Discovery Date: 2026-02-25 06:09:11 UTC
Discovery MJD: 61096.26
Disc i-Flux: 3424.21±204.34
Latest Date: 2026-02-25 06:13:14 UTC
Latest MJD: 61096.26
Latest i-Flux: 3789.67±197.05
| Peak Flux | 4000.24±211.59 (i-band) |
| UTC at Peak | 2026-02-25 06:11:12 |
| MJD at Peak | 61096.26 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 09:56:11.475, 02:50:51.458 |
| Galactic Lon,Lat | 235.292009, 41.612765 |
| Ecliptic Lon,Lat | 150.173975, -9.134502 |
| E(B-V) Extinction | 0.025595 |
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 2MASXJ09561133%2B0251167; an r=17.10 mag galaxy found in the NED/SDSS catalogues. Its located 24.73" S, 2.51" E (45.9 Kpc) from the galaxy centre. A host z=0.100 implies a m - M = 38.32.
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 06:26:58 | 0.8469397861602409 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.259196 | 2026-02-25 06:13:14 | i | 3790 ± 197 | 0.99 | target ref diff | data |
| 61096.258725 | 2026-02-25 06:12:33 | i | 3268 ± 200 | 0.97 | target ref diff | data |
| 61096.258258 | 2026-02-25 06:11:53 | i | 3163 ± 198 | 0.97 | target ref diff | data |
| 61096.257789 | 2026-02-25 06:11:12 | i | 4000 ± 212 | 0.99 | target ref diff | data |
| 61096.257320 | 2026-02-25 06:10:32 | i | 3737 ± 214 | 0.98 | target ref diff | data |
| 61096.256853 | 2026-02-25 06:09:52 | i | 3669 ± 210 | 0.99 | target ref diff | data |
| 61096.256384 | 2026-02-25 06:09:11 | i | 3424 ± 204 | 0.98 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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