Reporting Group
Gattini
Discovering Data Source
Gattini
Discovery Date
2022-08-16 04:33:36.000
TNS AT
Y
Public
Y
Discovery Mag
14.28
Filter
J-Bessel
Reporter/s
Kishalay De
Light curves
▌Gattini_Gattini-camera_J
▌Other_Other_Clear
Pointer position (MJD, Mag, Abs.Mag): (0.00, 0.00, 0.00)
Spectra
No Data
Light Curves
AT Reports
ID | Time received (UT) | Sender | Reporter/s | Reporting group | Disc. Data Source | RA | DEC | Discovery date (UT) | Discovery Mag. | Filter | Related files | AT Type | Host name | Internal name | Assoc. Groups | End prop. period | Remarks | ADS Bibcode | Unreal | Auto classification |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
185001 | 2023-08-18 09:25:32 | MASTER | V.Shumkov,K.Vetrov,V. Lipunov et al. | MASTER | MASTER | 20:00:29.270 | +34:53:09.10 | 2023-08-16 23:25:09.120 | 15 | Clear- | Other | MASTER OT J200029.27+345309.1 | MASTER | inspection | N | |||||
155935 | 2022-08-26 13:22:18 | Kishalay De | Kishalay De et al. | Gattini | Gattini | 20:00:29.256 | +34:53:09.14 | 2022-08-16 04:33:36.000 | 14.28 | J-Bessel | PNV | Gattini | 2022TNSTR2471....1D | N |
Classification Reports
No Data
Comments
follow-up photometry from the Dominion Astrophysical Observatory
A series of expoures were acquired of at2022sfe on UT 2022 Aug. 29.332 (9 x 60 sec) in the SDSS g' filter. The field is not in the Sloan footprint and as such we are using a Gaia Star at (J2000):
of magnitude of G = 14.97 as a secondary standard. We find at2022sfe to be G = 19.72 +/- 0.04. Inspection of a PanSTARRS image stack shows two faint stars at the position of the transient separated by 5 seconds of arc. The northern star corresponds closely to the at position of the transient and has a published (Gaia) magnitude od 20.98