Discovery Date: 2026-02-26 05:53:33 UTC
Discovery MJD: 61097.25
Disc i-Flux: 2902.82±192.21
Latest Date: 2026-02-26 05:57:35 UTC
Latest MJD: 61097.25
Latest i-Flux: 2754.16±189.40
| Peak Flux | 3113.53±205.26 (i-band) |
| UTC at Peak | 2026-02-26 05:56:54 |
| MJD at Peak | 61097.25 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 10:03:16.623, 01:30:3.154 |
| Galactic Lon,Lat | 238.146950, 42.274891 |
| Ecliptic Lon,Lat | 152.332159, -9.778822 |
| E(B-V) Extinction | 0.026251 |
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 2.69" S, 24.97" W (22.4 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 06:10:40 | 0.7835746652293358 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61097.248323 | 2026-02-26 05:57:35 | i | 2754 ± 189 | 0.97 | target ref diff | data |
| 61097.247857 | 2026-02-26 05:56:54 | i | 3114 ± 205 | 0.98 | target ref diff | data |
| 61097.247392 | 2026-02-26 05:56:14 | i | 2968 ± 195 | 0.95 | target ref diff | data |
| 61097.246923 | 2026-02-26 05:55:34 | i | 2829 ± 197 | 0.97 | target ref diff | data |
| 61097.246458 | 2026-02-26 05:54:53 | i | 2809 ± 186 | 0.96 | target ref diff | data |
| 61097.245992 | 2026-02-26 05:54:13 | i | 2748 ± 188 | 0.96 | target ref diff | data |
| 61097.245526 | 2026-02-26 05:53:33 | i | 2903 ± 192 | 0.96 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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