diaObjectId
170028532770013214

185.470095, 7.090790

Discovery Date: 2026-02-19 06:34:48 UTC
Discovery MJD: 61090.27
Disc i-Flux: 3310.33±364.45
Latest Date: 2026-02-24 05:07:48 UTC
Latest MJD: 61095.21
Latest i-Flux: 1696.67±315.06
Peak Flux 6738.62±448.69 (i-band)
UTC at Peak 2026-02-23 05:23:16
MJD at Peak 61094.22
Detection Count 11
Equatorial Lon,Lat 12:21:52.823, 07:05:26.846
Galactic Lon,Lat 282.294458, 68.769947
Ecliptic Lon,Lat 182.184945, 8.678181
E(B-V) Extinction 0.018528

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: Nuclear Transient

The transient is synonymous with SDSS J122152.85+070526.0; an r=16.96 mag galaxy found in the SDSS catalogue. Its located 1.0" (1.4 Kpc) from the galaxy core. A host z=0.075 implies a m - M = 37.64.

Difference Image Lightcurve

Access the data from this plot in the LSST Alert Packet Data table below.

Context Map

Recent Image Stamps

target

reference

difference

LSST Alert Packet Data

MJD UTC band target diff flux reliability images alert packet
61095.213751 2026-02-24 05:07:48 r 1697 ± 315 0.13 target ref diff data
61095.212819 2026-02-24 05:06:27 r 1932 ± 324 0.30 target ref diff data
61095.201268 2026-02-24 04:49:49 i 4920 ± 475 0.22 target ref diff data
61095.193902 2026-02-24 04:39:13 i 3292 ± 425 0.23 target ref diff data
61095.188449 2026-02-24 04:31:21 r 2605 ± 376 0.26 target ref diff data
61094.250129 2026-02-23 06:00:11 r 1404 ± 273 0.14 target ref diff data
61094.246450 2026-02-23 05:54:53 r 2652 ± 321 0.10 target ref diff data
61094.224501 2026-02-23 05:23:16 i 6739 ± 449 0.35 target ref diff data
61094.199582 2026-02-23 04:47:23 i 3647 ± 420 0.25 target ref diff data
61090.326282 2026-02-19 07:49:50 g 1942 ± 301 0.19 target ref diff data
61090.274634 2026-02-19 06:35:28 i 2178 ± 425 0.34 target ref diff data
61090.274169 2026-02-19 06:34:48 i 3310 ± 364 0.16 target ref diff data
MJD filter magpsf magpsf_error flux_status
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