Discovery Date: 2026-02-24 03:22:11 UTC
Discovery MJD: 61095.14
Disc g-Flux: 3864.37±99.82
Latest Date: 2026-02-24 03:26:12 UTC
Latest MJD: 61095.14
Latest g-Flux: 3725.06±96.00
| Peak Flux | 3961.10±102.30 (g-band) |
| UTC at Peak | 2026-02-24 03:24:11 |
| MJD at Peak | 61095.14 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 09:56:58.391, 02:16:30.381 |
| Galactic Lon,Lat | 236.069056, 41.446815 |
| Ecliptic Lon,Lat | 150.560501, -9.604051 |
| E(B-V) Extinction | 0.020228 |
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 10000,343924,19744; an r=24.70 mag galaxy found in the DESI catalogue. Its located 0.04" N, 0.15" E 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 | 2026-02-24 12:16:17 | 0.9695776723427909 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61095.143203 | 2026-02-24 03:26:12 | g | 3725 ± 96 | 0.98 | target ref diff | data |
| 61095.142270 | 2026-02-24 03:24:52 | g | 3949 ± 100 | 0.98 | target ref diff | data |
| 61095.141805 | 2026-02-24 03:24:11 | g | 3961 ± 102 | 0.98 | target ref diff | data |
| 61095.141340 | 2026-02-24 03:23:31 | g | 3832 ± 98 | 0.98 | target ref diff | data |
| 61095.140408 | 2026-02-24 03:22:11 | g | 3864 ± 100 | 0.98 | 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.