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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. 
 
starplanet.txt ยท Last modified: 2017/06/07 10:50 by Gracjan Maciejewski
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