|
|
|
|
LEADER |
02317 am a22002533u 4500 |
001 |
124729 |
042 |
|
|
|a dc
|
100 |
1 |
0 |
|a Huang, Chelsea
|e author
|
100 |
1 |
0 |
|a MIT Kavli Institute for Astrophysics and Space Research
|e contributor
|
700 |
1 |
0 |
|a Shporer, Avi
|e author
|
700 |
1 |
0 |
|a Ricker, George R.
|e author
|
700 |
1 |
0 |
|a Vanderspek, Roland K.
|e author
|
700 |
1 |
0 |
|a Seager, Sara
|e author
|
700 |
1 |
0 |
|a Goeke, Robert F.
|e author
|
700 |
1 |
0 |
|a Guerrero, Natalia
|e author
|
700 |
1 |
0 |
|a Villanueva, Steven
|e author
|
245 |
0 |
0 |
|a Two new HATNet hot Jupiters around A stars and the first glimpse at the occurrence rate of hot Jupiters from TESS
|
260 |
|
|
|b American Astronomical Society,
|c 2020-04-17T17:58:49Z.
|
856 |
|
|
|z Get fulltext
|u https://hdl.handle.net/1721.1/124729
|
520 |
|
|
|a Wide-field surveys for transiting planets are well suited to searching diverse stellar populations, enabling a better understanding of the link between the properties of planets and their parent stars. We report the discovery of HAT-P-69 b (TOI 625.01) and HAT-P-70 b (TOI 624.01), two new hot Jupiters around A stars from the Hungarian-made Automated Telescope Network (HATNet) survey that have also been observed by the Transiting Exoplanet Survey Satellite. HAT-P-69 b has a mass of M Jup and a radius of $ R Jup and resides in a prograde 4.79 day orbit. HAT-P-70 b has a radius of R Jup and a mass constraint of M Jup and resides in a retrograde 2.74 day orbit. We use the confirmation of these planets around relatively massive stars as an opportunity to explore the occurrence rate of hot Jupiters as a function of stellar mass. We define a sample of 47,126 main-sequence stars brighter than T mag = 10 that yields 31 giant planet candidates, including 18 confirmed planets, 3 candidates, and 10 false positives. We find a net hot Jupiter occurrence rate of 0.41 0.10% within this sample, consistent with the rate measured by Kepler for FGK stars. When divided into stellar mass bins, we find the occurrence rate to be 0.71 0.31% for G stars, 0.43 0.15% for F stars, and 0.26 0.11% for A stars. Thus, at this point, we cannot discern any statistically significant trend in the occurrence of hot Jupiters with stellar mass. ©2019
|
546 |
|
|
|a en
|
655 |
7 |
|
|a Article
|
773 |
|
|
|t 10.3847/1538-3881/AB36B5
|
773 |
|
|
|t Astronomical journal
|