diaObjectId
170059313215701089

150.009479, 2.509537

Discovery Date: 2026-02-26 07:20:10 UTC
Discovery MJD: 61097.31
Disc r-Flux: 2354.50±166.05
Latest Date: 2026-02-26 07:24:52 UTC
Latest MJD: 61097.31
Latest r-Flux: 2164.95±161.55
Peak Flux 2354.50±166.05 (r-band)
UTC at Peak 2026-02-26 07:20:10
MJD at Peak 61097.31
Detection Count 1
Equatorial Lon,Lat 10:00:2.275, 02:30:34.334
Galactic Lon,Lat 236.402473, 42.207897
Ecliptic Lon,Lat 151.205270, -9.118003
E(B-V) Extinction 0.017302
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 COSMOS2381493; a 24.80 mag VisS found in the NED catalogue. Its located 3.96" S, 3.41" E from the VisS centre. A host photoZ=0.470 implies a m - M = 42.10.

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

Annotations

Annotator Timestamp Annotation Explanation JSON Data Link
r0b_lvra a1 2026-02-26 11:42:04 0.939130284409246 r0b - Real Or Bogus Classifier JSON data https://las…

LSST Alert Packet Data

MJD UTC band target diff flux reliability images alert packet
61097.308945 2026-02-26 07:24:52 r 2165 ± 162 0.91 target ref diff data
61097.308475 2026-02-26 07:24:12 r 2116 ± 158 0.85 target ref diff data
61097.308008 2026-02-26 07:23:31 r 1994 ± 161 0.84 target ref diff data
61097.307541 2026-02-26 07:22:51 r 2166 ± 161 0.92 target ref diff data
61097.307074 2026-02-26 07:22:11 r 1963 ± 168 0.88 target ref diff data
61097.306605 2026-02-26 07:21:30 r 2116 ± 163 0.87 target ref diff data
61097.306137 2026-02-26 07:20:50 r 2178 ± 163 0.89 target ref diff data
61097.305672 2026-02-26 07:20:10 r 2354 ± 166 0.91 target ref diff data
MJD filter magpsf magpsf_error flux_status
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