Discovery Date: 2026-02-20 05:37:40 UTC
Discovery MJD: 61091.23
Disc i-Flux: -2095.57±278.22
Latest Date: 2026-02-24 04:05:48 UTC
Latest MJD: 61095.17
Latest i-Flux: -2213.89±302.49
| Peak Flux | -1540.16±298.18 (i-band) |
| UTC at Peak | 2026-02-20 06:17:47 |
| MJD at Peak | 61091.26 |
| Detection Count | 9 |
| Equatorial Lon,Lat | 12:22:41.513, 07:47:22.538 |
| Galactic Lon,Lat | 282.208239, 69.496482 |
| Ecliptic Lon,Lat | 182.087901, 9.399020 |
| E(B-V) Extinction | 0.022675 |
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 J122241.52+074722.6; an r=20.47 mag galaxy found in the SDSS/PS1/DESI catalogues. Its located 0.17" S, 0.11" W from the galaxy centre.
Difference Image Lightcurve
Access the data from this plot in the LSST Alert Packet Data table below.
Context Map
LSST Alert Packet Data
| MJD | UTC | band | target diff flux | reliability | images | alert packet |
|---|---|---|---|---|---|---|
| 61095.170699 | 2026-02-24 04:05:48 | i | -2214 ± 302 | 0.22 | target ref diff | data |
| 61095.169293 | 2026-02-24 04:03:46 | i | -2025 ± 306 | 0.10 | target ref diff | data |
| 61094.229264 | 2026-02-23 05:30:08 | i | -2111 ± 287 | 0.12 | target ref diff | data |
| 61094.224501 | 2026-02-23 05:23:16 | i | -2708 ± 287 | 0.21 | target ref diff | data |
| 61094.198629 | 2026-02-23 04:46:01 | i | -2401 ± 307 | 0.10 | target ref diff | data |
| 61091.262359 | 2026-02-20 06:17:47 | i | -1540 ± 298 | 0.31 | target ref diff | data |
| 61091.261894 | 2026-02-20 06:17:07 | i | -2413 ± 282 | 0.17 | target ref diff | data |
| 61091.256706 | 2026-02-20 06:09:39 | i | -1671 ± 280 | 0.14 | target ref diff | data |
| 61091.256241 | 2026-02-20 06:08:59 | i | -1873 ± 282 | 0.18 | target ref diff | data |
| 61091.234500 | 2026-02-20 05:37:40 | i | -2096 ± 278 | 0.14 | target ref diff | data |
| MJD | filter | magpsf | magpsf_error | flux_status |
|---|
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