Nova TCP J18385851-0351482, also called Nova Ser 2025, was discovered on Thursday, July 17, in the constellation Serpens Cauda. On Monday night, July 21, and again on Tuesday night, July 22, spectra of the nova were obtained with the 16″ telescope and Alpy 600 spectrograph in the IUSB Observatory. The diagram below shows the two IUSB spectra along with one collected on Sunday, July 20. The large peak at 6563 A wavelength is the “H-alpha” line — light emitted by hot hydrogen atoms. These spectra were collected roughly 24 hours apart, so this H-alpha line grew very rapidly in this period!

Here is a vertically expanded view of the spectrum, which gives a better look at the smaller peaks, many of which correspond to emission of light from singly ionized iron atoms (Fe II).
