diaObjectId
170028537654280256

186.498694, 7.913263

Discovery Date: 2026-02-19 08:01:21 UTC
Discovery MJD: 61090.33
Disc r-Flux: 1261.31±234.72
Latest Date: 2026-02-24 04:58:02 UTC
Latest MJD: 61095.21
Latest r-Flux: 865.91±142.44
Peak Flux 2317.28±321.57 (i-band)
UTC at Peak 2026-02-24 03:59:03
MJD at Peak 61095.17
Detection Count 10
Equatorial Lon,Lat 12:25:59.686, 07:54:47.747
Galactic Lon,Lat 284.346038, 69.861597
Ecliptic Lon,Lat 182.797540, 9.840454
E(B-V) Extinction 0.023732
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 J122559.64+075447.5; an r=19.06 mag galaxy found in the SDSS/PS1/DESI catalogues. Its located 0.26" N, 0.94" E from the galaxy centre. A host photoZ=0.272 (±0.050) implies a m - M = 40.71.

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
61095.206972 2026-02-24 04:58:02 g 866 ± 142 0.14 target ref diff data
61095.180986 2026-02-24 04:20:37 g 889 ± 145 0.16 target ref diff data
61095.180030 2026-02-24 04:19:14 g 798 ± 158 0.12 target ref diff data
61095.177689 2026-02-24 04:15:52 g 870 ± 155 0.11 target ref diff data
61095.166017 2026-02-24 03:59:03 i 2317 ± 322 0.10 target ref diff data
61094.226877 2026-02-23 05:26:42 i 1522 ± 291 0.13 target ref diff data
61094.221284 2026-02-23 05:18:38 r 991 ± 200 0.13 target ref diff data
61094.218188 2026-02-23 05:14:11 r 882 ± 179 0.12 target ref diff data
61091.279644 2026-02-20 06:42:41 r 1096 ± 203 0.14 target ref diff data
61090.334272 2026-02-19 08:01:21 r 1261 ± 235 0.13 target ref diff data
MJD filter magpsf magpsf_error flux_status
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