Discovery Date: 2026-02-25 08:41:00 UTC
Discovery MJD: 61096.36
Disc g-Flux: 1246.64±120.80
Latest Date: 2026-02-25 08:45:02 UTC
Latest MJD: 61096.36
Latest g-Flux: 1237.68±113.56
| Peak Flux | 1246.64±120.80 (g-band) |
| UTC at Peak | 2026-02-25 08:41:00 |
| MJD at Peak | 61096.36 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 12:24:55.998, 07:19:18.741 |
| Galactic Lon,Lat | 284.112550, 69.219517 |
| Ecliptic Lon,Lat | 182.793570, 9.193221 |
| E(B-V) Extinction | 0.024877 |
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 NGC4366; a W1=12.71 mag galaxy found in the LASR catalogue. Its located 112.72" S, 134.08" E (15.4 Kpc) from the galaxy centre. A host z=0.004 implies a m - M = 31.31.
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 08:54:10 | 0.36595494576989424 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.364617 | 2026-02-25 08:45:02 | g | 1238 ± 114 | 0.59 | target ref diff | data |
| 61096.363683 | 2026-02-25 08:43:42 | g | 1219 ± 118 | 0.57 | target ref diff | data |
| 61096.362751 | 2026-02-25 08:42:21 | g | 1057 ± 121 | 0.57 | target ref diff | data |
| 61096.361816 | 2026-02-25 08:41:00 | g | 1247 ± 121 | 0.67 | 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.