The HATSouth survey has discovered 61 exoplanets to date. The table below lists these planets, along with links to papers describing their discovery, as well as some of their fundamental properties. HATSouth discovery light curves for each planet are available. In most cases, data from follow-up photometric and spectroscopic campaigns are also provided. Click on any table column header to sort by that column.
Planet name | Period [days] | Semimajor axis [AU] | Eccentricity | Mass [MJupiter] | Radius [RJupiter] | Discovery paper |
---|---|---|---|---|---|---|
HATS-70b | 1.8882378 | 0.03632 | < 0.18 | 12.9 | 1.384 | Zhou+ 2018 |
HATS-69b | 2.2252577 | 0.03211 | < 0.013 | < 0.577 | 0.945 | Hartman+ 2018 |
HATS-68b | 3.5862234 | 0.05053 | < 0.005 | 1.286 | 1.284 | Hartman+ 2018 |
HATS-67b | 1.6091789 | 0.03036 | < 0.014 | 1.477 | 1.694 | Hartman+ 2018 |
HATS-66b | 3.141439 | 0.04709 | < 0.008 | 5.5 | 1.50 | Hartman+ 2018 |
HATS-65b | 3.1051602 | 0.04511 | < 0.006 | 0.793 | 1.479 | Hartman+ 2018 |
HATS-64b | 4.908896 | 0.06560 | < 0.001 | 0.93 | 1.674 | Hartman+ 2018 |
HATS-63b | 3.0566528 | 0.04026 | < 0.007 | 0.96 | 1.207 | Hartman+ 2018 |
HATS-62b | 3.2768838 | 0.04186 | < 0.001 | < 0.191 | 1.032 | Hartman+ 2018 |
HATS-61b | 7.817954 | 0.07904 | < 0.008 | 3.40 | 1.201 | Hartman+ 2018 |
HATS-60b | 3.560827 | 0.04710 | < 0.040 | 0.650 | 1.194 | Hartman+ 2018 |
HATS-59c | 1422 | 2.504 | < 0.083 | > 12.70 | Unavailable | Sarkis+ 2018 |
HATS-59b | 5.416081 | 0.06112 | 0.129 | 0.806 | 1.126 | Sarkis+ 2018 |
HATS-53b | 3.85378 | 0.04753 | < 0.330 | 0.595 | 1.340 | Henning+ 2017 |
HATS-52b | 1.36665 | 0.02498 | < 0.246 | 2.24 | 1.382 | Henning+ 2017 |
HATS-51b | 3.34887 | 0.04639 | < 0.330 | 0.768 | 1.41 | Henning+ 2017 |
HATS-50b | 3.82970 | 0.05046 | < 0.516 | 0.39 | 1.130 | Henning+ 2017 |
HATS-46b | 4.74237 | 0.05367 | < 0.559 | 0.173 | 0.903 | Brahm+ 2017 |
HATS-45b | 4.18762 | 0.05511 | < 0.240 | 0.70 | 1.286 | Brahm+ 2017 |
HATS-44b | 2.74390 | 0.03649 | < 0.279 | 0.56 | 1.067 | Brahm+ 2017 |
HATS-43b | 4.38888 | 0.04944 | 0.173 | 0.261 | 1.180 | Brahm+ 2017 |
HATS-42b | 2.29210 | 0.03689 | < 0.229 | 1.88 | 1.40 | Bento+ 2018 |
HATS-41b | 4.19365 | 0.0583 | 0.38 | 9.7 | 1.33 | Bento+ 2018 |
HATS-40b | 3.26427 | 0.04997 | < 0.312 | 1.59 | 1.58 | Bento+ 2018 |
HATS-39b | 4.57763 | 0.06007 | < 0.275 | 0.63 | 1.57 | Bento+ 2018 |
HATS-36b = EPIC 215969174b | 4.17524 | 0.0529 | < 0.294 | 2.79 | 1.263 | Bayliss+ 2017 |
HATS-35b | 1.82099 | 0.0319 | < 0.306 | 1.222 | 1.464 | de Val-Borro+ 2016 |
