We present the results of a survey using the WASP archive to search for high-frequency pulsations in F-, A- and B-type stars. Over 1.5 million targets have been searched for pulsations with amplitudes greater than 0.5 millimagnitude. We identify over 350 stars which pulsate with periods less than 30 min. Spectroscopic follow-up of selected targets has enabled us to confirm 10 new rapidly oscillating Ap stars, 13 pulsating Am stars and the fastest known δ Scuti star. We also observe stars which show pulsations in both the high-frequency domain and the low-frequency δ Scuti range. This work shows the power of the WASP photometric survey to find variable stars with amplitudes well below the nominal photometric precision per observation.Publish...
We present follow-up observations of the pulsating subdwarf B (sdB) star EC 01541–1409 as part of ou...
SuperWASP is the world's leading ground-based survey for transiting exoplanets. Its database now con...
A new survey for pulsating, chemically peculiar A- and F-type stars in the northern hemisphere has b...
peer reviewedWe present the results of a survey using the WASP archive to search for high-frequency ...
We present the results of a survey using the WASP archive to search for high-frequency pulsations in...
The searches for transiting exoplanets have produced a vast amount of time-resolved photometric data...
A survey of A-type stars is conducted with the SuperWASP archive in the search for pulsationally var...
We have studied over 1600 Am stars at a photometric precision of 1 mmag with SuperWASP photometric d...
The highly successful SuperWASP planetary transit finding programme has surveyed a large fraction of...
SuperWASP is a wide angle survey for transiting hot-Jupiter exoplanets around bright (V<13) solar-ty...
The WASP project is funded and operated by Queen’s University Belfast, the Universities of Keele, St...
We have analysed around 170 000 individual photometric WASP (Wide Angle Search for Planets) measurem...
We have analysed around 170 000 individual photometric WASP (Wide Angle Search for Planets) measurem...
SuperWASP is one of the largest ground-based surveys for transiting exoplanets. To date, it has obse...
We present follow-up observations of the pulsating subdwarf B (sdB) star EC 01541–1409 as part of ou...
SuperWASP is the world's leading ground-based survey for transiting exoplanets. Its database now con...
A new survey for pulsating, chemically peculiar A- and F-type stars in the northern hemisphere has b...
peer reviewedWe present the results of a survey using the WASP archive to search for high-frequency ...
We present the results of a survey using the WASP archive to search for high-frequency pulsations in...
The searches for transiting exoplanets have produced a vast amount of time-resolved photometric data...
A survey of A-type stars is conducted with the SuperWASP archive in the search for pulsationally var...
We have studied over 1600 Am stars at a photometric precision of 1 mmag with SuperWASP photometric d...
The highly successful SuperWASP planetary transit finding programme has surveyed a large fraction of...
SuperWASP is a wide angle survey for transiting hot-Jupiter exoplanets around bright (V<13) solar-ty...
The WASP project is funded and operated by Queen’s University Belfast, the Universities of Keele, St...
We have analysed around 170 000 individual photometric WASP (Wide Angle Search for Planets) measurem...
We have analysed around 170 000 individual photometric WASP (Wide Angle Search for Planets) measurem...
SuperWASP is one of the largest ground-based surveys for transiting exoplanets. To date, it has obse...
We present follow-up observations of the pulsating subdwarf B (sdB) star EC 01541–1409 as part of ou...
SuperWASP is the world's leading ground-based survey for transiting exoplanets. Its database now con...
A new survey for pulsating, chemically peculiar A- and F-type stars in the northern hemisphere has b...