RA/DEC (2000)
05:50:55.518 -14:47:21.22
87.731324 -14.789227
Type
---
Redshift
Discovery Report
Reporting Group
GOTO
Discovering Data Source
GOTO
Discovery Date
2024-09-28 04:44:54.240
TNS AT
Y
Public
Y
Discovery Mag
18.69
Filter
L-GOTO
Reporter/s
K. Ulaczyk, G. Ramsay, K. Ackley, M. Dyer, F. Jiménez-Ibarra, J. Lyman, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, L. Nuttall, E. Pallé, D. Pollacco, T. Killestein, A. Kumar, D. O'Neill, on behalf of GOTO collaboration
NEDSIMBADDECaLSPanSTARRS-1SkyMapperVizieRWISEDSSADS

Light curves

 ▌GOTO-N_GOTO-2_L
 ▌GOTO-N_GOTO-1_L
   
Pointer position (MJD, Mag, Abs.Mag): (0.00, 0.00, 0.00)
No Data
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
L-GOTO GOTO-N_GOTO-2 2024-09-28 04:44:54 - 2024-09-28 04:44:54 2460581.697854 - 2460581.697854 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
436193 2024-09-28 04:44:54 2460581.697854 18.69 0.1 ABMag L-GOTO GOTO-N_GOTO-2 180
L-GOTO GOTO-N_GOTO-1 2024-09-26 03:48:38 - 2024-09-26 03:48:38 2460579.658768 - 2460579.658768 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
436192 2024-09-26 03:48:38 2460579.658768 19.4 ABMag L-GOTO GOTO-N_GOTO-1 180 [Last non detection]
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
226996 2024-09-28 07:38:21 GOTO_bot K. Ulaczyk, G. Ramsay, K. Ackley et al. GOTO GOTO 05:50:55.518 -14:47:21.22 2024-09-28 04:44:54.240 18.69 L-GOTO Other GOTO24gin GOTO 2024TNSTR3750....1U N
No Data

Comments

Shubham
Srivastav

Sun, 12/22/2024 - 17:58

ATLAS non-detection following GOTO discovery

We note that following GOTO discovery on MJD 60581.20, we registered a non-detection in ATLAS 1.4 days later on MJD 60582.60, with o > 19.9 mag. Also, we note that AT2024wta is coincident with a red archival source in the Pan-STARRS stamp. Along with the rapid fading, this suggests that AT2024wta is likely a foreground variable or M-dwarf flare event.