NIR Tully-Fisher relation.
|Authors||α ± σα||β ± σβ||Fitting method||Number of galaxies|
|This work||−9.23 ± 0.26||−20.19 ± 0.18||OSL bisector||123|
|Sorce et al. (2014)||−9.77 ± 0.19||−20.14 ± 0.09||Inverse fitting||319|
|Sorce et al. (2014)||−9.89 ± 0.21||−20.17 ± 0.11||OSL bisector||319|
|Sorce et al. (2014)/HRS subsample||−9.31 ± 0.30||−20.25 ± 0.10||OSL bisector||89|
Notes. Coefficients obtained for the NIR S4G-1 band TF relation M3.6 μm = (β ± σβ)+(α ± σα) (log2Vmax − 2.5) in the literature and this work.
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