Discovery Date: 2026-02-25 08:44:22 UTC
Discovery MJD: 61096.36
Disc g-Flux: 1308.15±113.76
Latest Date: 2026-02-25 08:48:24 UTC
Latest MJD: 61096.37
Latest g-Flux: 1320.95±117.93
| Peak Flux | 1498.28±115.18 (g-band) |
| UTC at Peak | 2026-02-25 08:47:44 |
| MJD at Peak | 61096.37 |
| Detection Count | 3 |
| Equatorial Lon,Lat | 12:23:30.538, 07:27:56.565 |
| Galactic Lon,Lat | 283.040895, 69.251818 |
| Ecliptic Lon,Lat | 182.407445, 9.183513 |
| E(B-V) Extinction | 0.023499 |
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 NGC4334; a W1=10.04 mag galaxy found in the NED-D/LASR catalogues. Its located 26.95" S, 98.95" E (18.2 Kpc) from the galaxy centre. A host distance of 36.7 Mpc(z=0.014) implies a m - M = 32.82.
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 09:02:09 | 0.14359868090846428 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.366953 | 2026-02-25 08:48:24 | g | 1321 ± 118 | 0.66 | target ref diff | data |
| 61096.366485 | 2026-02-25 08:47:44 | g | 1498 ± 115 | 0.78 | target ref diff | data |
| 61096.366016 | 2026-02-25 08:47:03 | g | 1417 ± 117 | 0.72 | target ref diff | data |
| 61096.365551 | 2026-02-25 08:46:23 | g | 1377 ± 116 | 0.68 | target ref diff | data |
| 61096.365085 | 2026-02-25 08:45:43 | g | 1196 ± 111 | 0.62 | target ref diff | data |
| 61096.364617 | 2026-02-25 08:45:02 | g | 1250 ± 115 | 0.75 | target ref diff | data |
| 61096.364151 | 2026-02-25 08:44:22 | g | 1308 ± 114 | 0.63 | 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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