Discovery Date: 2026-02-24 04:15:11 UTC
Discovery MJD: 61095.18
Disc g-Flux: 2938.28±154.02
Latest Date: 2026-02-24 04:19:14 UTC
Latest MJD: 61095.18
Latest g-Flux: 2764.41±150.53
| Peak Flux | 3460.62±152.24 (g-band) |
| UTC at Peak | 2026-02-24 04:15:52 |
| MJD at Peak | 61095.18 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 12:25:58.051, 08:36:13.910 |
| Galactic Lon,Lat | 283.733583, 70.520314 |
| Ecliptic Lon,Lat | 182.509561, 10.470233 |
| E(B-V) Extinction | 0.020343 |
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 SDSSJ122557.46%2B083607.5; an r=17.87 mag galaxy found in the NED/SDSS catalogues. Its located 6.40" N, 9.55" E (35.2 Kpc) from the galaxy centre. A host z=0.183 implies a m - M = 39.74.
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 17:01:09 | 0.8300998031674793 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61095.180030 | 2026-02-24 04:19:14 | g | 2764 ± 151 | 0.91 | target ref diff | data |
| 61095.179563 | 2026-02-24 04:18:34 | g | 3016 ± 149 | 0.93 | target ref diff | data |
| 61095.179095 | 2026-02-24 04:17:53 | g | 3294 ± 160 | 0.94 | target ref diff | data |
| 61095.178627 | 2026-02-24 04:17:13 | g | 3300 ± 149 | 0.95 | target ref diff | data |
| 61095.178157 | 2026-02-24 04:16:32 | g | 3176 ± 152 | 0.94 | target ref diff | data |
| 61095.177689 | 2026-02-24 04:15:52 | g | 3461 ± 152 | 0.95 | target ref diff | data |
| 61095.177221 | 2026-02-24 04:15:11 | g | 2938 ± 154 | 0.94 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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