The 2dF QSO survey is a spectroscopic survey of 48 000 point-sources selected by colour with magnitudes in the range 18.35 <~B <~20.95. Amongst QSOs, white dwarfs, narrow-line galaxies and other objects are some cataclysmic variables. This survey should be sensitive to intrinsically faint CVs. In the standard picture of CV evolution, these form the majority of the CV population. We present the spectra of six CVs from this survey. Four have the spectra of dwarf novae and two are magnetic CVs. We present evidence that suggests that the dwarf novae have periods P < 2h and are indeed intrinsically less luminous than average. However, it is not clear yet whether these systems are present in the large numbers predicted
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Os...
The spatial distribution, galactic model parameters and luminosity function of cataclysmic variables...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...
The 2dF QSO survey is a spectroscopic survey of 48,000 point-sources selected by colour with magnitu...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
This thesis explores the cataclysmic variables (CVs) found by the Palomar-Green (PG) survey. This is...
We discuss the properties of 137 cataclysmic variables (CVs) which are included in the Sloan Digital...
The commissioning year of the Sloan Digital Sky Survey has demonstrated that many cataclysmic variab...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
Strong selection effects are present in observational samples of cataclysmic variables (CVs), compli...
Over six years of operation, the Catalina Real-time Transient Survey (CRTS) has identified 1043 cata...
The Sloan Digital Sky Survey has identified a total of 212 cataclysmic variables, most of which are ...
This paper completes the series of cataclysmic variables (CVs) identified from the Sloan Digital Sky...
Cataclysmic Variables (CV) are binary systems where a main-sequence star transfers mass onto a white...
We present 855 cataclysmic variable candidates detected by the Catalina Real-time Transient Survey (...
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Os...
The spatial distribution, galactic model parameters and luminosity function of cataclysmic variables...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...
The 2dF QSO survey is a spectroscopic survey of 48,000 point-sources selected by colour with magnitu...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
This thesis explores the cataclysmic variables (CVs) found by the Palomar-Green (PG) survey. This is...
We discuss the properties of 137 cataclysmic variables (CVs) which are included in the Sloan Digital...
The commissioning year of the Sloan Digital Sky Survey has demonstrated that many cataclysmic variab...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
Strong selection effects are present in observational samples of cataclysmic variables (CVs), compli...
Over six years of operation, the Catalina Real-time Transient Survey (CRTS) has identified 1043 cata...
The Sloan Digital Sky Survey has identified a total of 212 cataclysmic variables, most of which are ...
This paper completes the series of cataclysmic variables (CVs) identified from the Sloan Digital Sky...
Cataclysmic Variables (CV) are binary systems where a main-sequence star transfers mass onto a white...
We present 855 cataclysmic variable candidates detected by the Catalina Real-time Transient Survey (...
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Os...
The spatial distribution, galactic model parameters and luminosity function of cataclysmic variables...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...