diaObjectId
170046109549330626

186.482910, 7.909374

Discovery Date: 2026-02-23 05:03:50 UTC
Discovery MJD: 61094.21
Disc g-Flux: 744.76±142.98
Latest Date: 2026-02-24 04:58:42 UTC
Latest MJD: 61095.21
Latest g-Flux: 878.97±138.99
Peak Flux 2143.73±321.38 (i-band)
UTC at Peak 2026-02-24 04:47:42
MJD at Peak 61095.20
Detection Count 7
Equatorial Lon,Lat 12:25:55.898, 07:54:33.747
Galactic Lon,Lat 284.305782, 69.853389
Ecliptic Lon,Lat 182.784589, 9.830620
E(B-V) Extinction 0.023317
Duplicate diaObjects

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 J122555.84+075433.5; an r=19.24 mag unclear found in the SDSS/DESI/PS1 catalogues. Its located 0.20" N, 0.75" E from the unclear centre. A host photoZ=0.269 (±0.032) implies a m - M = 40.69.

Difference Image Lightcurve

Access the data from this plot in the LSST Alert Packet Data table below.
Learn how to interact with this plot.

Context Map

Recent Image Stamps

target

reference

difference

External Resources

Alerce Antares DECaLS Fink NED SIMBAD ZTF

LSST Alert Packet Data

MJD UTC band target diff flux reliability images alert packet
61095.207439 2026-02-24 04:58:42 g 879 ± 139 0.14 target ref diff data
61095.204636 2026-02-24 04:54:40 g 799 ± 141 0.15 target ref diff data
61095.199798 2026-02-24 04:47:42 i 2144 ± 321 0.12 target ref diff data
61095.187515 2026-02-24 04:30:01 r 1393 ± 220 0.15 target ref diff data
61095.180986 2026-02-24 04:20:37 g 766 ± 146 0.15 target ref diff data
61095.180030 2026-02-24 04:19:14 g 921 ± 157 0.14 target ref diff data
61095.176283 2026-02-24 04:13:50 g 741 ± 143 0.12 target ref diff data
61095.174878 2026-02-24 04:11:49 g 1106 ± 159 0.20 target ref diff data
61094.233786 2026-02-23 05:36:39 g 692 ± 130 0.16 target ref diff data
61094.211001 2026-02-23 05:03:50 g 745 ± 143 0.15 target ref diff data
MJD filter magpsf magpsf_error flux_status
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