TNS Classification Report No. 3621 [ 2019TNSCR.337....1S ]
Date Received (UTC): 2019-03-06 15:30:37 Sender: Lina Tomasella
Group: Padova-Asiago
Schuldt, Vogl, Taubenberger (MPA Garching), Fiore, Benetti, Cappellaro, Tomasella, Turatto (INAF OAPd) report/s a classification of object: SN 2019bmj
Type: OtherRedshift: 0.0538
Remarks: The Asiago spectrum shows a blue, featureless continuum, from which we derived a black-body temperature of about 14800 K. The redshift is deduced from the position of the narrow emission lines of the host galaxy.
The following Classification spectrum was provided:
Obsdate: 2019-03-06 03:07:30
Instrument: AFOSC
Telescope: Asiago Ekar Telescope
Remarks: The Asiago spectrum shows a blue, featureless continuum, from which we derived a black-body temperature of about 14800 K. The redshift is deduced from the position of the narrow emission lines of the host galaxy.
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2019bmj
Date Received (UTC): 2019-03-06 15:30:37 Sender: Lina Tomasella
Group: Padova-Asiago
Schuldt, Vogl, Taubenberger (MPA Garching), Fiore, Benetti, Cappellaro, Tomasella, Turatto (INAF OAPd) report/s a classification of object: SN 2019bmj
Type: OtherRedshift: 0.0538
Remarks: The Asiago spectrum shows a blue, featureless continuum, from which we derived a black-body temperature of about 14800 K. The redshift is deduced from the position of the narrow emission lines of the host galaxy.
The following Classification spectrum was provided:
Obsdate: 2019-03-06 03:07:30
Instrument: AFOSC
Telescope: Asiago Ekar Telescope
Remarks: The Asiago spectrum shows a blue, featureless continuum, from which we derived a black-body temperature of about 14800 K. The redshift is deduced from the position of the narrow emission lines of the host galaxy.
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2019bmj