Discovery Date: 2026-02-26 07:26:14 UTC
Discovery MJD: 61097.31
Disc r-Flux: 5131.71±168.69
Latest Date: 2026-02-26 07:29:54 UTC
Latest MJD: 61097.31
Latest r-Flux: 5695.28±196.79
| Peak Flux | 5743.97±173.96 (r-band) |
| UTC at Peak | 2026-02-26 07:26:54 |
| MJD at Peak | 61097.31 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 09:54:54.958, 02:34:57.847 |
| Galactic Lon,Lat | 235.342301, 41.200255 |
| Ecliptic Lon,Lat | 149.963721, -9.493025 |
| E(B-V) Extinction | 0.046300 |
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 111091487297109747; an r=21.38 mag galaxy found in the PS1/DESI catalogues. Its located 0.53" S, 2.35" 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 | 2026-02-26 11:41:43 | 0.979473071822307 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61097.312435 | 2026-02-26 07:29:54 | r | 5695 ± 197 | 0.99 | target ref diff | data |
| 61097.311965 | 2026-02-26 07:29:13 | r | 5443 ± 203 | 0.99 | target ref diff | data |
| 61097.311497 | 2026-02-26 07:28:33 | r | 5151 ± 200 | 0.99 | target ref diff | data |
| 61097.310824 | 2026-02-26 07:27:35 | r | 5382 ± 167 | 0.99 | target ref diff | data |
| 61097.310356 | 2026-02-26 07:26:54 | r | 5744 ± 174 | 0.99 | target ref diff | data |
| 61097.309887 | 2026-02-26 07:26:14 | r | 5132 ± 169 | 0.99 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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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.