This thesis investigates the characteristics of the Blazhko effect using data from the SuperWASP archive. The SuperWASP instrument combines wide-field coverage with a short cadence, providing time-series analysis on a range of timescales for a large number of stars. The Blazhko effect is the amplitude and frequency modulation of RR Lyrae variable pulsating stars. Its physical causes are still unexplained by stellar structure and evolution models. The stellar pulsation mechanism and modulation are introduced before comparing the WASP project to other wide-field surveys. The aim of this research is to identify correlations between the basic pulsation and Blazhko effect characteristics that may provide clues to its origins. To accomplish th...
The purpose of this thesis was to create an automated classifier for periodic stellar objects in the...
We present the first paper of a series focused on the Blazhko effect in RR Lyrae type stars pulsatin...
We briefly review the results obtained by using the times of maximum brightness of RR Lyrae variable...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and identify ...
Almost a century after its discovery the Blazhko effect in RR Lyrae stars remains a mystery. The Bla...
Almost a century after its discovery, the phenomenon of amplitude and/or phase modulation, observed ...
The unprecedented photometric precision along with the quasi-continuous sampling provided by the Kep...
To date, about 40 known RR Lyrae stars are located in the Kepler field. The outstandingly high-preci...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
Cette thèse propose une nouvelle théorie de l’effet Blazhko. Elle apporte également une justificatio...
The All Sky Automated Survey (ASAS) monitors bright stars (8 mag < V < 14 mag) south of declination ...
The purpose of this thesis was to create an automated classifier for periodic stellar objects in the...
We present the first paper of a series focused on the Blazhko effect in RR Lyrae type stars pulsatin...
We briefly review the results obtained by using the times of maximum brightness of RR Lyrae variable...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and identify ...
Almost a century after its discovery the Blazhko effect in RR Lyrae stars remains a mystery. The Bla...
Almost a century after its discovery, the phenomenon of amplitude and/or phase modulation, observed ...
The unprecedented photometric precision along with the quasi-continuous sampling provided by the Kep...
To date, about 40 known RR Lyrae stars are located in the Kepler field. The outstandingly high-preci...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
Cette thèse propose une nouvelle théorie de l’effet Blazhko. Elle apporte également une justificatio...
The All Sky Automated Survey (ASAS) monitors bright stars (8 mag < V < 14 mag) south of declination ...
The purpose of this thesis was to create an automated classifier for periodic stellar objects in the...
We present the first paper of a series focused on the Blazhko effect in RR Lyrae type stars pulsatin...
We briefly review the results obtained by using the times of maximum brightness of RR Lyrae variable...