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Table 4.

Main variants for H0 calculation.

# H0 1-σ Nd.o.f. Reduced PTE a Δσb Description
km s−1 Mpc−1 χ2
V00 73.499 0.809 119 0.9879 0.494 Baseline
V01 73.493 0.807 131 0.9566 0.600 −0.11 Baseline + JAGB
V02 73.508 0.809 121 0.9732 0.541 0.46 Baseline + Miras
V03 73.604 0.798 133 0.9736 0.546 0.80 Baseline + DESI FP calibrated to Coma
V04 73.515 0.805 129 0.9842 0.509 0.20 Baseline + empirically calibrated SNe II
V05 73.720 0.740 133 0.9250 0.700 0.68 Baseline + SNe II w. EPM
V06 73.957 0.787 194 1.4712 2.1e−5 2.46 Baseline + TF
V07 73.314 0.789 120 0.9907 0.511 −1.04 Baseline + SMC
V08 72.509 1.296 69 0.9544 0.551 −0.38 Baseline w/o Cepheids
V08B 72.873 0.874 98 0.9760 0.548 Custom baseline for V08
V09 73.526 0.878 56 0.9864 0.504 −0.72 Baseline w/o TRGB, SBF
V09B 73.738 0.827 106 0.8893 0.786 Custom baseline for V09
V10 73.609 0.929 118 0.9939 0.501 0.24 Baseline w/o Gaia parallaxes, MW
V11 73.337 0.853 118 0.9908 0.511 −0.60 Baseline w/o DEB, LMC
V12 73.084 0.920 47 0.8876 0.652 −1.70 Baseline w/o NGC 4258
V12B 73.632 0.861 87 0.9758 0.513 Custom baseline for V12
V13 73.434 1.795 23 0.4851 0.972 −0.04 Baseline w/o SNe Ia
V14 73.325 0.830 100 1.0694 0.299 −0.94 Baseline w/o SBF
V15 73.633 0.841 114 1.0149 0.438 0.58 Baseline w/o masers in the Hubble flow
V16 73.754 1.325 55 1.0295 0.377 −0.28 Exclude HST data, LMC, MW
V16B 74.024 0.924 85 0.9812 0.498 Custom baseline for V16
V17 73.002 0.856 85 0.9598 0.554 −1.77 Exclude JWST data
V18 73.690 0.822 108 0.9790 0.544 1.28 Exclude SN 1994D and earlier
V19 73.062 0.804 119 0.9853 0.502 Baseline w. SNe Ia, SBF, Masers in CMB frame
V20 73.190 0.862 100 1.0689 0.300 Hubble flow SNe Ia w. z < 0.06
V21 72.667 0.862 100 1.0674 0.304 SNe Ia in redshift range 0.03–0.10
V22 73.350 0.963 119 0.7933 0.946 SNe Ia from CSP, all 55 calibrators
V23 73.821 1.072 114 0.8671 0.843 SNe Ia from BayesSN
V24 73.445 0.810 119 0.9167 0.710 SNe Ia from PP processed w. SALT3 fitter
V25 72.459 1.099 64 0.8267 0.837 SNe Ia in H-band
V26 72.712 1.164 67 0.7035 0.962 SNe Ia in J-band
V27 73.411 0.800 119 0.9887 0.492 No off-diagonal covariance for SNe Ia in Hubble flow
V28 73.080 0.801 119 1.1347 0.135 No metallicity correction for Cepheid PL
V99 73.994 0.697 246 1.3078 8.3e−4 1.21 Everything available
V99A 73.656 0.713 172 0.8943 0.837 0.41 Everything available except TF

O1 73.110 0.920 57 0.9360 Orth. path 1 MW+LMC/SMC+Ceph+SNIa+FP
O2 73.434 1.795 23 0.4851 Orth. path 2 N4258+TRGB+SBF+MM (V00 equivalent)
O2_V99a 74.081 1.257 56 0.6016 Orth. path 2 O2+SNII+EPM (V99a equivalent)
O2_V99 74.759 1.148 151 1.4612 Orth. path 2 O2+SNII+EPM+TF(V99 equivalent)

Notes.

a)

PTE, or Probability to Exceed, is the probability of obtaining a value of χ2 larger than measured for that variant.

b)

Δσ is the significance of the change in H0 for the current variant in units of the relative uncertainty, determined as the quadrature difference of the total uncertainties. (See text for details.)

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