Discovery Date: 2026-02-25 02:59:26 UTC
Discovery MJD: 61096.12
Disc i-Flux: 5944.55±258.36
Latest Date: 2026-02-25 03:02:47 UTC
Latest MJD: 61096.13
Latest i-Flux: 6152.72±257.02
| Peak Flux | 6362.38±255.44 (i-band) |
| UTC at Peak | 2026-02-25 03:00:46 |
| MJD at Peak | 61096.13 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 10:05:15.873, 01:55:17.955 |
| Galactic Lon,Lat | 238.085962, 42.924280 |
| Ecliptic Lon,Lat | 152.652720, -9.209824 |
| E(B-V) Extinction | 0.038334 |
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 GALEXASCJ100514.99%2B015502.8; a 19.39 mag galaxy found in the NED catalogue. Its located 16.66" N, 11.00" E (37.3 Kpc) from the galaxy centre. A host z=0.102 implies a m - M = 38.35.
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 03:11:21 | 0.8511570157473658 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.126944 | 2026-02-25 03:02:47 | i | 6153 ± 257 | 1.00 | target ref diff | data |
| 61096.126475 | 2026-02-25 03:02:07 | i | 5914 ± 261 | 1.00 | target ref diff | data |
| 61096.126009 | 2026-02-25 03:01:27 | i | 5833 ± 264 | 1.00 | target ref diff | data |
| 61096.125542 | 2026-02-25 03:00:46 | i | 6362 ± 255 | 1.00 | target ref diff | data |
| 61096.125074 | 2026-02-25 03:00:06 | i | 6290 ± 258 | 1.00 | target ref diff | data |
| 61096.124611 | 2026-02-25 02:59:26 | i | 5945 ± 258 | 1.00 | 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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