Discovery Date: 2026-02-24 02:37:28 UTC
Discovery MJD: 61095.11
Disc g-Flux: 4088.53±142.52
Latest Date: 2026-02-24 02:41:31 UTC
Latest MJD: 61095.11
Latest g-Flux: 4090.16±135.65
| Peak Flux | 4394.28±146.46 (g-band) |
| UTC at Peak | 2026-02-24 02:39:30 |
| MJD at Peak | 61095.11 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 10:00:46.207, 01:31:33.298 |
| Galactic Lon,Lat | 237.621863, 41.783952 |
| Ecliptic Lon,Lat | 151.727853, -9.975557 |
| E(B-V) Extinction | 0.019570 |
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 WISEAJ100046.09%2B013124.4; an r=19.33 mag galaxy found in the NED/PS1 catalogues. Its located 8.76" N, 2.44" E (37.6 Kpc) from the galaxy centre. A host z=0.270 implies a m - M = 40.69.
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 11:00:40 | 0.9711114360741089 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61095.112166 | 2026-02-24 02:41:31 | g | 4090 ± 136 | 0.99 | target ref diff | data |
| 61095.111697 | 2026-02-24 02:40:50 | g | 4093 ± 141 | 0.99 | target ref diff | data |
| 61095.111232 | 2026-02-24 02:40:10 | g | 4292 ± 138 | 0.99 | target ref diff | data |
| 61095.110767 | 2026-02-24 02:39:30 | g | 4394 ± 146 | 0.99 | target ref diff | data |
| 61095.110295 | 2026-02-24 02:38:49 | g | 4243 ± 141 | 0.99 | target ref diff | data |
| 61095.109828 | 2026-02-24 02:38:09 | g | 4066 ± 144 | 0.99 | target ref diff | data |
| 61095.109361 | 2026-02-24 02:37:28 | g | 4089 ± 143 | 0.99 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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