Discovery Date: 2026-02-25 04:51:27 UTC
Discovery MJD: 61096.20
Disc g-Flux: 1385.68±108.00
Latest Date: 2026-02-25 04:54:48 UTC
Latest MJD: 61096.20
Latest g-Flux: 1422.77±99.24
| Peak Flux | 1484.49±106.46 (g-band) |
| UTC at Peak | 2026-02-25 04:54:07 |
| MJD at Peak | 61096.20 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 10:01:18.330, 02:28:39.993 |
| Galactic Lon,Lat | 236.684930, 42.447970 |
| Ecliptic Lon,Lat | 151.516908, -9.037130 |
| E(B-V) Extinction | 0.020426 |
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 10000,345369,6050; an r=24.55 mag galaxy found in the DESI catalogue. Its located 0.02" S, 0.57" 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 05:10:26 | 0.8632317922943512 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.204726 | 2026-02-25 04:54:48 | g | 1423 ± 99 | 0.85 | target ref diff | data |
| 61096.204259 | 2026-02-25 04:54:07 | g | 1484 ± 106 | 0.85 | target ref diff | data |
| 61096.203791 | 2026-02-25 04:53:27 | g | 1306 ± 100 | 0.87 | target ref diff | data |
| 61096.203330 | 2026-02-25 04:52:47 | g | 1275 ± 101 | 0.79 | target ref diff | data |
| 61096.202400 | 2026-02-25 04:51:27 | g | 1386 ± 108 | 0.78 | 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.