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 |