2019AJ....158..141Z

Query : 2019AJ....158..141Z

2019AJ....158..141Z - Astron. J., 158, 141-141 (2019/October-0)

Two new HATNet hot Jupiters around A stars and the first glimpse at the occurrence rate of hot Jupiters from TESS.

ZHOU G., HUANG C.X., BAKOS G.A., HARTMAN J.D., LATHAM D.W., QUINN S.N., COLLINS K.A., WINN J.N., WONG I., KOVACS G., CSUBRY Z., BHATTI W., PENEV K., BIERYLA A., ESQUERDO G.A., BERLIND P., CALKINS M.L., DE VAL-BORRO M., NOYES R.W., LAZAR J., PAPP I., SARI P., KOVACS T., BUCHHAVE L.A., SZKLENAR T., BEKY B., JOHNSON M.C., COCHRAN W.D., KNIAZEV A.Y., STASSUN K.G., FULTON B.J., SHPORER A., ESPINOZA N., BAYLISS D., EVERETT M., HOWELL S.B., HELLIER C., ANDERSON D.R., CAMERON A.C., WEST R.G., BROWN D.J.A., SCHANCHE N., BARKAOUI K., POZUELOS F., GILLON M., JEHIN E., BENKHALDOUN Z., DAASSOU A., RICKER G., VANDERSPEK R., SEAGER S., JENKINS J.M., LISSAUER J.J., ARMSTRONG J.D., COLLINS K.I., GAN T., HART R., HORNE K., KIELKOPF J.F., NIELSEN L.D., NISHIUMI T., NARITA N., PALLE E., RELLES H.M., SEFAKO R., TAN T.G., DAVIES M., GOEKE R.F., GUERRERO N., HAWORTH K. and VILLANUEVA S.

Abstract (from CDS):

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 3.58–0.58+0.58MJup and a radius of 1.676–0.033+0.051RJup and resides in a prograde 4.79 day orbit. HAT-P-70 b has a radius of 1.87–0.10+0.15RJup and a mass constraint of < 6.78(3σ )MJup 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 Tmag = 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.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): planetary systems - stars: individual: (HAT-P-69, HAT-P-70, TIC379929661, TIC399870368) - techniques: photometric - techniques: spectroscopic

VizieR on-line data: <Available at CDS (J/AJ/158/141): table2.dat table3.dat table5.dat table6.dat table9.dat table10.dat table11.dat table12.dat>

