The discovery of 1502 + 09, an emission-line star of magnitude 18.56 + or - 0.1 mag, on a IIIa-J plate obtained in a 60-min exposure using a 44-arcmin low-dispersion objective prism on the 1.2-m UK Schmidt telescope is reported. A finding chart, the objective-prism spectrum, and a 1-nm-resolution 330-610-nm spectrum obtained with the intensified Reticon spectrometer on the 5-m Hale telescope at Palomar Observatory are presented and characterized. The object is classified as a dwarf-nova cataclysmic variable of U Gem type lying at a distance of about 350 pc and about 280 pc above the Galactic plane; i.e., considerably farther than the 150-pc density scale height derived for dwarf novae by Patterson (1984).
N. Elias–Rosa, Schuyler D. Van Dyk, S. Benetti, E. Cappellaro, Nathan Smith, R. Kotak, M. Turatto, Alexei V Filippenko, G. Pignata, Ori D. Fox, L. Galbany, S. González–Gaitán, M Miluzio, L. A. G. Monard, M. Ergon
Manuel Boix-Chornet, Mario F. Fraga, Ana Villar‐Garea, Rosalía Caballero, Jesús Espada, Antonio Núñez, Juan Casado‐Vela, Cristina Largo, J. Ignacio Casal, Juan C. Cigudosa, Luís Franco, Manel Esteller, Esteban Ballestar
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