JWST program 3215 (PI: Eisenstein) collected data with the NIRCam F182M, F210M, and F335M filters in October 2023. The Observing All Phases of StochastIc Star formation (OASIS) program (PI: Looser; PID: 5997) collected data from these same filters one year later, in October 2024. These surveys, both conducted in the GOODS-S field, have ~ 2 arcmin2 of overlapping area and thus allowed for an archival transient search.
We created difference images by subtracting the NIRCam images for each common filter collected by these programs and investigated the overlapping regions for transients via visual inspection and by running DAOStarFinder over the difference images and performing signal-to-noise cuts. We performed aperture photometry to measure the transients' apparent magnitudes.
We report one supernova candidate that first appeared in the program 3215 data (epoch1) and 3 supernova candidates that first appeared in the OASIS data (epoch2), with magnitudes down to ~30.2 AB mag. We associated 3 of these with nearby host galaxies with redshifts of z=0.342, z~2.55, and z~2.92. Notably, AT 2024aihp belongs to a faint host galaxy for which there is no redshift information available.
The attached images show the 2023 images (program 3215), 2024 images (OASIS; program 5997), difference images, and three-color images for each transient.
| 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 | 2024aihp | 03:32:16.024 | -27:51:42.91 | 03:32:16.024 | -27:51:42.91 | |||||||
| TNS | 2024aiho | 03:32:20.346 | -27:52:23.39 | OASIS+53.08446-27.87283 | 0.35 | 03:32:20.346 | -27:52:23.39 | |||||
| TNS | 2023aeex | 03:32:18.269 | -27:51:34.89 | OASIS+53.07606-27.85979 | 2.92 | 03:32:18.269 | -27:51:34.89 | |||||
| TNS | 2024aihn | 03:32:23.084 | -27:50:56.16 | OASIS+53.09631-27.84909 | 2.55 | 03:32:23.084 | -27:50:56.16 |


Comments