Discovery Date: 2026-02-20 04:40:25 UTC
Discovery MJD: 61091.19
Disc r-Flux: 658.05±130.66
Latest Date: 2026-02-25 04:42:44 UTC
Latest MJD: 61096.20
Latest r-Flux: 5762.23±197.62
| Peak Flux | 5762.23±197.62 (i-band) |
| UTC at Peak | 2026-02-25 04:42:44 |
| MJD at Peak | 61096.20 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 09:57:25.559, 02:26:4.753 |
| Galactic Lon,Lat | 235.981028, 41.630952 |
| Ecliptic Lon,Lat | 150.611961, -9.415181 |
| E(B-V) Extinction | 0.021106 |
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 10000,345365,8476; an r=23.90 mag galaxy found in the DESI catalogue. Its located 4.77" N, 1.11" W from the galaxy centre.
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 04:56:33 | 0.9624387597190425 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.196346 | 2026-02-25 04:42:44 | i | 5762 ± 198 | 1.00 | target ref diff | data |
| 61096.195879 | 2026-02-25 04:42:03 | i | 5653 ± 194 | 1.00 | target ref diff | data |
| 61096.194952 | 2026-02-25 04:40:43 | i | 5509 ± 196 | 1.00 | target ref diff | data |
| 61096.194485 | 2026-02-25 04:40:03 | i | 5486 ± 193 | 1.00 | target ref diff | data |
| 61091.194735 | 2026-02-20 04:40:25 | r | 658 ± 131 | 0.12 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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Start with our documentation on readthedocs, you might find the FAQ section especially useful.
If you still have questions, want to report a bug, or make a feature request, please reach out to us on the Lasair topic on the Rubin Community pages.