WTS: A near-infrared transit survey
The WFCAM Transit Survey is a transiting planet survey running on the United Kingdom Infrared Telescope targeting M dwarf stars in the near infrared. The survey has been operating since 2007 and gathering photometric time series of about 15000 M dwarf stars brighter than J = 17 mag. We identified an...
Main Authors: | , , , |
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Format: | Article |
Language: | English |
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EDP Sciences
2013-04-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20134701001 |
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author | Hodgkin Simon Kovács Gábor Sipőcz Brigitta Pinfield David |
author_facet | Hodgkin Simon Kovács Gábor Sipőcz Brigitta Pinfield David |
author_sort | Hodgkin Simon |
collection | DOAJ |
description | The WFCAM Transit Survey is a transiting planet survey running on the United Kingdom Infrared Telescope targeting M dwarf stars in the near infrared. The survey has been operating since 2007 and gathering photometric time series of about 15000 M dwarf stars brighter than J = 17 mag. We identified and followed-up planet candidates from the most complete field and found two hot Jupiters around non-M dwarf hosts (WTS-1b & WTS-2b) but found no planets around the M dwarfs. |
first_indexed | 2024-12-14T01:14:53Z |
format | Article |
id | doaj.art-ab900c64aff2408882320dd9fe69bcdd |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-12-14T01:14:53Z |
publishDate | 2013-04-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
spelling | doaj.art-ab900c64aff2408882320dd9fe69bcdd2022-12-21T23:22:37ZengEDP SciencesEPJ Web of Conferences2100-014X2013-04-01470100110.1051/epjconf/20134701001WTS: A near-infrared transit surveyHodgkin SimonKovács GáborSipőcz BrigittaPinfield DavidThe WFCAM Transit Survey is a transiting planet survey running on the United Kingdom Infrared Telescope targeting M dwarf stars in the near infrared. The survey has been operating since 2007 and gathering photometric time series of about 15000 M dwarf stars brighter than J = 17 mag. We identified and followed-up planet candidates from the most complete field and found two hot Jupiters around non-M dwarf hosts (WTS-1b & WTS-2b) but found no planets around the M dwarfs.http://dx.doi.org/10.1051/epjconf/20134701001 |
spellingShingle | Hodgkin Simon Kovács Gábor Sipőcz Brigitta Pinfield David WTS: A near-infrared transit survey EPJ Web of Conferences |
title | WTS: A near-infrared transit survey |
title_full | WTS: A near-infrared transit survey |
title_fullStr | WTS: A near-infrared transit survey |
title_full_unstemmed | WTS: A near-infrared transit survey |
title_short | WTS: A near-infrared transit survey |
title_sort | wts a near infrared transit survey |
url | http://dx.doi.org/10.1051/epjconf/20134701001 |
work_keys_str_mv | AT hodgkinsimon wtsanearinfraredtransitsurvey AT kovacsgabor wtsanearinfraredtransitsurvey AT sipoczbrigitta wtsanearinfraredtransitsurvey AT pinfielddavid wtsanearinfraredtransitsurvey |