the default mass unit used in Prospector. However, logM M values in the literature are typically reported as stellar mass surviving. Surviving stellar mass is smaller than total mass formed by 0.1-0.3 dex due to stellar mass loss throughout a galaxy s lifetime (e.g., Conroy 2013). Figure 1 shows an updated version of the logM M distribution of SQuIGGLE galaxies. Table 1 includes the ID numbers and stellar masses of all galaxies in the SQuIGGLE sample. The median logM M value decreases by 0.2 dex with this unit change from 1011.39Me to 1011.20Me.

Original language	English (US)
Article number	73
Journal	Astrophysical Journal
Volume	931
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ac6dde
State	Published - May 1 2022

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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Suess, K. A., Kriek, M., Bezanson, R., Greene, J. E., Setton, D., Spilker, J. S., Feldmann, R., Goulding, A. D., Johnson, B. D., Leja, J., Narayanan, D., Hall-Hooper, K., Hunt, Q., Lower, S., & Verrico, M. (2022). Erratum: SQuIGGLE: Studying Quenching in Intermediate-z Galaxies-Gas, → AnguLar Momentum, and Evolution (ApJ, (2022) 926 (89) DOI: 10.48550/arXiv.2111.14878. Astrophysical Journal, 931(1), Article 73. https://doi.org/10.3847/1538-4357/ac6dde

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title = "Erratum: SQuIGGLE: Studying Quenching in Intermediate-z Galaxies-Gas, → AnguLar Momentum, and Evolution (ApJ, (2022) 926 (89) DOI: 10.48550/arXiv.2111.14878",

abstract = "In the published article, we fit all 1300 galaxies in the SQuIGGLE survey using the Prospector stellar population fitting code (Johnson et al. 2021). We reported logM M in Figure 9 and Table 2 as the total mass formed, the default mass unit used in Prospector. However, logM M values in the literature are typically reported as stellar mass surviving. Surviving stellar mass is smaller than total mass formed by 0.1-0.3 dex due to stellar mass loss throughout a galaxy s lifetime (e.g., Conroy 2013). Figure 1 shows an updated version of the logM M distribution of SQuIGGLE galaxies. Table 1 includes the ID numbers and stellar masses of all galaxies in the SQuIGGLE sample. The median logM M value decreases by 0.2 dex with this unit change from 1011.39Me to 1011.20Me.",

author = "Suess, {Katherine A.} and Mariska Kriek and Rachel Bezanson and Greene, {Jenny E.} and David Setton and Spilker, {Justin S.} and Robert Feldmann and Goulding, {Andy D.} and Johnson, {Benjamin D.} and Joel Leja and Desika Narayanan and Khalil Hall-Hooper and Qiana Hunt and Sidney Lower and Margaret Verrico",

year = "2022",

month = may,

day = "1",

doi = "10.3847/1538-4357/ac6dde",

language = "English (US)",

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journal = "Astrophysical Journal",

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Suess, KA, Kriek, M, Bezanson, R, Greene, JE, Setton, D, Spilker, JS, Feldmann, R, Goulding, AD, Johnson, BD, Leja, J, Narayanan, D, Hall-Hooper, K, Hunt, Q, Lower, S & Verrico, M 2022, 'Erratum: SQuIGGLE: Studying Quenching in Intermediate-z Galaxies-Gas, → AnguLar Momentum, and Evolution (ApJ, (2022) 926 (89) DOI: 10.48550/arXiv.2111.14878', Astrophysical Journal, vol. 931, no. 1, 73. https://doi.org/10.3847/1538-4357/ac6dde

TY - JOUR

T1 - Erratum

T2 - SQuIGGLE: Studying Quenching in Intermediate-z Galaxies-Gas, → AnguLar Momentum, and Evolution (ApJ, (2022) 926 (89) DOI: 10.48550/arXiv.2111.14878

AU - Suess, Katherine A.

AU - Kriek, Mariska

AU - Bezanson, Rachel

AU - Greene, Jenny E.

AU - Setton, David

AU - Spilker, Justin S.

AU - Feldmann, Robert

AU - Goulding, Andy D.

AU - Johnson, Benjamin D.

AU - Leja, Joel

AU - Narayanan, Desika

AU - Hall-Hooper, Khalil

AU - Hunt, Qiana

AU - Lower, Sidney

AU - Verrico, Margaret

PY - 2022/5/1

Y1 - 2022/5/1

N2 - In the published article, we fit all 1300 galaxies in the SQuIGGLE survey using the Prospector stellar population fitting code (Johnson et al. 2021). We reported logM M in Figure 9 and Table 2 as the total mass formed, the default mass unit used in Prospector. However, logM M values in the literature are typically reported as stellar mass surviving. Surviving stellar mass is smaller than total mass formed by 0.1-0.3 dex due to stellar mass loss throughout a galaxy s lifetime (e.g., Conroy 2013). Figure 1 shows an updated version of the logM M distribution of SQuIGGLE galaxies. Table 1 includes the ID numbers and stellar masses of all galaxies in the SQuIGGLE sample. The median logM M value decreases by 0.2 dex with this unit change from 1011.39Me to 1011.20Me.

AB - In the published article, we fit all 1300 galaxies in the SQuIGGLE survey using the Prospector stellar population fitting code (Johnson et al. 2021). We reported logM M in Figure 9 and Table 2 as the total mass formed, the default mass unit used in Prospector. However, logM M values in the literature are typically reported as stellar mass surviving. Surviving stellar mass is smaller than total mass formed by 0.1-0.3 dex due to stellar mass loss throughout a galaxy s lifetime (e.g., Conroy 2013). Figure 1 shows an updated version of the logM M distribution of SQuIGGLE galaxies. Table 1 includes the ID numbers and stellar masses of all galaxies in the SQuIGGLE sample. The median logM M value decreases by 0.2 dex with this unit change from 1011.39Me to 1011.20Me.

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JF - Astrophysical Journal

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Erratum: SQuIGGLE: Studying Quenching in Intermediate-z Galaxies-Gas, → AnguLar Momentum, and Evolution (ApJ, (2022) 926 (89) DOI: 10.48550/arXiv.2111.14878

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