diaObjectId
170028513202536498

150.238220, 3.143765

Discovery Date: 2026-02-19 04:33:41 UTC
Discovery MJD: 61090.19
Disc g-Flux: 1226.51±226.87
Latest Date: 2026-02-24 02:42:58 UTC
Latest MJD: 61095.11
Latest g-Flux: 1064.90±201.58
Peak Flux 2757.52±196.89 (g-band)
UTC at Peak 2026-02-23 04:11:09
MJD at Peak 61094.17
Detection Count 10
Equatorial Lon,Lat 10:00:57.173, 03:08:37.556
Galactic Lon,Lat 235.875916, 42.758942
Ecliptic Lon,Lat 151.197930, -8.443920
E(B-V) Extinction 0.025174
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 CGCG036-019; a J=12.06 mag galaxy found in the NED/SDSS/PS1/DESI/2MASS catalogues. Its located 7.11" N, 1.25" W (4.1 Kpc) from the galaxy centre. A host z=0.029 implies a m - M = 35.54.

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
61095.113173 2026-02-24 02:42:58 g 1065 ± 202 0.37 target ref diff data
61094.174411 2026-02-23 04:11:09 g 2758 ± 197 0.40 target ref diff data
61094.169335 2026-02-23 04:03:50 g 1134 ± 217 0.37 target ref diff data
61094.139626 2026-02-23 03:21:03 g 1040 ± 191 0.30 target ref diff data
61094.139088 2026-02-23 03:20:17 g 1102 ± 199 0.36 target ref diff data
61091.202643 2026-02-20 04:51:48 i 1752 ± 323 0.26 target ref diff data
61091.175429 2026-02-20 04:12:37 g 1074 ± 214 0.37 target ref diff data
61090.194715 2026-02-19 04:40:23 g 2183 ± 244 0.33 target ref diff data
61090.191459 2026-02-19 04:35:42 g 1127 ± 228 0.36 target ref diff data
61090.190066 2026-02-19 04:33:41 g 1227 ± 227 0.35 target ref diff data
MJD filter magpsf magpsf_error flux_status
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