Discovery Date: 2026-02-26 05:22:16 UTC
Discovery MJD: 61097.22
Disc i-Flux: 6892.64±213.01
Latest Date: 2026-02-26 05:26:18 UTC
Latest MJD: 61097.23
Latest i-Flux: 6238.98±205.90
| Peak Flux | 6892.64±213.01 (i-band) |
| UTC at Peak | 2026-02-26 05:22:16 |
| MJD at Peak | 61097.22 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 10:03:22.357, 02:30:3.169 |
| Galactic Lon,Lat | 237.067026, 42.881732 |
| Ecliptic Lon,Lat | 151.998135, -8.834403 |
| E(B-V) Extinction | 0.020951 |
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 14.34" N, 6.95" E (22.0 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 06:08:43 | 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 |
|---|---|---|---|---|---|---|
| 61097.226604 | 2026-02-26 05:26:18 | i | 6239 ± 206 | 1.00 | target ref diff | data |
| 61097.226132 | 2026-02-26 05:25:37 | i | 6637 ± 203 | 1.00 | target ref diff | data |
| 61097.225667 | 2026-02-26 05:24:57 | i | 6827 ± 205 | 1.00 | target ref diff | data |
| 61097.225203 | 2026-02-26 05:24:17 | i | 6481 ± 211 | 1.00 | target ref diff | data |
| 61097.224737 | 2026-02-26 05:23:37 | i | 6887 ± 217 | 1.00 | target ref diff | data |
| 61097.224271 | 2026-02-26 05:22:57 | i | 6853 ± 211 | 1.00 | target ref diff | data |
| 61097.223807 | 2026-02-26 05:22:16 | i | 6893 ± 213 | 1.00 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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