Simbad objects: 50

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Number of rows : 50
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 CD-55 9423 PM* 00 00 44.9091865512 -54 49 49.852301232   12.29 11.13 10.677   K4V 40 0
2 HD 2685 * 00 29 18.9525583296 -76 18 14.621613984   10.05 9.59     F2III/IV 25 0
3 HATS-71 PM* 01 02 12.2806419528 -61 45 21.661597188         14.01 M3 18 0
4 HD 10069 SB* 01 37 25.0332798696 -45 40 40.374717456   9.74 9.30     F6IV/V 260 1
5 HD 10069b Pl 01 37 25.0332798696 -45 40 40.374717456           ~ 444 1
6 CD-56 324 PM* 01 38 25.0565551464 -55 46 19.525595664   11.31 10.57     G5 48 0
7 HD 15082 EB* 02 26 51.0582618096 +37 33 01.736482032   8.41 8.14     kA5hA8mF4 229 1
8 BD-07 436A PM* 02 28 37.2277668480 -07 03 38.376446076   11.07 10.29     G8 77 1
9 CD-50 777 * 02 39 35.4433933368 -50 00 28.879171596   10.08 9.48     F8 38 0
10 HD 20267 SB* 03 15 25.0234457184 -02 10 31.025592912   9.31 8.76     F6/7V 16 0
11 BD-20 646 * 03 28 54.1419221544 -19 58 47.171271252   10.577 10.097 9.95   F8 42 0
12 HD 27342 EB* 04 17 14.7416253504 -38 50 39.008822784   8.92 8.82     A2/3V 16 0
13 CD-30 1812 * 04 25 29.0166589296 -30 36 01.610731368   10.45 10.04     F5 72 1
14 CPD-65 373 EB* 04 42 40.8919901208 -64 53 06.708896448   10.36 10.08     ~ 15 0
15 BD+01 828 Em* 04 50 38.5587679752 +01 53 38.102222400   10.49 10.07     F5 34 0
16 HD 287325 * 04 58 12.5627969184 +09 59 52.804564656   9.62 9.47     A2 21 0
17 HD 287325b Pl 04 58 12.5627969184 +09 59 52.804564656           ~ 57 0
18 HD 33512 SB* 05 09 02.4466404144 -36 27 52.415052984   9.77 9.29     F5/6V 19 0
19 HD 35804 EB* 05 27 41.6603100912 +07 55 06.792627468   10.37 10.22     A2 9 0
20 NGTS-1 PM* 05 30 51.4522649760 -36 37 50.895680268   16.94 15.57 15.36 13.97 M0.5V 27 0
21 CPD-64 484 * 05 48 33.5933253192 -63 59 18.388382028   10.73 10.21 9.93 9.742 ~ 89 1
22 HATS-6 * 05 52 35.2366980288 -19 01 53.970810276   16.664 15.160     M1V 36 0
23 CD-57 1311 SB* 05 55 32.62392 -57 17 26.1312           ~ 30 0
24 BD-19 1337 EB* 06 03 39.8481551640 -19 02 27.134675016   10.47 10.13 10.238   ~ 8 0
25 HD 44717B BD? 06 23 18.69 +00 53 00.1           ~ 11 0
26 HD 44717 Em* 06 23 18.6911952888 +00 53 00.105902772   8.84 8.74     A0V 13 0
27 CPD-23 1329 * 06 33 24.2671186968 -23 29 10.297934988   10.78 10.34     F6 50 0
28 HD 288842b Pl 06 37 03.1363669152 +01 46 03.194967396           ~ 10 0
29 HD 288842 * 06 37 03.1363669152 +01 46 03.194967396   10.67 10.11     G0 17 0
30 HD 47874 EB* 06 38 19.5401003856 -47 36 49.897567548   9.46 9.17     F2IV/V 15 0
31 CD-24 5016 * 07 12 29.5499506296 -24 57 12.826133532   9.80 9.63     ~ 19 0
32 CD-57 1712 * 07 22 02.9952922776 -57 23 05.600400108   10.75 9.97     ~ 19 0
33 BD+07 1721 Pe* 07 26 02.2901761080 +07 36 56.815027668   10.21 9.86     A8V+G9V/K1V 35 0
34 BD+06 1909 Em* 08 15 47.9802408792 +05 50 12.350816484   10.95 10.35     F7 85 1
35 HAT-P-69b Pl 08 42 01.3562355288 +03 42 38.021676300           ~ 23 0
36 1SWASP J084201.35+034238.0 Pe* 08 42 01.3562355288 +03 42 38.021676300   10.05 9.77     A7V(Sr) 27 0
37 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
38 BD+46 2629 ** 19 07 53.104944 +46 52 06.00420   10.12 9.70 9.80   kA2hA5mA7(IV)m: 173 0
39 HD 195689 SB* 20 31 26.3534153736 +39 56 19.773037500   7.59 7.56     A0 151 0
40 CD-34 14724A PM* 20 55 07.9443524136 -34 08 08.007489384   10.74 10.05 10.17 9.774 F8 94 0
41 * alf Cep PM* 21 18 34.77233 +62 35 08.0681 2.770 2.680 2.460 2.22 2.11 A8Vn 374 0
42 HD 202772 ** 21 18 47.876136 -26 36 58.05108   10.72 10.21 8.94   G8/K1+A/F 29 0
43 HD 202678 * 21 19 47.9065883424 -58 08 55.991602356   10.98 10.47     G1/3(V) 38 1
44 HD 203621 * 21 24 27.5858065560 -37 51 00.552487788   9.99 9.56     F8V 12 0
45 TOI-155.01 Pl? 21 24 27.5858065560 -37 51 00.552487788           ~ 2 0
46 HD 208180 * 21 55 04.2428047728 -22 36 45.287047764   10.70 10.25 10.232   F6V 31 0
47 CD-48 14223 PM* 22 29 49.7355107880 -48 00 11.048684184   10.78 10.09     G2 39 0
48 HD 220559 ** 23 24 54.9994408307 -38 09 38.520682233   10.056 9.537 9.771   F7V 15 0
49 HD 222259A RS* 23 39 39.4808078664 -69 11 44.707735104   9.161 8.226 9.28 7.352 G6V 190 0
50 CD-35 16019 PM* 23 59 36.0711872328 -35 01 52.923618408   10.49 9.87 9.91   G6 139 0

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