Discovery Date: 2026-02-24 03:02:23 UTC
Discovery MJD: 61095.13
Disc r-Flux: 6249.24±142.50
Latest Date: 2026-02-24 03:06:40 UTC
Latest MJD: 61095.13
Latest r-Flux: 6452.30±150.61
| Peak Flux | 6452.30±150.61 (r-band) |
| UTC at Peak | 2026-02-24 03:06:40 |
| MJD at Peak | 61095.13 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 10:00:45.421, 01:31:36.899 |
| Galactic Lon,Lat | 237.618196, 41.781891 |
| Ecliptic Lon,Lat | 151.724383, -9.975769 |
| E(B-V) Extinction | 0.019513 |
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 WISEAJ100045.56%2B013131.8; an r=20.42 mag galaxy found in the NED/PS1 catalogues. Its located 5.15" N, 1.21" W (28.9 Kpc) from the galaxy centre. A host z=0.440 implies a m - M = 41.93.
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 12:31:10 | 0.9213760744858681 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61095.129634 | 2026-02-24 03:06:40 | r | 6452 ± 151 | 1.00 | target ref diff | data |
| 61095.128996 | 2026-02-24 03:05:45 | r | 5982 ± 155 | 1.00 | target ref diff | data |
| 61095.128531 | 2026-02-24 03:05:05 | r | 6292 ± 147 | 1.00 | target ref diff | data |
| 61095.128063 | 2026-02-24 03:04:24 | r | 6356 ± 144 | 1.00 | target ref diff | data |
| 61095.127596 | 2026-02-24 03:03:44 | r | 6404 ± 148 | 1.00 | target ref diff | data |
| 61095.127128 | 2026-02-24 03:03:03 | r | 6287 ± 148 | 1.00 | target ref diff | data |
| 61095.126660 | 2026-02-24 03:02:23 | r | 6249 ± 143 | 1.00 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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