diaObjectId
170028529615372409

187.013853, 6.496303

Discovery Date: 2026-02-19 06:14:25 UTC
Discovery MJD: 61090.26
Disc g-Flux: 971.63±181.00
Latest Date: 2026-02-24 05:00:44 UTC
Latest MJD: 61095.21
Latest g-Flux: 859.01±170.85
Peak Flux 1629.39±181.86 (g-band)
UTC at Peak 2026-02-23 04:52:17
MJD at Peak 61094.20
Detection Count 8
Equatorial Lon,Lat 12:28:3.325, 06:29:46.690
Galactic Lon,Lat 286.806223, 68.632858
Ecliptic Lon,Lat 183.846853, 8.746529
E(B-V) Extinction 0.016402
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 10000,368499,9099; an r=21.15 mag galaxy found in the DESI catalogue. Its located 0.66" S, 0.60" E from the galaxy centre.

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
61095.208843 2026-02-24 05:00:44 g 859 ± 171 0.18 target ref diff data
61095.206506 2026-02-24 04:57:22 g 872 ± 165 0.13 target ref diff data
61095.180986 2026-02-24 04:20:37 g 1042 ± 183 0.15 target ref diff data
61095.180519 2026-02-24 04:19:56 g 1220 ± 190 0.13 target ref diff data
61094.242234 2026-02-23 05:48:49 g 1077 ± 168 0.18 target ref diff data
61094.237516 2026-02-23 05:42:01 g 890 ± 164 0.14 target ref diff data
61094.212987 2026-02-23 05:06:42 g 1293 ± 186 0.15 target ref diff data
61094.210510 2026-02-23 05:03:08 g 1296 ± 174 0.15 target ref diff data
61094.202976 2026-02-23 04:52:17 g 1629 ± 182 0.14 target ref diff data
61091.240999 2026-02-20 05:47:02 g 991 ± 164 0.15 target ref diff data
61090.260023 2026-02-19 06:14:25 g 972 ± 181 0.10 target ref diff data
MJD filter magpsf magpsf_error flux_status
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