Discovery Date: 2026-02-26 05:39:58 UTC
Discovery MJD: 61097.24
Disc i-Flux: 2205.98±213.07
Latest Date: 2026-02-26 05:44:00 UTC
Latest MJD: 61097.24
Latest i-Flux: 2118.93±197.39
| Peak Flux | 2711.85±205.14 (i-band) |
| UTC at Peak | 2026-02-26 05:43:19 |
| MJD at Peak | 61097.24 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 10:02:5.994, 01:47:40.522 |
| Galactic Lon,Lat | 237.592164, 42.210713 |
| Ecliptic Lon,Lat | 151.947983, -9.607378 |
| E(B-V) Extinction | 0.019682 |
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 SDSSJ100207.15%2B014722.0; an r=20.83 mag galaxy found in the NED/SDSS catalogues. Its located 18.82" N, 18.04" W (39.9 Kpc) from the galaxy centre. A host z=0.081 implies a m - M = 37.84.
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 05:59:10 | 0.712734315734864 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61097.238893 | 2026-02-26 05:44:00 | i | 2119 ± 197 | 0.86 | target ref diff | data |
| 61097.238423 | 2026-02-26 05:43:19 | i | 2712 ± 205 | 0.85 | target ref diff | data |
| 61097.237959 | 2026-02-26 05:42:39 | i | 2575 ± 203 | 0.89 | target ref diff | data |
| 61097.237498 | 2026-02-26 05:41:59 | i | 2209 ± 207 | 0.82 | target ref diff | data |
| 61097.237032 | 2026-02-26 05:41:19 | i | 2534 ± 217 | 0.89 | target ref diff | data |
| 61097.236564 | 2026-02-26 05:40:39 | i | 2395 ± 210 | 0.85 | target ref diff | data |
| 61097.236098 | 2026-02-26 05:39:58 | i | 2206 ± 213 | 0.68 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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