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starplanet [2017/06/07 10:38] Gracjan Maciejewski |
starplanet [2017/06/07 10:50] Gracjan Maciejewski |
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| WASP-12 b | 1.0914 | 06 30 33 | +29 40 20 | 11.6 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=WASP-12&PLANET=b|ETD]] | only high quality data | | | WASP-12 b | 1.0914 | 06 30 33 | +29 40 20 | 11.6 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=WASP-12&PLANET=b|ETD]] | only high quality data | | ||
| WASP-103 b | 0.9255 | 16 37 15 | +07 11 00 | 12.1 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=WASP-103&PLANET=b|ETD]] | ongoing since 2017 | | | WASP-103 b | 0.9255 | 16 37 15 | +07 11 00 | 12.1 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=WASP-103&PLANET=b|ETD]] | ongoing since 2017 | | ||
- | | HAT-23 b | 1.2128 | 20 24 29 | +16 45 44 | 12.4 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=HAT-P-23&PLANET=b|ETD]] | ongoing since 2017 | | + | | HAT-P-23 b | 1.2128 | 20 24 29 | +16 45 44 | 12.4 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=HAT-P-23&PLANET=b|ETD]] | ongoing since 2017 | |
| KELT-16 b | 0.9690 | 20 57 04 | +31 39 40 | 10.9 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=KELT-16&PLANET=b|ETD]] | ongoing since 2017 | | | KELT-16 b | 0.9690 | 20 57 04 | +31 39 40 | 10.9 | [[http://var2.astro.cz/ETD/predict_detail.php?STARNAME=KELT-16&PLANET=b|ETD]] | ongoing since 2017 | | ||
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=== RESULTS === | === RESULTS === | ||
- | //WASP-12 b//: We have detected the apparent shortening of the orbital period that could be caused by orbital decay or apsidal precession ([[http://adsabs.harvard.edu/abs/2016A%26A...588L...6M|Maciejewski et al. 2016]]). New observations are needed to track apparent orbital decay of WASP-12 b. | + | //WASP-12 b//: We have detected the apparent shortening of the orbital period that could be caused by orbital decay or apsidal precession ([[http://adsabs.harvard.edu/abs/2016A%26A...588L...6M|Maciejewski et al. 2016]]). New observations are needed to follow the TTV signal. |
//Remaining targets//: Lower constraints on the values of stellar //Q'// will be determined using observations acquired by the end of 2017. Those initial results will be published in an introduction paper in early 2018. | //Remaining targets//: Lower constraints on the values of stellar //Q'// will be determined using observations acquired by the end of 2017. Those initial results will be published in an introduction paper in early 2018. |