Table 3.
Final sample of supernovae and their host galaxies.
| ZTFID | IAUID | Type | RA (SN) | Dec (SN) | z | AV, MW | RA (host) | Dec (host) | Mg,host | |
|---|---|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss) | (dd:mm:ss) | (mag) | (hh:mm:ss) | (dd:mm:ss) | (mag) | |||||
| ZTF19abauylg | SN 2019ieh | SN Ic | 16:42:10.83 | +06:59:02.4 | 0.032 | 0.28 | 16:42:10.80 | +06:59:02.1 |
 |
|
| ZTF19abfiqjg | SN 2019lfj | SN Ic | 01:57:48.75 | +13:10:34.2 | 0.089 | 0.15 | 01:57:48.76 | +13:10:34.4 |
 |
|
| ZTF19abztknu | SN 2019qvt | SN Ib | 03:09:01.53 | +24:02:38.1 | 0.053 | 0.48 | 03:09:01.52 | +24:02:39.2 |
 |
|
| ZTF20acvebcu | SN 2020abqx | SN Ib | 11:52:24.66 | +67:32:51.7 | 0.063 | 0.03 | 11:52:24.94 | +67:32:51.8 |
 |
|
| ZTF18abecbks | SN 2018ddu | SN Ic | 16:35:46.53 | +71:41:15.1 | 0.030 | 0.12 | 16:35:45.74 | +71:41:12.5 |
 |
|
| ZTF20aaiftgi | SN 2020aut | SN Ic | 14:10:13.35 | −06:49:20.7 | 0.034 | 0.10 | 14:10:14.29 | −06:49:20.6 |
 |
|
| ZTF21aannoix | SN 2021dwg | SN Ic | 14:18:15.96 | +00:53:18.4 | 0.026 | 0.11 | 14:18:14.91 | +00:53:27.9 |
 |
|
| ZTF21aaufwyh | SN 2021jao | SN Ib | 10:20:52.91 | +06:09:24.1 | 0.028 | 0.06 | 10:20:53.36 | +06:09:22.3 |
 |
|
| ZTF19aakpcuw | SN 2019bgl | SN Ic | 17:22:03.03 | +59:06:53.3 | 0.031 | 0.08 | 17:22:04.76 | +59:06:47.5 |
 |
|
| ZTF20aajcdad | SN 2020bcq | SN Ib | 13:26:29.65 | +36:00:31.1 | 0.019 | 0.04 | 13:26:28.54 | +36:00:37.0 |
 |
|
| ZTF19acmelor | SN 2019uff | SN Ib | 00:19:13.27 | −14:23:52.1 | 0.027 | 0.09 | 00:19:13.77 | −14:23:48.2 |
 |
|
| ZTF19abqmsbk | SN 2019orb | SN Ic | 17:40:34.75 | +14:52:47.9 | 0.027 | 0.24 | 17:40:34.76 | +14:52:47.9 |
 |
|
| ZTF20aalcyih | SN 2020bpf | SN Ib | 06:55:23.49 | +27:43:19.0 | 0.018 | 0.20 | 06:55:23.52 | +27:43:18.0 |
 |
|
| ZTF20abaszgh | SN 2020ksa | SN Ib | 10:59:27.94 | +46:07:28.4 | 0.022 | 0.05 | 10:59:27.35 | +46:07:20.5 |
 |
Notes. The host galaxy photometry was measured from SDSS and PanSTARRS images using LAMBDAR (Wright et al. 2016) and translated to absolute magnitudes by modeling the host-galaxy spectral energy distributions with Prospector (Johnson et al. 2021) following Schulze et al. (2021). The absolute magnitudes are corrected for MW extinction but not for host attenuation. The coordinates of the SNe and their host galaxies are measured in the J2000 reference system. About 2″ from the center of the host galaxy of SN 2019ieh is another object. It is uncertain whether this is a star-forming region or a separate galaxy.
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