SIMBAD references

After posting on the Central Bureau's TOCP, D. D. Balam, Dominion Astrophysical Observatory, National Research Council of Canada (NRCC); M. L. Graham, Las Cumbres Observatory Global Telescope, University of California at Santa Barbara; and E. Y. Hsiao, Lawrence Berkeley Laboratory, report that a spectrogram (range 385-694 nm, resolution 0.3 nm) of TCP J06195996+1926590, obtained on Jan. 10.267 UT with the 1.82-m Plaskett Telescope of the NRCC, exhibits a strong blue continuum showing very broad (FWHM = 4.2 nm at H-beta) Balmer series absorption lines. The H-alpha line appears to be filled in by emission.