diaObjectId
170032920140972123

187.400257, 6.698486

Discovery Date: 2026-02-19 07:58:40 UTC
Discovery MJD: 61090.33
Disc r-Flux: 1507.43±249.95
Latest Date: 2026-02-24 05:00:03 UTC
Latest MJD: 61095.21
Latest r-Flux: 760.88±151.78
Peak Flux 1507.43±249.95 (r-band)
UTC at Peak 2026-02-19 07:58:40
MJD at Peak 61090.33
Detection Count 6
Equatorial Lon,Lat 12:29:36.062, 06:41:54.549
Galactic Lon,Lat 287.699821, 68.921969
Ecliptic Lon,Lat 184.121295, 9.085212
E(B-V) Extinction 0.017009
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 J122936.03+064154.3; an r=19.56 mag galaxy found in the SDSS/PS1/DESI catalogues. Its located 0.15" N, 0.43" E from the galaxy centre. A host photoZ=0.203 (±0.039) implies a m - M = 39.99.

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
61095.208374 2026-02-24 05:00:03 g 761 ± 152 0.11 target ref diff data
61095.189580 2026-02-24 04:32:59 r 1353 ± 235 0.14 target ref diff data
61095.185174 2026-02-24 04:26:38 r 848 ± 231 0.22 target ref diff data
61095.183777 2026-02-24 04:24:38 r 150 ± 237 0.12 target ref diff data
61095.177689 2026-02-24 04:15:52 g 906 ± 171 0.12 target ref diff data
61094.263945 2026-02-23 06:20:04 r 1002 ± 195 0.14 target ref diff data
61094.220566 2026-02-23 05:17:36 r 941 ± 190 0.13 target ref diff data
61091.252060 2026-02-20 06:02:57 r 1331 ± 216 0.13 target ref diff data
61091.248261 2026-02-20 05:57:29 r 1238 ± 238 0.13 target ref diff data
61090.332412 2026-02-19 07:58:40 r 1507 ± 250 0.31 target ref diff data
MJD filter magpsf magpsf_error flux_status
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