Discovery Date: 2026-02-25 03:03:28 UTC
Discovery MJD: 61096.13
Disc i-Flux: 1747.38±232.41
Latest Date: 2026-02-25 03:14:52 UTC
Latest MJD: 61096.14
Latest i-Flux: 1781.38±205.29
| Peak Flux | 1871.84±224.25 (i-band) |
| UTC at Peak | 2026-02-25 03:08:49 |
| MJD at Peak | 61096.13 |
| Detection Count | 3 |
| Equatorial Lon,Lat | 10:00:42.683, 03:11:16.966 |
| Galactic Lon,Lat | 235.779552, 42.734717 |
| Ecliptic Lon,Lat | 151.125198, -8.423461 |
| E(B-V) Extinction | 0.025433 |
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 UGC05377; a W1=14.16 mag galaxy found in the LASR catalogue. Its located 62.12" S, 166.63" E (26.2 Kpc) from the galaxy centre. A host z=0.007 implies a m - M = 32.45.
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 03:35:11 | 0.08837150404640129 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.135324 | 2026-02-25 03:14:52 | i | 1781 ± 205 | 0.78 | target ref diff | data |
| 61096.134392 | 2026-02-25 03:13:31 | i | 1756 ± 202 | 0.56 | target ref diff | data |
| 61096.131131 | 2026-02-25 03:08:49 | i | 1872 ± 224 | 0.65 | target ref diff | data |
| 61096.127412 | 2026-02-25 03:03:28 | i | 1747 ± 232 | 0.52 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
Need Help?
readthedocs
Lasair Community
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.