ZTF SN Ia DR2
Open Access

Table 2.

Properties of the hostless SNe Ia from the volume-limited ZTF DR2 SN Ia sample.

SN name Redshift ( * ) Sub-type SALT2 x1 SALT2 c Mg, SN(a) Mi, host upper log(M/M) AV Galactic latitude (b)
(mag) limit (mag) upper limit (mag) (deg)
SN 2019eks 0.047 ± 0.003 99aa-like 0.66 ± 0.16 −0.12 ± 0.04 −19.00 ± 0.04 −14.0 < 6.6 0.67 10.1
SN 2020bdq 0.043 ± 0.004 Normal 0.07 ± 0.40 −0.15 ± 0.04 −18.90 ± 0.06 −13.6 < 6.6 0.37 7.6
SN 2020isd 0.030 ± 0.003 Ia-unclear 1.07 ± 0.35 0.13 ± 0.04 −18.98 ± 0.06 −14.2 < 6.0 2.18 12.2
SN 2020lmd 0.011 Normal 2.12 ± 0.29 0.01 ± 0.04 −18.31 ± 0.05 −11.2 < 5.3 1.11 −8.0
SN 2020lmd ( † ) 0.018 Normal 2.12 ± 0.29 0.01 ± 0.04 −18.31 ± 0.05 −12.1 < 6.0 1.11 −8.0
SN 2020lyt 0.037 ± 0.003 Ia-unclear −0.42 ± 1.08 0.13 ± 0.15 −19.04 ± 0.29 −13.2 < 6.5 0.15 −29.8
SN 2020rzx 0.041 ± 0.003 Normal 1.29 ± 0.09 −0.07 ± 0.03 −19.18 ± 0.04 −13.7 < 6.5 0.64 −18.8

Notes. ( * )The upper bounds of the redshifts are used to place the most conservative limits on the host parameters.

(a)

Absolute magnitude of the SN in ZTF g-band.

( † )Due to the HV feature observed in the Si IIλ6355 line, the SN matches better with observations at higher redshifts. In this study, we identified the upper range of redshifts where the SN showed the best match for the HV feature. In the subsequent analysis, we use the values calculated from this optimal redshift value.

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