Discovery Date: 2026-02-26 05:26:58 UTC
Discovery MJD: 61097.23
Disc i-Flux: 6629.60±207.23
Latest Date: 2026-02-26 05:31:00 UTC
Latest MJD: 61097.23
Latest i-Flux: 6222.28±219.00
| Peak Flux | 6629.60±207.23 (i-band) |
| UTC at Peak | 2026-02-26 05:26:58 |
| MJD at Peak | 61097.23 |
| Detection Count | 1 |
| Equatorial Lon,Lat | 10:03:22.229, 02:30:3.829 |
| Galactic Lon,Lat | 237.066400, 42.881407 |
| Ecliptic Lon,Lat | 151.997566, -8.834418 |
| E(B-V) Extinction | 0.020947 |
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 15.29" N, 4.47" E (21.9 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 05:45:44 | 0.9637952286646795 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61097.229869 | 2026-02-26 05:31:00 | i | 6222 ± 219 | 1.00 | target ref diff | data |
| 61097.229401 | 2026-02-26 05:30:20 | i | 5988 ± 221 | 1.00 | target ref diff | data |
| 61097.228934 | 2026-02-26 05:29:39 | i | 6361 ± 222 | 1.00 | target ref diff | data |
| 61097.228467 | 2026-02-26 05:28:59 | i | 5811 ± 213 | 1.00 | target ref diff | data |
| 61097.227999 | 2026-02-26 05:28:19 | i | 6553 ± 210 | 1.00 | target ref diff | data |
| 61097.227536 | 2026-02-26 05:27:39 | i | 6430 ± 203 | 1.00 | target ref diff | data |
| 61097.227069 | 2026-02-26 05:26:58 | i | 6630 ± 207 | 1.00 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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