| Autor: |
Judah Van Zandt, Erik A. Petigura, Mason MacDougall, Gregory J. Gilbert, Jack Lubin, Thomas Barclay, Natalie M. Batalha, Ian J. M. Crossfield, Courtney Dressing, Benjamin Fulton, Andrew W. Howard, Daniel Huber, Howard Isaacson, Stephen R. Kane, Paul Robertson, Arpita Roy, Lauren M. Weiss, Aida Behmard, Corey Beard, Ashley Chontos, Fei Dai, Paul A. Dalba, Tara Fetherolf, Steven Giacalone, Christopher E. Henze, Michelle L. Hill, Lea A. Hirsch, Rae Holcomb, Steve B. Howell, Jon M. Jenkins, David W. Latham, Andrew Mayo, Ismael Mireles, Teo Močnik, Joseph M. Akana Murphy, Daria Pidhorodetska, Alex S. Polanski, George R. Ricker, Lee J. Rosenthal, Ryan A. Rubenzahl, S. Seager, Nicholas Scarsdale, Emma V. Turtelboom, Roland Vanderspek, Joshua N. Winn |
| Jazyk: |
angličtina |
| Rok vydání: |
2022 |
| Předmět: |
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| Popis: |
We present the Distant Giants Survey, a three-year radial velocity campaign to measure P(DG∣CS), the conditional occurrence of distant giant planets (DG; M p ∼ 0.3–13 M J, P > 1 yr) in systems hosting a close-in small planet (CS; R p < 10 R ⊕). For the past two years, we have monitored 47 Sun-like stars hosting small transiting planets detected by TESS. We present the selection criteria used to assemble our sample and report the discovery of two distant giant planets, TOI-1669 b and TOI-1694 c. For TOI-1669 b we find that M sin i = 0.573 ± 0.074 M J , P = 502 ± 16 days, and e < 0.27, while for TOI-1694 c, M sin i = 1.05 ± 0.05 M J , P = 389.2 ± 3.9 days, and e = 0.18 ± 0.05. We also confirmed the 3.8 days transiting planet TOI-1694 b by measuring a true mass of M = 26.1 ± 2.2 M ⊕. At the end of the Distant Giants Survey, we will incorporate TOI-1669 b and TOI-1694 c into our calculation of P(DG∣CS), a crucial statistic for understanding the relationship between outer giants and small inner companions. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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