diaObjectId
170028538061652034

187.077838, 8.729432

Discovery Date: 2026-02-19 08:03:22 UTC
Discovery MJD: 61090.34
Disc r-Flux: 13737.47±679.81
Latest Date: 2026-02-24 04:40:33 UTC
Latest MJD: 61095.19
Latest r-Flux: 5745.08±502.21
Peak Flux 13737.47±679.81 (r-band)
UTC at Peak 2026-02-19 08:03:22
MJD at Peak 61090.34
Detection Count 9
Equatorial Lon,Lat 12:28:18.681, 08:43:45.954
Galactic Lon,Lat 285.302965, 70.805447
Ecliptic Lon,Lat 182.997925, 10.818025
E(B-V) Extinction 0.021306
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: Nuclear Transient

The transient is synonymous with UGC07590; an r=14.18 mag galaxy found in the NED-D/SDSS/LASR catalogues. Its located 1.2" (0.2 Kpc) from the galaxy core. A host distance of 28.6 Mpc(z=0.004) implies a m - M = 32.28.

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
61095.194838 2026-02-24 04:40:33 i 5745 ± 502 0.18 target ref diff data
61095.180986 2026-02-24 04:20:37 g 4931 ± 314 0.30 target ref diff data
61095.171640 2026-02-24 04:07:09 i -2651 ± 494 0.31 target ref diff data
61094.235676 2026-02-23 05:39:22 g 2168 ± 294 0.20 target ref diff data
61094.211945 2026-02-23 05:05:12 g 2965 ± 373 0.28 target ref diff data
61094.211468 2026-02-23 05:04:30 g 2256 ± 360 0.29 target ref diff data
61094.198629 2026-02-23 04:46:01 i 3084 ± 451 0.11 target ref diff data
61091.269145 2026-02-20 06:27:34 g 5810 ± 803 0.10 target ref diff data
61091.240066 2026-02-20 05:45:41 g 3273 ± 347 0.20 target ref diff data
61090.335674 2026-02-19 08:03:22 r 13737 ± 680 0.11 target ref diff data
MJD filter magpsf magpsf_error flux_status
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