Skip to content Skip to navigation
University of Warwick
  • Study
  • |
  • Research
  • |
  • Business
  • |
  • Alumni
  • |
  • News
  • |
  • About

University of Warwick
Publications service & WRAP

Highlight your research

  • WRAP
    • Home
    • Search WRAP
    • Browse by Warwick Author
    • Browse WRAP by Year
    • Browse WRAP by Subject
    • Browse WRAP by Department
    • Browse WRAP by Funder
    • Browse Theses by Department
  • Publications Service
    • Home
    • Search Publications Service
    • Browse by Warwick Author
    • Browse Publications service by Year
    • Browse Publications service by Subject
    • Browse Publications service by Department
    • Browse Publications service by Funder
  • Help & Advice
University of Warwick

The Library

  • Login
  • Admin

SuperWASP lightcurves of subdwarf stars

Tools
- Tools
+ Tools

Maxted, P. F. L., Norton, Andrew J., West, Richard G., Copperwheat, C. M. and Marsh, T. R. (2008) SuperWASP lightcurves of subdwarf stars. In: Hot Subdwarf Stars and Related Objects ASP Conference Series, Otto-Friedrich-Universität, Bamberg, Germany, 23-27 Jul 2007. Published in: Hot Subdwarf Stars and Related Objects ASP Conference Series, Vol.392

Research output not available from this repository.

Request-a-Copy directly from author or use local Library Get it For Me service.

Official URL: http://ukads.nottingham.ac.uk/abs/2008ASPC..392..1...

Request Changes to record.

Abstract

SuperWASP is a wide angle survey for transiting hot-Jupiter exoplanets around bright (V<13) solar-type stars. Lightcurves for millions of stars with a few thousand observations per star are available in the SuperWASP archive. We report the results of a search for periodic variable subdwarf stars in the data from the 2004 observing season. A Fourier transform of the SuperWASP lightcurve for Balloon 090100001 recovers the main pulsation frequency of this star. No new pulsators are found among the stars studied (about 200 objects). The binary sdB star HS 2333+3927 with a large reflection effect was recovered. We find that the hot subdwarf PG 1348+369 is variable with a period of 3.316days and a semi-amplitude of 13%. Follow-up spectroscopy shows that this variation is due to irradiation of a cool companion star in a binary system.

Item Type: Conference Item (Paper)
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
Library of Congress Subject Headings (LCSH): Dwarf stars
Journal or Publication Title: Hot Subdwarf Stars and Related Objects ASP Conference Series
Official Date: 2008
Dates:
DateEvent
2008Published
Volume: Vol.392
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Description:

Proceedings of the conference held 23-27 July, 2007

Conference Paper Type: Paper
Title of Event: Hot Subdwarf Stars and Related Objects ASP Conference Series
Type of Event: Conference
Location of Event: Otto-Friedrich-Universität, Bamberg, Germany
Date(s) of Event: 23-27 Jul 2007

Request changes or add full text files to a record

Repository staff actions (login required)

View Item View Item
twitter

Email us: wrap@warwick.ac.uk
Contact Details
About Us