Spectroscopy of CSS transients and variables

Details Spectroscopy of CSS transients and variables Spectroscopy of CSS transients and variables

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1520....1m&link_type=abstract

The Astronomer's Telegram, #1520

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2

Optical, Novae, Quasars, Supernovae, Transients, Variables

Scientific paper

Spectra of several optical transients and variables from the Catalina Sky Survey were obtained at the Palomar 200-inch telescope using the Double Beam Spectrograph, on the nights of UT 2008 May 5, 6, and 7. The transients were all published in real-time on the VOEventNet pages at www.voeventnet.org. The other candidates were chosen based on their variability. Their spectroscopic identifications are as follows: CSS080409:154159+235603 = possible blazar, blue continuum with a possible broad line at ~ 5530A; if this is Mg II 2799, then z ~ 0.98.

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