Discovery Date: 2026-02-24 04:05:08 UTC
Discovery MJD: 61095.17
Disc i-Flux: 6110.06±271.34
Latest Date: 2026-02-24 04:08:31 UTC
Latest MJD: 61095.17
Latest i-Flux: 5940.91±259.52
| Peak Flux | 6135.30±277.53 (i-band) |
| UTC at Peak | 2026-02-24 04:06:29 |
| MJD at Peak | 61095.17 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 12:27:8.646, 07:06:44.119 |
| Galactic Lon,Lat | 285.759423, 69.170079 |
| Ecliptic Lon,Lat | 183.387604, 9.220669 |
| E(B-V) Extinction | 0.023386 |
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 116531867870624279; an r=21.73 mag galaxy found in the PS1 catalogue. Its located 2.67" N, 3.82" 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 | 2026-02-24 17:01:30 | 0.905320156886024 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61095.172587 | 2026-02-24 04:08:31 | i | 5941 ± 260 | 1.00 | target ref diff | data |
| 61095.171640 | 2026-02-24 04:07:09 | i | 6065 ± 274 | 1.00 | target ref diff | data |
| 61095.171171 | 2026-02-24 04:06:29 | i | 6135 ± 278 | 1.00 | target ref diff | data |
| 61095.170699 | 2026-02-24 04:05:48 | i | 5871 ± 276 | 1.00 | target ref diff | data |
| 61095.170232 | 2026-02-24 04:05:08 | i | 6110 ± 271 | 1.00 | 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.