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Table 1
Comparison of different sets of distance determinations with the TRGB set from EDD.
Sample | N | ⟨μ − μEDD⟩ | σ | Notes | ||
|
||||||
TRGB | ||||||
Rizzi et al. (2007) excluding EDD | 83 | −0.016 ± 0.008 | 0.060 | Rizzi et al. (2007) | ||
Makarov et al. (2013) | 26 | −0.022 ± 0.005 | 0.025 | Rizzi et al. (2007) | ||
Radburn-Smith et al. (2011) | 13 | −0.021 ± 0.024 | 0.086 | Rizzi et al. (2007) | ||
Dalcanton et al. (2009) | 87 | −0.064 ± 0.008 | 0.062 | Padova isochrones | ||
MI(TRGB) = −4.05 | 181 | −0.027 ± 0.006 | 0.062 | |||
Lee et al. (1993) | 30 | −0.073 ± 0.021 | 0.114 | |||
Cepheids | ||||||
Saha et al. (2006) | 15 | −0.013 ± 0.048 | 0.157 | |||
Fouqué et al. (2003) | 7 | +0.002 ± 0.041 | 0.103 | |||
Kanbur et al. (2003) | 8 | +0.003 ± 0.062 | 0.197 | |||
Tammann et al. (2003) | 7 | +0.063 ± 0.047 | 0.110 | |||
Freedman et al. (2001) | 13 | −0.065 ± 0.030 | 0.100 | |||
Freedman et al. (2001) | 14 | −0.016 ± 0.034 | 0.143 | metallicity corrected | ||
Lanoix et al. (1999) | 16 | −0.029 ± 0.044 | 0.147 | |||
Udalski et al. (1999) | 8 | +0.015 ± 0.061 | 0.196 | corrected to μLMC = 18.50 | ||
Gieren et al. (1998) | 7 | −0.005 ± 0.047 | 0.109 | |||
Madore & Freedman (1991) | 13 | +0.007 ± 0.035 | 0.117 | |||
SBF | ||||||
Jensen et al. (2003) | 8 | −0.223 ± 0.076 | 0.223 | |||
Tonry et al. (2000) | 16 | +0.092 ± 0.057 | 0.250 | |||
PNLF | ||||||
Ciardullo et al. (1989) | 10 | +0.043 ± 0.089 | 0.225 | |||
Brightest stars | ||||||
Brightest blue stars | 61 | −0.039 ± 0.076 | 0.586 | |||
Brightest red stars | 21 | −0.080 ± 0.140 | 0.632 |
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