GCN Circular 18371

I.A Steele, C.M. Copperwheat, A.S. Piascik (Liverpool JMU)
report on behalf of the larger ARI-LJMU collaboration

In further analysis of the LT spectrum reported in GCN 18370
Not found
 
 
 of PS15ccx
we have now succeeded in obtaining a classification of the spectrum
using SNID by truncating the wavelength range to between 4500 and
7500 Angstroms to remove the regions of poorest signal to noise ratio.

SNID reports a 96% probability that the transient is a Supernova Type Ia
at age 15-23 days post maximum with z~0.097.



________________________________
Important Notice: the information in this email and any attachments is for the sole use of the intended recipient(s). If you are not an intended recipient, or a person responsible for delivering it to an intended recipient, you should delete it from your system immediately without disclosing its contents elsewhere and advise the sender by returning the email or by telephoning a number contained in the body of the email. No responsibility is accepted for loss or damage arising from viruses or changes made to this message after it was sent. The views contained in this email are those of the author and not necessarily those of Liverpool John Moores University.