Spectroscopic Follow-up of Optical Transients from the Catalina Sky Survey

Details Spectroscopic Follow-up of Optical Transients from the Catalina Sky Survey Spectroscopic Follow-up of Optical Transients from the Catalina Sky Survey

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1416....1d&link_type=abstract

The Astronomer's Telegram, #1416

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2

Optical, Cataclysmic Variables, Novae, Supernovae, Transients, Variables

Scientific paper

Spectra of several optical transients from the Catalina Sky Survey, reported earlier (Drake et al., ATEL #1388, ATEL #1399, ATEL #1404; Glikman et al. ATEL #1413) were obtained at the Palomar 200-inch telescope using the Double Spectrograph instrument, on the nights of UT 2008 March 1, 2, and 3. Their spectroscopic identifications are as follows: CSS080130:021110+171624 = Possible CV: a blue continuum with narrow Balmer emission lines (alpha through epsilon, possibly higher); but no obvious helium or other lines.

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