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
2022mbc	CGCG 352-013	11:59:57.120	+76:14:23.53	ATLAS	Ic	0.017582	REF		fits
2022myz	NGC4217	12:15:44.591	+47:04:33.96	ZTF	I	0.003429	REF		fits
2022ffg	CGCG093-074	10:13:48.2	+18:07:38.68	Atlas	II	0.012	REF		fits
2022io		08:24:38.400	+54:40:26.16	ATLAS	Ia	0.063219	REF		fits
2022im		07:55:00.120	+42:46:10.39	ATLAS	Ia-91T	0.067683	REF		fits