Discovery Date: 2026-02-26 04:25:38 UTC
Discovery MJD: 61097.18
Disc i-Flux: 2405.07±212.47
Latest Date: 2026-02-26 04:29:40 UTC
Latest MJD: 61097.19
Latest i-Flux: 2408.92±231.53
| Peak Flux | 2947.68±246.00 (i-band) |
| UTC at Peak | 2026-02-26 04:29:00 |
| MJD at Peak | 61097.19 |
| Detection Count | 3 |
| Equatorial Lon,Lat | 10:02:8.762, 01:47:19.750 |
| Galactic Lon,Lat | 237.607614, 42.216651 |
| Ecliptic Lon,Lat | 151.960985, -9.608731 |
| E(B-V) Extinction | 0.019806 |
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%2B014722.1; an r=20.83 mag galaxy found in the NED/SDSS catalogues. Its located 2.35" S, 24.02" E (37.0 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 04:46:53 | 0.3397662346799702 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61097.187274 | 2026-02-26 04:29:40 | i | 2409 ± 232 | 0.83 | target ref diff | data |
| 61097.186806 | 2026-02-26 04:29:00 | i | 2948 ± 246 | 0.91 | target ref diff | data |
| 61097.186338 | 2026-02-26 04:28:19 | i | 2496 ± 228 | 0.91 | target ref diff | data |
| 61097.185872 | 2026-02-26 04:27:39 | i | 2613 ± 228 | 0.92 | target ref diff | data |
| 61097.185405 | 2026-02-26 04:26:59 | i | 2501 ± 220 | 0.87 | target ref diff | data |
| 61097.184940 | 2026-02-26 04:26:18 | i | 2149 ± 212 | 0.76 | target ref diff | data |
| 61097.184471 | 2026-02-26 04:25:38 | i | 2405 ± 212 | 0.78 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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