The transient host galaxy light in our photometric measurement is minimized via one of two methods: Reference images are downloaded from the PanSTARRS image access (Flewelling, H. A., et al.) and are convolved, using the nightly PSF to match our images. The reference is then subtracted from our co-added images. A secondary photometric standard is defined and retained on the subtracted image using a pixel mask.
A second method involves creating a model galaxy, using the IRAF artdata packages, scaling it to the images and subtracting the host galaxy. The differential photometry was then performed using Image Reduction and Analysis Facility (IRAF) (Tody, D. 1986, "The IRAF Data Reduction and Analysis System").
| Name | Date | g | host_g | z |
| 2023vou | 2023-10-26.166 | non-detection | --------- | --------- |
| 2023voz | 2023-10-26.107 | 17.33 | --------- | --------- |
| 2023voz | 2023-10-27.138 | 17.30 | --------- | --------- |
| 2023vqn | 2023-10-26.132 | 17.86 | 16.17 | 0.050 |
| 2023vka | 2023-10-27.170 | 19.82 | 21.34 | --------- |
| 2023vod | 2023-10-27.260 | 19.79 | --------- | 0.032 |
| 2023vpd | 2023-10-27.214 | 18.42 | 18.46 | 0.063 |
| 2023vqv | 2023-10-27.108 | 19.44 | 21.73 | 0.357 |
| 2023vuh | 2023-10-27.485 | non-detection | ---------- | --------- |
Several different secondary standards were used from SDSS DR16 (Ahumada+, 2020) and PS1 Survey DR1 (Chambers+, 2016) to perform differential photometry using Image Reduction and Analysis Facility.
*All the z values are photoZ (KD-tree method) from Sloan Digtial Sky Survey (SDSS) Sky Server.
| Catalog | Name | Reported RA | Reported DEC | Reported Obj-Type | Reported Redshift | Host Name | Host Redshift | Remarks | TNS RA | TNS DEC | TNS Obj-Type | TNS Redshift |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| TNS | 2023vou | 22:46:41.785 | +50:10:37.32 | 22:46:41.785 | +50:10:37.32 | |||||||
| TNS | 2023voz | 18:46:55.196 | +32:58:01.79 | WISEA J184654.84+325758.3 | 18:46:55.196 | +32:58:01.79 | ||||||
| TNS | 2023vqn | 22:52:31.722 | +18:14:06.48 | SN Ia | 0.07 | 22:52:31.726 | +18:14:06.46 | SN Ia | 0.07 | |||
| TNS | 2023vka | 22:22:18.043 | +30:48:29.02 | 22:22:18.043 | +30:48:29.02 | |||||||
| TNS | 2023vod | 22:55:52.398 | +56:22:44.62 | ZOAG G107.39-02.97 | 0.02228 | 22:55:52.398 | +56:22:44.62 | |||||
| TNS | 2023vpd | 22:40:12.907 | +19:30:24.54 | SN Ia | 0.034 | SDSS J224012.90+193024.7 | 22:40:12.907 | +19:30:24.54 | SN Ia | 0.034 | ||
| TNS | 2023vqv | 17:49:17.626 | +58:46:16.39 | SDSS J174917.52+584616.5 | 17:49:17.626 | +58:46:16.39 | ||||||
| TNS | 2023vuh | 07:12:33.443 | +46:13:20.97 | 07:12:33.443 | +46:13:20.97 |