Presentation
The program started in 2011 with the aim to classify all transients that are accessible from Asiago and are bright enough for our telescope/instrumentation. We use mainly the 1.82m Copernico telescope of Cima Ekar and, if not available, the 1.22m Galileo telescope of the Pennar station. A few cases of transients classified by our group with other facilities (eg. TNG) are included in the database.
Transient classification information and spectra (fits format) are made immediately available at our site. The spectra are semi-automatic reduction with archive calibration data. Please keep this in mind when using them.
For SN classification we compare the output of two automatic SN classification codes: Gelato (Harutyunyan et al. 2008, A&A 488, 383) and SNID (Blondin and Tonry 2007, Ap.J. 666, 1024).
If you use some of the information posted in these pages please make a reference to the paper Tomasella etal. 2014, A.N. 335, 841.

sn	galaxy	RA	DEC	discoverer	type	redshift	ref	class	fits
2020lhs	WISEA J202302.62+212	20:23:02.310	+21:23:48.59	ASASSN	CV	0	REF		fits
2020hhg		17:24:22.610	+42:40:08.19	ZTF	CV		ATEL		fits
2020gpe	NGC6214	16:39:32.19	+66:02:14.01	ISSP	II	0.025414	ATEL		fits
2020fkb	Arp 299	11:28:30.436	+58:33:46.78	ALeRCE ZTF	Ib	0.010	ATEL		fits
2020euy	WISEA J133629.46+473	13:36:29.482	+47:34:26.35	ASASSN	Ic	0.062312	ATEL		fits