Discovery Date: 2026-02-26 05:43:19 UTC
Discovery MJD: 61097.24
Disc i-Flux: 3376.56±205.75
Latest Date: 2026-02-26 05:47:21 UTC
Latest MJD: 61097.24
Latest i-Flux: 2943.55±185.69
| Peak Flux | 3376.56±205.75 (i-band) |
| UTC at Peak | 2026-02-26 05:43:19 |
| MJD at Peak | 61097.24 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 10:03:16.932, 01:30:0.345 |
| Galactic Lon,Lat | 238.148833, 42.275468 |
| Ecliptic Lon,Lat | 152.333664, -9.779097 |
| E(B-V) Extinction | 0.026265 |
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 SDSSJ100318.28%2B013005.8; an r=17.33 mag galaxy found in the NED/SDSS catalogues. Its located 5.46" S, 20.36" W (18.8 Kpc) from the galaxy centre. A host z=0.045 implies a m - M = 36.52.
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 06:05:31 | 0.7651536045601817 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61097.241226 | 2026-02-26 05:47:21 | i | 2944 ± 186 | 0.96 | target ref diff | data |
| 61097.240758 | 2026-02-26 05:46:41 | i | 3045 ± 190 | 0.98 | target ref diff | data |
| 61097.240290 | 2026-02-26 05:46:01 | i | 3202 ± 193 | 0.97 | target ref diff | data |
| 61097.239824 | 2026-02-26 05:45:20 | i | 3003 ± 196 | 0.97 | target ref diff | data |
| 61097.239358 | 2026-02-26 05:44:40 | i | 3207 ± 193 | 0.98 | target ref diff | data |
| 61097.238893 | 2026-02-26 05:44:00 | i | 3292 ± 200 | 0.98 | target ref diff | data |
| 61097.238423 | 2026-02-26 05:43:19 | i | 3377 ± 206 | 0.98 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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