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High-speed photometry of faint cataclysmic variables - IX. Targets from multiple transient surveys
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High-speed photometry of faint cataclysmic variables - IX. Targets from multiple transient surveys
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We present high-speed photometric observations of 25 cataclysmic variables detected by the All Sky Automated Search for Super-Novae (ASAS-SN), the Mobile Astronomical System of the TElescope-Robot (MASTER) and the Catalina Real-Time Transient Survey (CRTS). From these observations we determine 16 new orbital periods and 1 new superhump period. Two systems (ASASSN-14ik and ASASSN-14ka) have outburst periods of approximately 1 month, with a third (ASASSN-14hv) having outbursts approximately every 2 months. Included in the sample are 11 eclipsing systems, one probable intermediate polar (ASASSN-15fm), 1 SW Sex-type star (MLS 0720+17), 1 WZ Sge-type star (ASASSN-17fz) and one system showing different photometric and spectroscopic periods (ASASSN-15kw).
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Cited by 1 Pith paper
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1000 cataclysmic variables identified from DESI spectroscopy
1,029 cataclysmic variables (221 new) were identified from 98.97 million DESI spectra using a CNN trained on SDSS CVs.
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