TY - JOUR
T1 - Erratum
T2 - The completed SDSS-IV extended baryon oscillation spectroscopic survey: Geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/icesjms/staa3074)
AU - Nadathur, Seshadri
AU - Woodfinden, Alex
AU - Percival, Will J.
AU - Aubert, Marie
AU - Bautista, Julian
AU - Dawson, Kyle
AU - Escoffier, Stéphanie
AU - Fromenteau, Sebastien
AU - Gil-Marín, Héctor
AU - Rich, James
AU - Ross, Ashley J.
AU - Rossi, Graziano
AU - Vargas Magaña, Mariana
AU - Brownstein, Joel R.
AU - Schneider, Donald P.
N1 - Publisher Copyright:
© 2022 Oxford University Press. All rights reserved.
PY - 2022/10/1
Y1 - 2022/10/1
N2 - There was a numerical error in the code implementation of the Gaussian streaming model (GSM) for the redshift-space void galaxy cross-correlation function shown in equation (A1) of Nadathur et al. ( 2020 ). After correcting this error, e v aluation of equation (A1) with the current version of the VICTOR package leads to results that are identical to those obtained from the baseline model, equation (5), used in the main body of the paper (see Woodfinden et al. 2022, for a deri v ation of the equi v alence of the models). Various statements regarding the GSM and equation (A1) made in appendix A of the paper were incorrect due to this error. The GSM performs identically to the baseline model used for the main analysis. Evaluation of all other models is unaffected by this correction. As equation (A1) was not used for the main analysis presented in the paper, the results presented are all unchanged. Ho we ver, the model comparison in fig. A1 is incorrect. The updated figure is shown below. The systematic errors for the fits of equation (A1) to the data presented in the bottom two rows of table A1 are also incorrect. The corrected entries for these rows are now redundant, since they are identical to those shown in table 1. While the remaining rows of the table are unchanged, for completeness the updated version of Table A1 is shown below. (Figure Presented).
AB - There was a numerical error in the code implementation of the Gaussian streaming model (GSM) for the redshift-space void galaxy cross-correlation function shown in equation (A1) of Nadathur et al. ( 2020 ). After correcting this error, e v aluation of equation (A1) with the current version of the VICTOR package leads to results that are identical to those obtained from the baseline model, equation (5), used in the main body of the paper (see Woodfinden et al. 2022, for a deri v ation of the equi v alence of the models). Various statements regarding the GSM and equation (A1) made in appendix A of the paper were incorrect due to this error. The GSM performs identically to the baseline model used for the main analysis. Evaluation of all other models is unaffected by this correction. As equation (A1) was not used for the main analysis presented in the paper, the results presented are all unchanged. Ho we ver, the model comparison in fig. A1 is incorrect. The updated figure is shown below. The systematic errors for the fits of equation (A1) to the data presented in the bottom two rows of table A1 are also incorrect. The corrected entries for these rows are now redundant, since they are identical to those shown in table 1. While the remaining rows of the table are unchanged, for completeness the updated version of Table A1 is shown below. (Figure Presented).
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U2 - 10.1093/mnras/stac2156
DO - 10.1093/mnras/stac2156
M3 - Comment/debate
AN - SCOPUS:85160093075
SN - 0035-8711
VL - 516
SP - 2936
EP - 2937
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 2
ER -