SN 2019duj
RA/DEC ()
13:29:32.228 +07:00:18.38
202.384284 +7.0051066
Type
SN Ia
Redshift
0.072
Source Group
ZTF
Discovery Date
2019-04-20 07:35:22
TNS AT
Y
Public
Y
Discovery Mag
19.06
Filter
g-ZTF
Discoverer/s
J. Nordin, V. Brinnel, M. Giomi, J. van Santen (HU Berlin), A. Gal-Yam, O. Yaron, S. Schulze (Weizmann) on behalf of ZTF

Spectra

 SN_2019duj - 2019-05-16 23:51:57 WHT-4.2m / ACAM (None)z=
 SN_2019duj - 2019-04-28 01:27:42 P60 / SEDM (ZTF)z=
Show H at z=vexp= km/s
Show He at z=vexp= km/s
Show He II 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 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 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)
Spectra
SelectIDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
46152019-05-16 23:51:57WHT-4.2m / ACAM2700C. Fariña (ING staff), I. Pérez-Fournon et al.R. Marques-ChavesNone tns_2019duj_2019-05-16_23-51-57_WHT-4.2m_ACAM.datObjectThe absorption feature at about 7600 Angstrom is due to uncorrected atmospheric absorption.
40432019-04-28 01:27:42P60 / SEDM2475SEDmRobotautoZTF tns_2019duj_2019-04-28_01-27-42_P60_SEDM_ZTF.asciiObjectZTF
Light Curves
FilterTel / InstObs-date rangePhotometry
g-ZTFP48_ZTF-Cam2019-04-14 08:59:15 - 2019-04-23 05:32:472
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
624672019-04-23 05:32:4719.060.0920.25ABMagg-ZTFP48_ZTF-Cam30
624662019-04-14 08:59:1519.562ABMagg-ZTFP48_ZTF-Cam30[Last non detection]
r-ZTFP48_ZTF-Cam2019-04-20 07:35:22 - 2019-04-20 07:35:221
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
624682019-04-20 07:35:2219.560.3219.1ABMagr-ZTFP48_ZTF-Cam30
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
334332019-04-23 08:36:19ZTF_AMPEL_NEWJ. Nordin, V. Brinnel, M. Giomi, J. van Santen (HU Berlin), A. Gal-Yam, O. Yaron, S. Schulze (Weizmann) on behalf of ZTFZTF13:29:32.228+07:00:18.382019-04-20 07:35:2219.06g-ZTFPSNZTF19aariwpfZTF
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
46082019-07-18 09:15:13ipfI. Perez-Fournon (IAC), C. Jimenez Angel (IAC), F. Poidevin (IAC), R. Shirley (IAC), R. Marques-Chaves (CAB), S. Geier (GRANTECAN), Y. Shu (IoA), S. Rodney (Univ. of South Carolina), J. Roberts-Pierel (Univ. of South Carolina), A. Bolton (NOAO), S. Chakrabarti (RIT), and B. Lewis (RIT)NoneSN Ia0.072We observed SN2019duj with the ACAM imager/spectrograph of the William Herschel Telescope (WHT) on 2019-05-16 23:51:57. Comparison with several libraries of SN spectra using SNID (S. Blondin & J. L. Tonry 2007, ApJ, 666, 1024) shows that this is likely a normal type Ia SN at z = 0.072, different from the larger redshift, z=0.351, reported to TNS by Fremling et al. from P60 / SEDM observations close to the maximum of the light curve. The SNID-derived phase of the WHT ACAM SN spectrum is 18 days after maximum. Our reanalysis of the P60 / SEDM SN spectrum of Fremling et al. shows also a good match to the type Ia SN2004dt close to maximum at z=0.074. SN2019duj is likely associated with SDSS J132932.20+070018.2 (with an SDSS-based photoZ=0.131 ± 0.028). The SN is located at only 0.4" from the galaxy nucleus. There are several galaxies within a few arcmin of SN2019duj and its host galaxy, with SDSS spectroscopic redshifts of z=0.074 - 0.075, that are part of the galaxy cluster MSPM 2057 (Smith et al. 2012, MNRAS, 422, 25). Our estimate of the redshift of SN2019duj is consistent with the spectroscopic redshift of the MSPM 2057 galaxy cluster.
40362019-05-10 20:26:04ZTF_Bot1C. Fremling, A. Dugas (Caltech), Y. Sharma (IIT Bombay) on behalf of the Zwicky Transient Facility (ZTF)ZTFSN Ia0.351ZTF