Discovery Date: 2026-01-17 07:20:48 UTC
Discovery MJD: 61057.31
Disc g-Flux: 550.43±97.79
Latest Date: 2026-02-25 03:46:21 UTC
Latest MJD: 61096.16
Latest g-Flux: 6060.96±361.72
| Peak Flux | 6173.67±340.99 (z-band) |
| UTC at Peak | 2026-02-25 03:45:01 |
| MJD at Peak | 61096.16 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 09:55:49.513, 02:26:47.983 |
| Galactic Lon,Lat | 235.662955, 41.309694 |
| Ecliptic Lon,Lat | 150.227456, -9.542356 |
| E(B-V) Extinction | 0.032061 |
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 10000,345363,11897; an r=23.77 mag galaxy found in the DESI catalogue. Its located 2.43" N, 0.33" 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 03:57:37 | 0.8063963090777653 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.157197 | 2026-02-25 03:46:21 | z | 6061 ± 362 | 0.98 | target ref diff | data |
| 61096.156733 | 2026-02-25 03:45:41 | z | 5856 ± 333 | 1.00 | target ref diff | data |
| 61096.156266 | 2026-02-25 03:45:01 | z | 6174 ± 341 | 1.00 | target ref diff | data |
| 61096.155801 | 2026-02-25 03:44:21 | z | 5612 ± 349 | 1.00 | target ref diff | data |
| 61057.306119 | 2026-01-17 07:20:48 | g | 550 ± 98 | 0.19 | 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.