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errata, addenda, techniques: spectroscopic, stars: atmospheres, stars: fundamental parameters, stars: late-type, supergiants, infrared: stars

This is an erratum to the paper by Taniguchi et al. (2021) entitled ‘Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, |$0.97-1.32\, \mu {\rm m}$|’ (2021, MNRAS, 502, 4210–4226). In table 9 of the original published version of this manuscript, the derived bolometric luminosities, log (L/L⊙), were old values before the revision taking into accounts the referee’s comment. Other columns were correct. Also, log (L/L⊙) plotted in fig. 9 of the original manuscript was correct, and the conclusion of the manuscript was not affected by this error.

Table 1 lists the corrected values of log (L/L⊙) together with the other columns.

Table 1.
Open in new tab

Final estimates of effective temperatures and luminosities of ten RSGs derived with 11 LDR–Teff relationships, except ID (2) (see section 4.1). The statistical error associated with TLDR is calculated with equation (8). The fourth and fifth columns show the parallax tabulated in the Gaia EDR3 catalogue (Gaia Collaboration et al. 2021) and the bias involved in it estimated following Lindegren et al. (2021), respectively, except for Betelgeuse. Its parallax, marked with an asterisk, is from the Hipparcos catalogue (van Leeuwen 2007).

ObjectHDTLDR[K]NpairParallax [mas]Bias [mas]log (L/L⊙)
ζ Cep2107454073 ± 31103.297 ± 0.146−0.022|$3.73^{+0.08}_{-0.08}$|
41 Gem520053940 ± 29110.721 ± 0.091−0.033|$4.28^{+0.17}_{-0.17}$|
ξ Cyg2009053891 ± 24112.836 ± 0.127−0.023|$3.96^{+0.09}_{-0.09}$|
V809 Cas2199783768 ± 35110.999 ± 0.039−0.032|$4.57^{+0.08}_{-0.08}$|
V424 Lac2169463749 ± 49111.402 ± 0.113−0.027|$4.22^{+0.10}_{-0.10}$|
|$\psi \, {}^{1}$| Aur445373740 ± 67110.443 ± 0.110−0.036|$5.25^{+0.24}_{-0.20}$|
TV Gem424753676 ± 11780.478 ± 0.135−0.029|$5.10^{+0.28}_{-0.22}$|
BU Gem425433883 ± 6790.564 ± 0.125−0.043|$5.05^{+0.22}_{-0.19}$|
Betelgeuse398013611 ± 3811 6.55 ± 0.83|$^{\ast }$||$4.91^{+0.14}_{-0.13}$|
NO Aur375363651 ± 31110.919 ± 0.093−0.042|$4.49^{+0.12}_{-0.11}$|
ObjectHDTLDR[K]NpairParallax [mas]Bias [mas]log (L/L⊙)
ζ Cep2107454073 ± 31103.297 ± 0.146−0.022|$3.73^{+0.08}_{-0.08}$|
41 Gem520053940 ± 29110.721 ± 0.091−0.033|$4.28^{+0.17}_{-0.17}$|
ξ Cyg2009053891 ± 24112.836 ± 0.127−0.023|$3.96^{+0.09}_{-0.09}$|
V809 Cas2199783768 ± 35110.999 ± 0.039−0.032|$4.57^{+0.08}_{-0.08}$|
V424 Lac2169463749 ± 49111.402 ± 0.113−0.027|$4.22^{+0.10}_{-0.10}$|
|$\psi \, {}^{1}$| Aur445373740 ± 67110.443 ± 0.110−0.036|$5.25^{+0.24}_{-0.20}$|
TV Gem424753676 ± 11780.478 ± 0.135−0.029|$5.10^{+0.28}_{-0.22}$|
BU Gem425433883 ± 6790.564 ± 0.125−0.043|$5.05^{+0.22}_{-0.19}$|
Betelgeuse398013611 ± 3811 6.55 ± 0.83|$^{\ast }$||$4.91^{+0.14}_{-0.13}$|
NO Aur375363651 ± 31110.919 ± 0.093−0.042|$4.49^{+0.12}_{-0.11}$|
Table 1.
Open in new tab

Final estimates of effective temperatures and luminosities of ten RSGs derived with 11 LDR–Teff relationships, except ID (2) (see section 4.1). The statistical error associated with TLDR is calculated with equation (8). The fourth and fifth columns show the parallax tabulated in the Gaia EDR3 catalogue (Gaia Collaboration et al. 2021) and the bias involved in it estimated following Lindegren et al. (2021), respectively, except for Betelgeuse. Its parallax, marked with an asterisk, is from the Hipparcos catalogue (van Leeuwen 2007).

ObjectHDTLDR[K]NpairParallax [mas]Bias [mas]log (L/L⊙)
ζ Cep2107454073 ± 31103.297 ± 0.146−0.022|$3.73^{+0.08}_{-0.08}$|
41 Gem520053940 ± 29110.721 ± 0.091−0.033|$4.28^{+0.17}_{-0.17}$|
ξ Cyg2009053891 ± 24112.836 ± 0.127−0.023|$3.96^{+0.09}_{-0.09}$|
V809 Cas2199783768 ± 35110.999 ± 0.039−0.032|$4.57^{+0.08}_{-0.08}$|
V424 Lac2169463749 ± 49111.402 ± 0.113−0.027|$4.22^{+0.10}_{-0.10}$|
|$\psi \, {}^{1}$| Aur445373740 ± 67110.443 ± 0.110−0.036|$5.25^{+0.24}_{-0.20}$|
TV Gem424753676 ± 11780.478 ± 0.135−0.029|$5.10^{+0.28}_{-0.22}$|
BU Gem425433883 ± 6790.564 ± 0.125−0.043|$5.05^{+0.22}_{-0.19}$|
Betelgeuse398013611 ± 3811 6.55 ± 0.83|$^{\ast }$||$4.91^{+0.14}_{-0.13}$|
NO Aur375363651 ± 31110.919 ± 0.093−0.042|$4.49^{+0.12}_{-0.11}$|
ObjectHDTLDR[K]NpairParallax [mas]Bias [mas]log (L/L⊙)
ζ Cep2107454073 ± 31103.297 ± 0.146−0.022|$3.73^{+0.08}_{-0.08}$|
41 Gem520053940 ± 29110.721 ± 0.091−0.033|$4.28^{+0.17}_{-0.17}$|
ξ Cyg2009053891 ± 24112.836 ± 0.127−0.023|$3.96^{+0.09}_{-0.09}$|
V809 Cas2199783768 ± 35110.999 ± 0.039−0.032|$4.57^{+0.08}_{-0.08}$|
V424 Lac2169463749 ± 49111.402 ± 0.113−0.027|$4.22^{+0.10}_{-0.10}$|
|$\psi \, {}^{1}$| Aur445373740 ± 67110.443 ± 0.110−0.036|$5.25^{+0.24}_{-0.20}$|
TV Gem424753676 ± 11780.478 ± 0.135−0.029|$5.10^{+0.28}_{-0.22}$|
BU Gem425433883 ± 6790.564 ± 0.125−0.043|$5.05^{+0.22}_{-0.19}$|
Betelgeuse398013611 ± 3811 6.55 ± 0.83|$^{\ast }$||$4.91^{+0.14}_{-0.13}$|
NO Aur375363651 ± 31110.919 ± 0.093−0.042|$4.49^{+0.12}_{-0.11}$|

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© 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://dbpia.nl.go.kr/journals/pages/open_access/funder_policies/chorus/standard_publication_model)
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