Discovery Date: 2026-02-17 02:21:48 UTC
Discovery MJD: 61088.10
Disc r-Flux: -1096.04±214.99
Latest Date: 2026-02-24 01:03:11 UTC
Latest MJD: 61095.04
Latest r-Flux: 1312.77±232.65
| Peak Flux | 1312.77±232.65 (i-band) |
| UTC at Peak | 2026-02-24 01:03:11 |
| MJD at Peak | 61095.04 |
| Detection Count | 10 |
| Equatorial Lon,Lat | 04:20:20.038, -46:47:4.645 |
| Galactic Lon,Lat | 253.130105, -44.880114 |
| Ecliptic Lon,Lat | 44.132109, -66.301075 |
| E(B-V) Extinction | 0.014002 |
Transient Name Server
This transient has probably not been reported to the TNS as yet. Check the TNS directly at this location.
Sherlock Contextual Classification
Prediction: Supernova
The transient is possibly associated with APMUKS(BJ)B041850.79-465410.1; an r=18.66 mag galaxy found in the NED/DESI catalogues. Its located 0.05" N, 0.11" E from the galaxy centre.
Difference Image Lightcurve
Access the data from this plot in the LSST Alert Packet Data table below.
Context Map
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61095.043882 | 2026-02-24 01:03:11 | i | 1313 ± 233 | 0.13 | target ref diff | data |
| 61094.115994 | 2026-02-23 02:47:01 | r | -1211 ± 225 | 0.16 | target ref diff | data |
| 61094.114263 | 2026-02-23 02:44:32 | r | -1367 ± 223 | 0.15 | target ref diff | data |
| 61094.110723 | 2026-02-23 02:39:26 | r | -1575 ± 210 | 0.27 | target ref diff | data |
| 61094.108989 | 2026-02-23 02:36:56 | r | -1355 ± 240 | 0.12 | target ref diff | data |
| 61094.106389 | 2026-02-23 02:33:12 | r | -1627 ± 246 | 0.16 | target ref diff | data |
| 61091.158956 | 2026-02-20 03:48:53 | r | -1461 ± 239 | 0.11 | target ref diff | data |
| 61091.157217 | 2026-02-20 03:46:23 | r | -1336 ± 247 | 0.16 | target ref diff | data |
| 61091.150980 | 2026-02-20 03:37:24 | r | -1200 ± 236 | 0.12 | target ref diff | data |
| 61088.098476 | 2026-02-17 02:21:48 | r | -1096 ± 215 | 0.11 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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