HATS-34b | 2.10616 | 0.0317 | < 0.108 | 0.941 | 1.43 | de Val-Borro+ 2016 |
HATS-33b | 2.54955 | 0.0373 | < 0.080 | 1.192 | 1.230 | de Val-Borro+ 2016 |
HATS-32b | 2.81265 | 0.0402 | < 0.471 | 0.92 | 1.249 | de Val-Borro+ 2016 |
HATS-31b | 3.37796 | 0.0478 | < 0.233 | 0.88 | 1.64 | de Val-Borro+ 2016 |
HATS-30b | 3.17435 | 0.04354 | < 0.096 | 0.706 | 1.175 | Espinoza+ 2016 |
HATS-29b | 4.60587 | 0.0548 | < 0.158 | 0.653 | 1.251 | Espinoza+ 2016 |
HATS-28b | 3.18108 | 0.0413 | < 0.202 | 0.672 | 1.194 | Espinoza+ 2016 |
HATS-27b | 4.63704 | 0.0611 | < 0.581 | 0.53 | 1.50 | Espinoza+ 2016 |
HATS-26b | 3.30238 | 0.0474 | < 0.245 | 0.650 | 1.75 | Espinoza+ 2016 |
HATS-25b | 4.29864 | 0.0516 | < 0.176 | 0.613 | 1.26 | Espinoza+ 2016 |
HATS-24b | 1.34849 | 0.0255 | < 0.242 | 2.44 | 1.487 | Bento+ 2016 |
HATS-23b | 2.16052 | 0.0339 | < 0.114 | 1.470 | 1.86 | Bento+ 2016 |
HATS-22b | 4.72281 | 0.0503 | 0.079 | 2.74 | 0.953 | Bento+ 2016 |
HATS-21b | 3.55440 | 0.0468 | < 0.149 | 0.332 | 1.123 | Bhatti+ 2016 |
HATS-20b | 3.79930 | 0.0462 | < 0.501 | 0.273 | 0.776 | Bhatti+ 2016 |
HATS-19b | 4.56967 | 0.0589 | 0.30 | 0.427 | 1.66 | Bhatti+ 2016 |
HATS-18b | 0.83784 | 0.0176 | < 0.166 | 1.980 | 1.337 | Penev+ 2016 |
HATS-17b | 16.25461 | 0.1308 | 0.029 | 1.338 | 0.777 | Brahm+ 2015 |
HATS-16b | 2.68650 | 0.03744 | 0.0 (fixed) | 3.27 | 1.30 | Ciceri+ 2015 |
HATS-15b | 1.74749 | 0.02712 | < 0.126 | 2.17 | 1.105 | Ciceri+ 2015 |
HATS-14b | 2.76676 | 0.03815 | < 0.142 | 1.071 | 1.039 | Mancini+ 2015 |
HATS-13b | 3.04405 | 0.04057 | < 0.181 | 0.543 | 1.212 | Mancini+ 2015 |
HATS-12b = EPIC 218131080b | 3.14283 | 0.04795 | < 0.085 | 2.38 | 1.35 | Rabus+ 2016 |
HATS-11b = EPIC 216414930b | 3.61916 | 0.04614 | < 0.340 | 0.85 | 1.510 | Rabus+ 2016 |
HATS-10b | 3.31285 | 0.04491 | < 0.501 | 0.526 | 0.969 | Brahm+ 2015 |
HATS-9b = EPIC 217671466b | 1.91531 | 0.03048 | < 0.129 | 0.837 | 1.065 | Brahm+ 2015 |
HATS-8b | 3.58389 | 0.04667 | < 0.376 | 0.138 | 0.873 | Bayliss+ 2015 |
HATS-7b | 3.18532 | 0.04012 | < 0.170 | 0.120 | 0.563 | Bakos+ 2015 |
HATS-6b | 3.32527 | 0.03621 | 0 (fixed) | 0.333 | 1.000 | Hartman+ 2014 |
HATS-5b | 4.76339 | 0.0542 | 0.019 | 0.237 | 0.912 | Zhou+ 2014 |
HATS-4b | 2.51673 | 0.0362 | 0.013 | 1.323 | 1.020 | Jordan+ 2014 |
HATS-3b | 3.54785 | 0.0485 | 0 (fixed) | 1.071 | 1.381 | Bayliss+ 2013 |
HATS-2b | 1.35413 | 0.0230 | 0 (fixed) | 1.345 | 1.168 | Mohler-Fischer+ 2013 |
HATS-1b | 3.44646 | 0.0444 | 0.120 | 1.855 | 1.302 | Penev+ 2013 |