diaObjectId
170028521394536525

149.724225, 3.674773

Discovery Date: 2026-02-19 05:25:14 UTC
Discovery MJD: 61090.23
Disc g-Flux: -2014.04±252.25
Latest Date: 2026-02-24 03:23:31 UTC
Latest MJD: 61095.14
Latest g-Flux: -1127.28±174.06
Peak Flux -1023.54±206.25 (g-band)
UTC at Peak 2026-02-20 04:55:47
MJD at Peak 61091.21
Detection Count 10
Equatorial Lon,Lat 09:58:53.814, 03:40:29.182
Galactic Lon,Lat 234.885001, 42.637019
Ecliptic Lon,Lat 150.525087, -8.124693
E(B-V) Extinction 0.026224

Transient Name Server

AT2025wt

The transient was discovered on 20th January 2025 at 07:37:13 (MJD 60695.32) by ZTF as ZTF25aacqtcq with a discovery magnitude of r = 19.54..

Sherlock Contextual Classification

Prediction: Nuclear Transient

The transient is synonymous with SDSSJ095853.85%2B034029.1; a J=15.93 mag galaxy found in the NED/SDSS/2MASS catalogues. Its located 0.7" (2.0 Kpc) from the galaxy core. A host z=0.152 implies a m - M = 39.30.

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
61095.141340 2026-02-24 03:23:31 g -1127 ± 174 0.31 target ref diff data
61095.128531 2026-02-24 03:05:05 r -1917 ± 253 0.20 target ref diff data
61095.113173 2026-02-24 02:42:58 g -1229 ± 220 0.19 target ref diff data
61095.110767 2026-02-24 02:39:30 g -1443 ± 226 0.18 target ref diff data
61094.171230 2026-02-23 04:06:34 g -1056 ± 183 0.23 target ref diff data
61094.167940 2026-02-23 04:01:50 g -1442 ± 223 0.41 target ref diff data
61094.138624 2026-02-23 03:19:37 g -1297 ± 222 0.34 target ref diff data
61091.210659 2026-02-20 05:03:20 g -2284 ± 351 0.18 target ref diff data
61091.205407 2026-02-20 04:55:47 g -1024 ± 206 0.33 target ref diff data
61090.226324 2026-02-19 05:25:54 g -1926 ± 265 0.35 target ref diff data
61090.225862 2026-02-19 05:25:14 g -2014 ± 252 0.25 target ref diff data
MJD filter magpsf magpsf_error flux_status
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