Discovery Date: 2026-02-25 06:29:20 UTC
Discovery MJD: 61096.27
Disc g-Flux: 2498.70±121.66
Latest Date: 2026-02-25 06:33:22 UTC
Latest MJD: 61096.27
Latest g-Flux: 2643.65±121.51
| Peak Flux | 2741.21±123.61 (g-band) |
| UTC at Peak | 2026-02-25 06:32:42 |
| MJD at Peak | 61096.27 |
| Detection Count | 3 |
| Equatorial Lon,Lat | 10:01:3.389, 02:30:26.212 |
| Galactic Lon,Lat | 236.603571, 42.414313 |
| Ecliptic Lon,Lat | 151.447459, -9.031248 |
| E(B-V) Extinction | 0.020360 |
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 SDSSJ100103.70%2B023053.1; an r=18.48 mag galaxy found in the NED/SDSS catalogues. Its located 26.95" S, 4.73" W (37.4 Kpc) from the galaxy centre. A host z=0.072 implies a m - M = 37.55.
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 06:49:37 | 0.7606773631210563 | r0b - Real Or Bogus Classifier | JSON data | https://las… |
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61096.273180 | 2026-02-25 06:33:22 | g | 2644 ± 122 | 0.72 | target ref diff | data |
| 61096.272711 | 2026-02-25 06:32:42 | g | 2741 ± 124 | 0.72 | target ref diff | data |
| 61096.272244 | 2026-02-25 06:32:01 | g | 2296 ± 125 | 0.60 | target ref diff | data |
| 61096.271777 | 2026-02-25 06:31:21 | g | 2311 ± 122 | 0.67 | target ref diff | data |
| 61096.271309 | 2026-02-25 06:30:41 | g | 2398 ± 121 | 0.68 | target ref diff | data |
| 61096.270840 | 2026-02-25 06:30:00 | g | 2172 ± 119 | 0.60 | target ref diff | data |
| 61096.270373 | 2026-02-25 06:29:20 | g | 2499 ± 122 | 0.62 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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