RA/DEC (2000)
03:38:01.190 -26:56:46.77
54.5049599517 -26.9463260969
Type
SN
Redshift
0.4245
Discovery ReportClassification Report
Reporting Group
Pan-STARRS
Discovering Data Source
Pan-STARRS
Discovery Date
2019-01-15 05:22:33.000
TNS AT
Y
Public
Y
Discovery Mag
18.24
Filter
i-Sloan
Reporter/s
K. C. Chambers, T. de Boer, J. Bulger, J. Fairlamb, M. Huber, C.-C. Lin, T. Lowe, E. Magnier, A. Schultz, R. J. Wainscoat, M. Willman (IfA, University of Hawaii), K. W. Smith, D. R. Young, O. McBrien, J. Gillanders. S. Srivastav, S. J. Smartt, D. O'Neil, P. Clark, S. Sim (Queen's University Belfast), D. E. Wright (University of Minnesota)
NEDSIMBADDECaLSPanSTARRS-1SkyMapperVizieRWISEDSSADS

Spectra

 ▌SN_2019jrj - 2019-02-03 00:00:00 VLT-UT1 / FORS2 (None)z=
▌Show H at z=vexp= km/s
▌Show He at z=vexp= km/s
▌Show He II at z=vexp= km/s
▌Show C II at z=vexp= km/s
▌Show C III at z=vexp= km/s
▌Show C IV at z=vexp= km/s
▌Show N II at z=vexp= km/s
▌Show N III at z=vexp= km/s
▌Show N IV at z=vexp= km/s
▌Show N V at z=vexp= km/s
▌Show O at z=vexp= km/s
▌Show [O I] at z=vexp= km/s
▌Show O II at z=vexp= km/s
▌Show [O II] at z=vexp= km/s
▌Show [O III] at z=vexp= km/s
▌Show O V at z=vexp= km/s
▌Show O VI at z=vexp= km/s
▌Show Na at z=vexp= km/s
▌Show Mg at z=vexp= km/s
▌Show Mg II at z=vexp= km/s
▌Show Si II at z=vexp= km/s
▌Show S II at z=vexp= km/s
▌Show Ca II at z=vexp= km/s
▌Show [Ca II] at z=vexp= km/s
▌Show Fe II at z=vexp= km/s
▌Show Fe III at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Tellurics 
▌Show Galaxy lines at z=
▌Show WR-WN at z=vexp= km/s
▌Show WR-WC/O at z=vexp= km/s
   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),0 (observed)

Light curves

 ▌PS1_GPC1_i
 ▌VLT-UT1_FORS2_z
 ▌Other_Other_Clear
   
Pointer position (MJD, Mag, Abs.Mag): (0.00, 0.00, 0.00)
Spectra
 ID Obs-date (UT) Tel / Inst Exp-Time Observer/s Reducer/s Group Spectrum ascii file Spectrum fits file Spec. Type Assoc. Groups End prop. period Remarks
8619 2019-02-03 00:00:00 VLT-UT1 / FORS2 E. Pian None tns_2019jrj_2019-02-03_VLT-UT1_FORS2_0.txt tns_2019jrj_2019-02-03_VLT-UT1_FORS2.fits Object 2021-07-19 The uploaded reduced spectrum (ASCII file) corresponds to the supernova emission associated with GRB190114C. The detailed description of the reduction procedure (removal of the GRB afterglow and host-galaxy contributions) is described in the paper we are in the process to submit.
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
i-P1 PS1_GPC1 2019-01-15 05:22:33 - 2019-01-15 05:22:33 2458498.7239931 - 2458498.7239931 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
75279 2019-01-15 05:22:33 2458498.7239931 18.24 0.02 20.7 ABMag i-P1 PS1_GPC1 45 Robot
z-Sloan VLT-UT1_FORS2 2019-02-03 00:00:00 - 2019-02-03 00:00:00 2458517.5 - 2458517.5 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
186923 2019-02-03 00:00:00 2458517.5 20.81 0.07 ABMag z-Sloan VLT-UT1_FORS2 We observed GRB190114C for several epochs with VLT/FORS2. GRB190114C is located in the nuclear region of an interacting galaxy. The reported magnitude refers to the aperture magnitude of the two-galaxies system.
Clear- Other_Other 2015-08-26 04:52:08 - 2019-01-14 21:04:44 2457260.7028704 - 2458498.378287 3
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
118840 2019-01-14 21:04:44 2458498.378287 15.5 18.4 VegaMag Clear- Other_Other 90 Robot MASTER-IAC
118841 2019-01-14 21:04:44 2458498.378287 15.4 18.4 VegaMag Clear- Other_Other 90 Robot MASTER-IAC
118839 2015-08-26 04:52:08 2457260.7028704 20 VegaMag Clear- Other_Other 540 Robot [Last non detection] MASTER-IAC
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
96872 2021-01-15 15:09:31 Andrea Melandri Andrea Melandri et al. 03:38:01.160 -26:56:46.90 2019-02-03 00:00:00.000 20.81 z-Sloan 1 PSN 2021-03-16 We observed GRB190114C for several epochs with VLT/FORS2. Here we are reporting the detection evidence of the associated supernova (SN) emission. Our aim is to get a name for the associated SN as it is typically done for other GRB/SN connections. N
Related files
File Comments Last Modified (UT) Modified By
tns_2019jrj_atrep_96872.png This a VLT image (R-filter) of the two-galaxies system where GRB190114C is located. The object marked with A is the host-galaxy of the GRB/SN. 2021-01-15 15:09:31 Andrea Melandri
61150 2020-02-05 21:20:30 MASTER V. Lipunov,E. Gorbovskoy,V.Kornilov et al. MASTER MASTER 03:38:01.170 -26:56:46.70 2019-01-14 21:04:44.000 15.5 Clear- Other MASTER OT J033801.17-265646.7 MASTER grbxxyyzz.ff MASTER optical counterpart candidate N
39937 2019-07-01 08:36:11 PS1_Bot1 K. C. Chambers,T. de Boer,J. Bulger et al. Pan-STARRS Pan-STARRS 03:38:01.190 -26:56:46.77 2019-01-15 05:22:33.000 18.24 i-P1 PSN PS19ctb Pan-STARRS 2019TNSTR1114....1C N
Classification Reports
ID Time received (UT) Sender Classifier/s Group Classification Redshift Spectra Related files Assoc. Groups End prop. period Remarks ADS Bibcode
8607 2021-01-19 09:57:53 Andrea Melandri Andrea Melandri None SN 0.4245 1 1 2021TNSCR.203....1M
Related files
File Comments Last Modified (UT) Modified By
tns_2019jrj_classrep_8607.png 2021-01-19 09:57:53 Andrea Melandri
Spectra
ID Obs-date (UT) Tel / Inst Exp-Time Observer/s Reducer/s Group Spectrum ascii file Spectrum fits file Spec. Type Assoc. Groups End prop. period Remarks
8619 2019-02-03 00:00:00 VLT-UT1 / FORS2 E. Pian None tns_2019jrj_2019-02-03_VLT-UT1_FORS2_0.txt tns_2019jrj_2019-02-03_VLT-UT1_FORS2.fits Object 2021-07-19 The uploaded reduced spectrum (ASCII file) corresponds to the supernova emission associated with GRB190114C. The detailed description of the reduction procedure (removal of the GRB afterglow and host-galaxy contributions) is described in the paper we are in the process to submit.

Comments