Discovery Date: 2026-02-25 04:36:34 UTC
Discovery MJD: 61096.19
Disc i-Flux: 6779.93±201.86
Latest Date: 2026-02-25 04:40:43 UTC
Latest MJD: 61096.19
Latest i-Flux: 6819.57±192.67
| Peak Flux | 7412.15±209.36 (i-band) |
| UTC at Peak | 2026-02-25 04:37:21 |
| MJD at Peak | 61096.19 |
| Detection Count | 2 |
| Equatorial Lon,Lat | 09:58:2.558, 03:28:0.005 |
| Galactic Lon,Lat | 234.955782, 42.343733 |
| Ecliptic Lon,Lat | 150.395980, -8.393796 |
| E(B-V) Extinction | 0.032204 |
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 SDSS J095802.13+032804.0; an r=19.47 mag galaxy found in the SDSS/PS1 catalogues. Its located 4.09" S, 6.42" E from the galaxy centre. A host photoZ=0.206 (±0.035) implies a m - M = 40.03.
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 | 2026-02-25 04:51:51 | 0.9714056325200665 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.194952 | 2026-02-25 04:40:43 | i | 6820 ± 193 | 1.00 | target ref diff | data |
| 61096.194485 | 2026-02-25 04:40:03 | i | 7374 ± 200 | 1.00 | target ref diff | data |
| 61096.194015 | 2026-02-25 04:39:22 | i | 7212 ± 199 | 1.00 | target ref diff | data |
| 61096.193548 | 2026-02-25 04:38:42 | i | 7320 ± 199 | 1.00 | target ref diff | data |
| 61096.193080 | 2026-02-25 04:38:02 | i | 6934 ± 205 | 1.00 | target ref diff | data |
| 61096.192613 | 2026-02-25 04:37:21 | i | 7412 ± 209 | 1.00 | target ref diff | data |
| 61096.192071 | 2026-02-25 04:36:34 | i | 6780 ± 202 | 1.00 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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