The BlackGEM consortium reports the detection of BGEM J184740.50-630939.4 /AT2025tpu at RA,DEC (ICRS) = 281.918767 -63.160972 =
=18:47:40.504 -63:09:39.50. The transient was first detected at 2025-08-12 00:34:44 UT at q=19.25 +/- 0.07, and subsequently brightened on a second visit at 2025-08-12 01:50:14 to q=19.00 +-/- 0.09. The last non-detection of the source was on 2025-08-11 03:21:54 UT at a 6-sigma limit for transients of q>19.68 as the last of four multi-band visits during that night, where the source was detected in none of the images.
AT2025tpu is located in the outskirts of the Seyfert 2 galaxy IC 4769 at a distance of 58 Mpc and at 28" from the center of IC4769 in an uncrowded region of the galaxy. Adopting the distance of IC4769 for the transient, it is currently at an absolute magnitude of -14.8. We note that IC4769 was also host to SN2004ac, a Type Ia supernova.
Spectroscopic identification of this young transient is requested.
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 | 2004ac | 18:47:43.670 | -63:08:54.60 | SN Ia | IC 4769 | 18:47:43.670 | -63:08:54.60 | SN Ia | ||||
| TNS | 2025tpu | 18:47:40.504 | -63:09:39.50 | 18:47:40.504 | -63:09:39.50 | SN IIn | 0.015 |


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