TNS Classification Report No. 7244 [ 2020TNSCR2311....1P ]
Date Received (UTC): 2020-07-28 21:57:05 Sender: Ismael Perez-Fournon
Group: SIRAH
Frederick Poidevin, Ismael Perez-Fournon, Camilo Jimenez Angel (IAC and ULL), Thomas Brink, WeiKang Zheng, Alexei Filippenko (UC Berkeley), Saurabh W. Jha, Mi Dai (Rutgers), Raphael Shirley (Univ. Southampton), Rui Marques Chaves (CAB), Qinan Wang, Sofia Rest (JHU), Armin Rest (STScI), and Steve Rodney (Univ. of South Carolina), on behalf of the SIRAH team report/s a classification of object: SN 2020qic
Type: SN IaRedshift: 0.048
Remarks: Spectra of SN 2020qic were obtained with the Liverpool Telescope + SPRAT spectrograph at the Observatorio del Roque de los Muchachos and with the Lick Observatory 3m Shane Telescope + KAST spectrograph. In the 3m Shane Telescope + KAST observations the host galaxy was also placed on the slit and it gives z = 0.048 from numerous emission lines. For both spectra SNID (S. Blondin & J. L. Tonry 2007, ApJ, 666, 1024) shows good matches to the normal SN Ia 2005eu at one week before maximum light or earlier.
The following Classification spectrum was provided:
Obsdate: 2020-07-28 02:02:49
Instrument: SPRAT
Telescope: Liverpool Telescope
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2020qic
Date Received (UTC): 2020-07-28 21:57:05 Sender: Ismael Perez-Fournon
Group: SIRAH
Frederick Poidevin, Ismael Perez-Fournon, Camilo Jimenez Angel (IAC and ULL), Thomas Brink, WeiKang Zheng, Alexei Filippenko (UC Berkeley), Saurabh W. Jha, Mi Dai (Rutgers), Raphael Shirley (Univ. Southampton), Rui Marques Chaves (CAB), Qinan Wang, Sofia Rest (JHU), Armin Rest (STScI), and Steve Rodney (Univ. of South Carolina), on behalf of the SIRAH team report/s a classification of object: SN 2020qic
Type: SN IaRedshift: 0.048
Remarks: Spectra of SN 2020qic were obtained with the Liverpool Telescope + SPRAT spectrograph at the Observatorio del Roque de los Muchachos and with the Lick Observatory 3m Shane Telescope + KAST spectrograph. In the 3m Shane Telescope + KAST observations the host galaxy was also placed on the slit and it gives z = 0.048 from numerous emission lines. For both spectra SNID (S. Blondin & J. L. Tonry 2007, ApJ, 666, 1024) shows good matches to the normal SN Ia 2005eu at one week before maximum light or earlier.
The following Classification spectrum was provided:
Obsdate: 2020-07-28 02:02:49
Instrument: SPRAT
Telescope: Liverpool Telescope
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2020qic