The BlackGEM consortium reports the detection of BGEM J132508.95-430244.3/AT2025rza at RA,DEC (ICRS) = 201.287308 -43.045653
= 13:25:08.954 -43:02:44.35. The transient was first detected at 2025-07-22 23:39:16 UT at q=19.42 +/- 0.10, with no detections in the BlackGEM u- and i-bands and brightened on the subsequent night to q=18.59 +-/- 0.06 and i = 18.55 +/- 0.1. The last non-detection of the source was on 2025-07-20 23:49:59 UT at 6-sigma limit for transients of q>20.1.
AT2025rza is located in the outskirts of the giant elliptical galaxy Centaurus A, at ~4 arcminutes from the center of Centaurus A. Adopting a distance to Centaurus A of 3.5 Mpc, the transient is currently at absolute magnitude of -9.1.
The relatively slow rise is more indicative of a nova than a supernova, but spectroscopic confirmation is needed.
BlackGEM is designed, built and operated at the ESO La Silla Observatory, Chile by a consortia of universities and institutes, including
Radboud, NOVA, KU Leuven, Armagh, Barcelona, Tel Aviv, Weizmann, HUJI, Potsdam, Hamburg, DTU Space, Manchester, Warwick, Durham, UC Davis, TexasTech, LCO, Valparaiso.
| 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 | 2025rza | 13:25:08.954 | -43:02:44.35 | 13:25:08.954 | -43:02:44.35 |


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