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Table F.1.

Peculiar velocities and Tully (2015) group redshifts used in Sect. 7.1.5.

Name Host galaxy zCMB zCMB, group vpec [km/s]

T15 baseline baseline + T15 2M++ C15 2MRS Cf3 Cf4
Literature

SN 2003bn 2MASX J10023529-2110531 0.01393 −90 −209 −83 −133 +158
SN 2006it NGC 6956 0.01449 0.01430 −127 −127 −146 −204 −473 −226
SN 2010id NGC 7483 0.01523 0.01501 −180 −180 −213 −180 −243 −106
SN 2013fs NGC 7610 0.01061 −68 −40 −122 −242 +39

ePESSTO+

SN 2019luo MCG -01-01-040 0.03908 −144 −172 −88 +353 −84
SN 2020bad WISEA J092426.48+203802.9 0.02711 +62 +88 −171 +23 +183
SN 2020cvy IC 2217 0.01801 0.01808 −202 −189 −255 −142 −374 −100
SN 2021gvv WISEA J170435.95+140450.4 0.03789 −134 −185 −221 +517 +272
SN 2021hkf CGCG 040-036 0.02077 +256 +351 +141 −352 −250
SN 2021acvc WISEA J053038.62-225410.2 0.03157 +178 +230 +276 −157 −276

Notes. In the baseline + T15 correction scheme, group redshifts (zCMB, group) and group-based peculiar velocities (vpec, baseline + T15) are used for SNe whose host galaxies are members of groups identified in the Tully (2015) catalogue; for all other SNe, individual galaxy redshifts (zCMB) and baseline peculiar velocities (vpec, baseline) are used.

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