Discovery Date: 2026-02-25 08:52:02 UTC
Discovery MJD: 61096.37
Disc g-Flux: 2099.33±133.99
Latest Date: 2026-02-25 08:56:04 UTC
Latest MJD: 61096.37
Latest g-Flux: 1903.15±118.80
| Peak Flux | 2143.91±120.53 (g-band) |
| UTC at Peak | 2026-02-25 08:52:42 |
| MJD at Peak | 61096.37 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 12:29:26.618, 07:40:57.235 |
| Galactic Lon,Lat | 286.916594, 69.867484 |
| Ecliptic Lon,Lat | 183.685868, 9.971518 |
| E(B-V) Extinction | 0.024156 |
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 NGC4466; a W1=12.78 mag galaxy found in the NED/NED-D/LASR catalogues. Its located 50.12" S, 58.50" W (11.1 Kpc) from the galaxy centre. A host distance of 29.8 Mpc(z=0.002) implies a m - M = 32.37.
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 09:05:33 | 0.6235383316377 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.372277 | 2026-02-25 08:56:04 | g | 1903 ± 119 | 0.90 | target ref diff | data |
| 61096.371808 | 2026-02-25 08:55:24 | g | 2058 ± 135 | 0.87 | target ref diff | data |
| 61096.371341 | 2026-02-25 08:54:43 | g | 1966 ± 125 | 0.89 | target ref diff | data |
| 61096.370872 | 2026-02-25 08:54:03 | g | 2133 ± 131 | 0.90 | target ref diff | data |
| 61096.370407 | 2026-02-25 08:53:23 | g | 1858 ± 134 | 0.85 | target ref diff | data |
| 61096.369938 | 2026-02-25 08:52:42 | g | 2144 ± 121 | 0.93 | target ref diff | data |
| 61096.369468 | 2026-02-25 08:52:02 | g | 2099 ± 134 | 0.91 | 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.
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