Discovery Date: 2026-02-25 04:14:52 UTC
Discovery MJD: 61096.18
Disc r-Flux: 5444.40±141.17
Latest Date: 2026-02-25 04:19:35 UTC
Latest MJD: 61096.18
Latest r-Flux: 5672.13±141.39
| Peak Flux | 5672.13±141.39 (r-band) |
| UTC at Peak | 2026-02-25 04:19:35 |
| MJD at Peak | 61096.18 |
| Detection Count | 4 |
| Equatorial Lon,Lat | 09:57:34.138, 02:40:7.049 |
| Galactic Lon,Lat | 235.751225, 41.794014 |
| Ecliptic Lon,Lat | 150.563665, -9.183350 |
| E(B-V) Extinction | 0.018682 |
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 SDSSJ095732.27%2B024002.0; an r=17.21 mag galaxy found in the NED/SDSS catalogues. Its located 5.00" N, 27.80" E (38.6 Kpc) from the galaxy centre. A host z=0.072 implies a m - M = 37.55.
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 04:35:33 | 0.9714056325200665 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.180275 | 2026-02-25 04:19:35 | r | 5672 ± 141 | 1.00 | target ref diff | data |
| 61096.179340 | 2026-02-25 04:18:14 | r | 5433 ± 136 | 1.00 | target ref diff | data |
| 61096.178873 | 2026-02-25 04:17:34 | r | 5561 ± 139 | 1.00 | target ref diff | data |
| 61096.178406 | 2026-02-25 04:16:54 | r | 5470 ± 142 | 1.00 | target ref diff | data |
| 61096.177934 | 2026-02-25 04:16:13 | r | 5616 ± 139 | 1.00 | target ref diff | data |
| 61096.177466 | 2026-02-25 04:15:33 | r | 5546 ± 145 | 1.00 | target ref diff | data |
| 61096.177002 | 2026-02-25 04:14:52 | r | 5444 ± 141 | 1.00 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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