Discovery Date: 2026-02-27 05:26:52 UTC
Discovery MJD: 61098.23
Disc g-Flux: 3543.76±190.62
Latest Date: 2026-02-27 05:30:16 UTC
Latest MJD: 61098.23
Latest g-Flux: 3061.36±202.12
| Peak Flux | 3543.76±190.62 (g-band) |
| UTC at Peak | 2026-02-27 05:26:52 |
| MJD at Peak | 61098.23 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 12:23:22.208, 06:43:8.918 |
| Galactic Lon,Lat | 283.574107, 68.529541 |
| Ecliptic Lon,Lat | 182.678061, 8.485626 |
| E(B-V) Extinction | 0.024511 |
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 116061858434293419; an r=21.14 mag galaxy found in the PS1 catalogue. Its located 0.60" S, 2.37" 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 | 2026-02-27 05:37:37 | 0.9102559173970928 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61098.229360 | 2026-02-27 05:30:16 | g | 3061 ± 202 | 0.95 | target ref diff | data |
| 61098.228892 | 2026-02-27 05:29:36 | g | 3300 ± 194 | 0.96 | target ref diff | data |
| 61098.227941 | 2026-02-27 05:28:14 | g | 3346 ± 193 | 0.96 | target ref diff | data |
| 61098.227468 | 2026-02-27 05:27:33 | g | 3207 ± 191 | 0.97 | target ref diff | data |
| 61098.227000 | 2026-02-27 05:26:52 | g | 3544 ± 191 | 0.97 | 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.