Discovery Date: 2026-02-27 05:05:11 UTC
Discovery MJD: 61098.21
Disc i-Flux: 2435.55±261.81
Latest Date: 2026-02-27 05:09:14 UTC
Latest MJD: 61098.21
Latest i-Flux: 2928.52±249.74
| Peak Flux | 3122.73±251.47 (i-band) |
| UTC at Peak | 2026-02-27 05:06:32 |
| MJD at Peak | 61098.21 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 12:28:51.621, 07:06:7.547 |
| Galactic Lon,Lat | 286.926830, 69.269284 |
| Ecliptic Lon,Lat | 183.787130, 9.381695 |
| E(B-V) Extinction | 0.019243 |
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 SDSSJ122850.46%2B070629.4; an r=17.46 mag galaxy found in the NED/SDSS catalogues. Its located 21.90" S, 17.30" E (40.2 Kpc) from the galaxy centre. A host z=0.076 implies a m - M = 37.69.
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 | 2026-02-27 05:20:00 | 0.6839890458758751 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61098.214749 | 2026-02-27 05:09:14 | i | 2929 ± 250 | 0.91 | target ref diff | data |
| 61098.214280 | 2026-02-27 05:08:33 | i | 2505 ± 248 | 0.89 | target ref diff | data |
| 61098.213812 | 2026-02-27 05:07:53 | i | 2911 ± 256 | 0.97 | target ref diff | data |
| 61098.213341 | 2026-02-27 05:07:12 | i | 2747 ± 252 | 0.87 | target ref diff | data |
| 61098.212871 | 2026-02-27 05:06:32 | i | 3123 ± 251 | 0.97 | target ref diff | data |
| 61098.212403 | 2026-02-27 05:05:51 | i | 2935 ± 261 | 0.95 | target ref diff | data |
| 61098.211936 | 2026-02-27 05:05:11 | i | 2436 ± 262 | 0.73 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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