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Table 1

Summary of the galaxy/supernova sample investigated in this work.

Galaxy Type Assoc. SN RA (J2000)a Dec (J2000)a Galaxy V-mag SN magb D25c Distanced Linear scale
h:m:s d:m:s AB-mag mag arcsec Mpc kpc/′′

NGC 1058 SA SN 1969L 02:43:30 +37:20:29 11.20 12.8 90.6  ×  84.6 7.3 0.035
NGC 2968 I0 SN 1970L 09:43:12 +31:55:43 11.73 13.0 60.4  ×  46.8 22.0 0.110
NGC 3160 S SN 1997C 10:13:55 +38:50:34 14.17 17.5 63.9  ×  12.9 97.0 0.460
??? ??? SN 2005nc 18:32:32 +26:20:23  >27.4 ??? ??? 2233.3 6.725
UGC 5434 SAB SN 2006bx 10:05:13 +21:27:21 14.21 18.1 38.5  ×  24.0 78.3 0.373

Notes. All quantities given below were taken from the NASA Extragalactic Database (NED).

(a)

For all galaxies, the center coordinates are given, except for SN 2005nc where there is no host galaxy, hence the SN coordinates are provided.

(b)

Magnitude of the supernova as given in the initial CBAT discovery notice (therefore not necessarily AB system, mostly clear filter). Note that all magnitudes are consistent with the supernova being in their respective host galaxy using the standard candle relationships from Drout et al. (2011) and Kasen & Woosley (2009) for type I resp. type II supernovae.

(c)

The isophotes were taken from the SDSS database and are measured in the r-band (except for NGC 1058 which is not within the SDSS coverage, hence an RC3 B-band value is used).

(d)

For NGC 1058, and NGC 2968, the distances were estimated using the Tully-Fisher relation. All other distances were calculated using the redshift of the corresponding galaxy and a flat ΛCDM cosmology as described in Sect. 1.

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