RA/DEC (2000)
22:32:17.210 -23:42:09.04
338.071709079 -23.7025098783
Type
SN Ia
Redshift
0.065
Discovery ReportClassification Report
Reporting Group
Pan-STARRS
Discovering Data Source
Pan-STARRS
Discovery Date
2016-09-07 09:14:24.000
TNS AT
Y
Public
Y
Discovery Mag
18.83
Filter
w-P1
Reporter/s
K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, N. Primak, A. Schultz, (IfA, University of Hawaii), S. J. Smartt, K. W. Smith, (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright, D. R. Young (Queen's University Belfast)
NEDSIMBADDECaLSPanSTARRS-1SkyMapperVizieRWISEDSSADS

Spectra

 ▌SN_2016gcr - 2016-09-12 00:37:36 SALT / RSS (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_w
   
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
412 2016-09-12 00:37:36 SALT / RSS 1933 M. Kotze S. W. Jha None tns_2016gcr_2457643.526122687_SALT_RSS.dat tns_2016gcr_2457643.526122687_SALT_RSS.fits Object Significant host-galaxy contamination (host+SN was extracted).
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
w-P1 PS1_GPC1 2016-09-07 09:14:24 - 2016-09-07 09:14:24 2457638.885 - 2457638.885 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
7050 2016-09-07 09:14:24 2457638.885 18.83 0.02 22 ABMag w-P1 PS1_GPC1 45 Robot
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
5172 2016-09-08 23:10:05 PS1_Bot1 K. C. Chambers,M. E. Huber,H. Flewelling et al. Pan-STARRS Pan-STARRS 22:32:17.210 -23:42:09.04 2016-09-07 09:14:24.000 18.83 w-P1 PSN PS16eho Pan-STARRS 2016TNSTR.647....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
404 2016-09-13 09:16:58 Saurabh W. Jha Saurabh Jha None SN Ia 0.065 1 1 Cross-correlation of the spectrum with a supernova template library using SNID (Blondin & Tonry 2007, ApJ, 666, 1024) shows PS16eho is a type-Ia supernova approximately two weeks past maximum light. A good SNID match is obtained with SN 2005hf at +12 days. SNID matches to post-maximum SN Ic spectra are plausible, but not as compelling. 2016TNSCR.678....1J
Related files
File Comments Last Modified (UT) Modified By
tns_2016gcr_classrep_404.pdf SNID match to type-Ia SN 2005hf at +12 days. 2016-09-13 09:16:58 Saurabh W. Jha
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
412 2016-09-12 00:37:36 SALT / RSS 1933 M. Kotze S. W. Jha None tns_2016gcr_2457643.526122687_SALT_RSS.dat tns_2016gcr_2457643.526122687_SALT_RSS.fits Object Significant host-galaxy contamination (host+SN was extracted).

Comments