Discovery Date: 2026-02-25 07:46:22 UTC
Discovery MJD: 61096.32
Disc r-Flux: 4755.93±209.80
Latest Date: 2026-02-25 07:50:24 UTC
Latest MJD: 61096.33
Latest r-Flux: 4706.67±201.15
| Peak Flux | 4849.93±202.54 (r-band) |
| UTC at Peak | 2026-02-25 07:49:04 |
| MJD at Peak | 61096.33 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 09:59:46.300, 01:41:29.619 |
| Galactic Lon,Lat | 237.246040, 41.678907 |
| Ecliptic Lon,Lat | 151.431699, -9.907713 |
| E(B-V) Extinction | 0.018259 |
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 WISEAJ095946.17%2B014133.9; an r=21.42 mag galaxy found in the NED/PS1 catalogues. Its located 4.50" S, 1.95" E (25.1 Kpc) from the galaxy centre. A host z=0.371 implies a m - M = 41.49.
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 08:03:23 | 0.9332808673081903 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.326677 | 2026-02-25 07:50:24 | r | 4707 ± 201 | 0.99 | target ref diff | data |
| 61096.326209 | 2026-02-25 07:49:44 | r | 4549 ± 203 | 0.99 | target ref diff | data |
| 61096.325741 | 2026-02-25 07:49:04 | r | 4850 ± 203 | 0.99 | target ref diff | data |
| 61096.325274 | 2026-02-25 07:48:23 | r | 4682 ± 204 | 0.99 | target ref diff | data |
| 61096.324807 | 2026-02-25 07:47:43 | r | 4712 ± 204 | 0.99 | target ref diff | data |
| 61096.324340 | 2026-02-25 07:47:02 | r | 4377 ± 200 | 0.99 | target ref diff | data |
| 61096.323869 | 2026-02-25 07:46:22 | r | 4756 ± 210 | 0.99 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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