Discovery Date: 2026-02-26 05:49:23 UTC
Discovery MJD: 61097.24
Disc i-Flux: 5597.96±193.67
Latest Date: 2026-02-26 05:53:33 UTC
Latest MJD: 61097.25
Latest i-Flux: 5563.37±203.63
| Peak Flux | 5966.14±204.34 (i-band) |
| UTC at Peak | 2026-02-26 05:50:03 |
| MJD at Peak | 61097.24 |
| Detection Count | 3 |
| Equatorial Lon,Lat | 10:03:21.359, 02:30:8.407 |
| Galactic Lon,Lat | 237.062112, 42.879204 |
| Ecliptic Lon,Lat | 151.993684, -8.834500 |
| E(B-V) Extinction | 0.020921 |
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 SDSSJ100321.91%2B022948.6; an r=17.52 mag galaxy found in the NED/SDSS catalogues. Its located 19.81" N, 8.40" W (29.6 Kpc) from the galaxy centre. A host z=0.072 implies a m - M = 37.58.
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 | 2026-02-26 06:11:16 | 0.9694551368538161 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61097.245526 | 2026-02-26 05:53:33 | i | 5563 ± 204 | 1.00 | target ref diff | data |
| 61097.245062 | 2026-02-26 05:52:53 | i | 5626 ± 206 | 1.00 | target ref diff | data |
| 61097.244500 | 2026-02-26 05:52:04 | i | 5757 ± 202 | 1.00 | target ref diff | data |
| 61097.244031 | 2026-02-26 05:51:24 | i | 5817 ± 197 | 1.00 | target ref diff | data |
| 61097.243565 | 2026-02-26 05:50:44 | i | 5385 ± 195 | 1.00 | target ref diff | data |
| 61097.243096 | 2026-02-26 05:50:03 | i | 5966 ± 204 | 1.00 | target ref diff | data |
| 61097.242629 | 2026-02-26 05:49:23 | i | 5598 ± 194 | 1.00 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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