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arXiv · 1407.3315

Followup Observations of SDSS and CRTS Candidate Cataclysmic Variables

Paula Szkody·Mark E. Everett·Steve B. Howell·Arlo U. Landolt·Howard E. Bond·David R. Silva·Stephanie Vasquez-Soltero
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Abstract

We present photometry of 11 and spectroscopy of 35 potential cataclysmic variables from the Sloan Digital Sky Survey, the Catalina Real-Time Transient Survey and vsnet-alerts. The photometry results include quasi-periodic oscillations during the decline of V1363 Cyg, nightly accretion changes in the likely Polar (AM Herculis binary) SDSS J1344+20, eclipses in SDSS J2141+05 with an orbital period of 76+/-2 min, and possible eclipses in SDSS J2158+09 at an orbital period near 100 min. Time-resolved spectra reveal short orbital periods near 80 min for SDSS J0206+20, 85 min for SDSS J1502+33, and near 100 min for CSS J0015+26, RXS J0150+37, SDSS J1132+62, SDSS J2154+15 and SDSS J2158+09. The prominent HeII line and velocity amplitude of SDSS J2154+15 are consistent with a Polar nature for this object, while the lack of this line and a low velocity amplitude argue against this classification for RXS J0150+37. Single spectra of 10 objects were obtained near outburst and the rest near quiescence, confirming the dwarf novae nature of these objects.

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Paula Szkody, Mark E. Everett, Steve B. Howell, Arlo U. Landolt, Howard E. Bond, David R. Silva, Stephanie Vasquez-Soltero. 2014-07-11. Followup Observations of SDSS and CRTS Candidate Cataclysmic Variables. https://doi.org/10.1088/0004-6256%2F148%2F4%2F63

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