Discovery Date: 2026-02-25 07:43:40 UTC
Discovery MJD: 61096.32
Disc r-Flux: 2649.46±198.96
Latest Date: 2026-02-25 07:47:43 UTC
Latest MJD: 61096.32
Latest r-Flux: 2950.47±196.65
| Peak Flux | 3230.13±192.39 (r-band) |
| UTC at Peak | 2026-02-25 07:47:02 |
| MJD at Peak | 61096.32 |
| Detection Count | 3 |
| Equatorial Lon,Lat | 09:59:29.394, 02:13:46.839 |
| Galactic Lon,Lat | 236.603791, 41.934534 |
| Ecliptic Lon,Lat | 151.174201, -9.428034 |
| E(B-V) Extinction | 0.020254 |
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 SDSS J095929.92+021352.1; an r=18.94 mag galaxy found in the SDSS/PS1 catalogues. Its located 5.29" S, 7.91" W (46.5 Kpc) from the galaxy centre. A host z=0.345 implies a m - M = 41.31.
Difference Image Lightcurve
Access the data from this plot in the LSST Alert Packet Data table below.
Context Map
Annotations
| Annotator | Timestamp | Annotation | Explanation | JSON Data | Link |
|---|---|---|---|---|---|
| r0b_lvra a1 | 2026-02-25 07:58:39 | 0.44214406276854895 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.324807 | 2026-02-25 07:47:43 | r | 2950 ± 197 | 0.96 | target ref diff | data |
| 61096.324340 | 2026-02-25 07:47:02 | r | 3230 ± 192 | 0.96 | target ref diff | data |
| 61096.323869 | 2026-02-25 07:46:22 | r | 2683 ± 205 | 0.92 | target ref diff | data |
| 61096.323400 | 2026-02-25 07:45:41 | r | 3183 ± 204 | 0.93 | target ref diff | data |
| 61096.322932 | 2026-02-25 07:45:01 | r | 3147 ± 200 | 0.97 | target ref diff | data |
| 61096.322463 | 2026-02-25 07:44:20 | r | 3097 ± 210 | 0.95 | target ref diff | data |
| 61096.321994 | 2026-02-25 07:43:40 | r | 2649 ± 199 | 0.95 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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