TY - JOUR
T1 - Cataclysmic variables from the Sloan Digital Sky Survey. III. The third year
AU - Szkody, Paula
AU - Henden, Arne
AU - Fraser, Oliver
AU - Silvestri, Nicole
AU - Bochanski, John
AU - Wolfe, Michael A.
AU - Agüeros, Marcel
AU - Warner, Brian
AU - Woudt, Patrick
AU - Tramposch, Jonica
AU - Homer, Lee
AU - Schmidt, Gary
AU - Knapp, Gillian R.
AU - Anderson, Scott F.
AU - Covey, Kevin
AU - Harris, Hugh
AU - Hawley, Suzanne
AU - Schneider, Donald P.
AU - Voges, Wolfgang
AU - Brinkmann, J.
PY - 2004/10
Y1 - 2004/10
N2 - This paper continues the series that identifies new cataclysmic variables found in the Sloan Digital Sky Survey (SDSS). We present 36 cataclysmic variables and one possible symbiotic star from Sloan spectra obtained during 2002, of which 34 are new discoveries, two are known dwarf novae (BC UMa and KS UMa), and one is a known cataclysmic variable identified from the Two-Degree Field survey. The positions, colors, and spectra of all 37 systems are presented, along with follow-up spectroscopic/photometric observations of 10 systems. As in the past 2 yr of data, the new SDSS systems show a large variety of characteristics based on their inclination and magnetic fields, including three eclipsing systems, four with prominent He n emission, and 15 systems showing features of the underlying stars.
AB - This paper continues the series that identifies new cataclysmic variables found in the Sloan Digital Sky Survey (SDSS). We present 36 cataclysmic variables and one possible symbiotic star from Sloan spectra obtained during 2002, of which 34 are new discoveries, two are known dwarf novae (BC UMa and KS UMa), and one is a known cataclysmic variable identified from the Two-Degree Field survey. The positions, colors, and spectra of all 37 systems are presented, along with follow-up spectroscopic/photometric observations of 10 systems. As in the past 2 yr of data, the new SDSS systems show a large variety of characteristics based on their inclination and magnetic fields, including three eclipsing systems, four with prominent He n emission, and 15 systems showing features of the underlying stars.
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U2 - 10.1086/423997
DO - 10.1086/423997
M3 - Article
AN - SCOPUS:9344232734
SN - 0004-6256
VL - 128
SP - 1882
EP - 1893
JO - Astronomical Journal
JF - Astronomical Journal
IS - 4
ER -