TNS Classification Report No. 995 [ 2017TNSCR.536....1H ]
Date Received (UTC): 2017-05-09 20:13:41 Sender: Griffin Hosseinzadeh
Group: Global SN Project
Griffin Hosseinzadeh, D. Andrew Howell, Iair Arcavi, Curtis McCully, Stefano Valenti report/s a classification of object: SN 2017csc
Type: SN Ib/cRedshift: 0.03
Remarks: Using Superfit (Howell et al. 2005, ApJ, 634, 1190), we find good fits to several Type Ib/c supernovae, including some Type Ic-BL supernovae, after maximum light at redshifts around z=0.03. This redshift implies that the potential host galaxy is very faint (M_g ~ -13 mag; SDSS DR13). Follow-up photometry from Las Cumbres Observatory's network of 1-meter telescopes shows that maximum light occurred around 2017 April 10.
The following Classification spectrum was provided:
Obsdate: 2017-05-04 11:13:20
Instrument: FLOYDS-N
Telescope: Faulkes Telescope North
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2017csc
Date Received (UTC): 2017-05-09 20:13:41 Sender: Griffin Hosseinzadeh
Group: Global SN Project
Griffin Hosseinzadeh, D. Andrew Howell, Iair Arcavi, Curtis McCully, Stefano Valenti report/s a classification of object: SN 2017csc
Type: SN Ib/cRedshift: 0.03
Remarks: Using Superfit (Howell et al. 2005, ApJ, 634, 1190), we find good fits to several Type Ib/c supernovae, including some Type Ic-BL supernovae, after maximum light at redshifts around z=0.03. This redshift implies that the potential host galaxy is very faint (M_g ~ -13 mag; SDSS DR13). Follow-up photometry from Las Cumbres Observatory's network of 1-meter telescopes shows that maximum light occurred around 2017 April 10.
The following Classification spectrum was provided:
Obsdate: 2017-05-04 11:13:20
Instrument: FLOYDS-N
Telescope: Faulkes Telescope North
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2017csc