SuperWASP-N extrasolar planet candidates from fields 06h

S.R. Kane, W.I. Clarkson, R.G. West, D.M. Wilson, Damian Christian, A. Collier-Cameron, B. Enoch, T.A. Lister, R.A. Street, A. Evans, Alan Fitzsimmons, C.A. Haswell, C. Hellier, S.T. Hodgkin, K. Horne, J. Irwin, Francis Keenan, A.J. Norton, J. Osborne, N.R. ParleyDon Pollacco, Robert Ryans, I. Skillen, P.J. Wheatley

Research output: Contribution to journalArticlepeer-review

11 Citations (Scopus)
127 Downloads (Pure)

Abstract

TheWide Angle Search for Planets (WASP) survey currently operates two installations, designated SuperWASP-N and SuperWASP-S, located in the Northern and Southern hemispheres, respectively. These installations are designed to provide high time-resolution photometry for the purpose of detecting transiting extrasolar planets, asteroids, and transient events. Here, we present results from a transit-hunting observing campaign using SuperWASP-N covering a right ascension (RA) range of 06h < RA < 16h. This paper represents the fifth and final in the series of transit candidates released from the 2004 observing season. In total, 729 335 stars from 33 fields were monitored with 130 566 having sufficient precision to be scanned for transit signatures. Using a robust transit detection algorithm and selection criteria, six stars were found to have events consistent with the signature of a transiting extrasolar planet based on the photometry, including the known transiting planet XO-1b. These transit candidates are presented here along with discussion of follow-up observations and the expected number of candidates in relation to the overall observing strategy.
Original languageEnglish
Pages (from-to)1097-1108
JournalMonthly Notices of the Royal Astronomical Society
Volume384
DOIs
Publication statusPublished - Mar 2008

ASJC Scopus subject areas

  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'SuperWASP-N extrasolar planet candidates from fields 06h'. Together they form a unique fingerprint.

Cite this