diaObjectId
170032919571595288

186.475154, 7.213110

Discovery Date: 2026-02-20 05:52:48 UTC
Discovery MJD: 61091.25
Disc g-Flux: 864.76±164.39
Latest Date: 2026-02-24 04:55:20 UTC
Latest MJD: 61095.21
Latest g-Flux: 816.39±149.97
Peak Flux 1063.09±167.25 (g-band)
UTC at Peak 2026-02-23 05:00:24
MJD at Peak 61094.21
Detection Count 10
Equatorial Lon,Lat 12:25:54.037, 07:12:47.194
Galactic Lon,Lat 284.847302, 69.183352
Ecliptic Lon,Lat 183.060362, 9.189630
E(B-V) Extinction 0.025763
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 J122554.2+071250.3; a J=14.30 mag galaxy found in the SDSS/DESI/PS1/2MASS catalogues. Its located 3.52" S, 3.48" W (5.8 Kpc) from the galaxy centre. A host z=0.076 implies a m - M = 37.69.

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
61095.205103 2026-02-24 04:55:20 g 816 ± 150 0.25 target ref diff data
61095.180986 2026-02-24 04:20:37 g 917 ± 155 0.23 target ref diff data
61095.180030 2026-02-24 04:19:14 g 821 ± 167 0.26 target ref diff data
61095.178157 2026-02-24 04:16:32 g 1057 ± 175 0.29 target ref diff data
61095.175815 2026-02-24 04:13:10 g -201 ± 196 0.13 target ref diff data
61095.174410 2026-02-24 04:11:09 g -503 ± 185 0.18 target ref diff data
61094.208621 2026-02-23 05:00:24 g 1063 ± 167 0.27 target ref diff data
61094.202976 2026-02-23 04:52:17 g 893 ± 178 0.26 target ref diff data
61091.264732 2026-02-20 06:21:12 g 863 ± 162 0.21 target ref diff data
61091.245012 2026-02-20 05:52:48 g 865 ± 164 0.25 target ref diff data
MJD filter magpsf magpsf_error flux_status
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