Two New HATNet Hot Jupiters around A Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS

G. Zhou; C. X. Huang; G. Á. Bakos; J. D. Hartman; David W. Latham; S. N. Quinn; K. A. Collins; J. N. Winn; I. Wong; G. Kovács; Z. Csubry; W. Bhatti; K. Penev; A. Bieryla; G. A. Esquerdo; P. Berlind; M. L. Calkins; M. de Val-Borro; R. W. Noyes; J. Lázár; I. Papp; P. Sári; T. Kovács; Lars A. Buchhave; T. Szklenar; B. Béky; M. C. Johnson; W. D. Cochran; A. Y. Kniazev; K. G. Stassun; B. J. Fulton; A. Shporer; N. Espinoza; D. Bayliss; M. Everett; S. B. Howell; C. Hellier; D. R. Anderson; A. Collier Cameron; R. G. West; D. J. A. Brown; N. Schanche; K. Barkaoui; F. Pozuelos; M. Gillon; E. Jehin; Z. Benkhaldoun; A. Daassou; G. Ricker; R. Vanderspek; S. Seager; J. M. Jenkins; Jack J. Lissauer; J. D. Armstrong; K. I. Collins; T. Gan; R. Hart; K. Horne; J. F. Kielkopf; L. D. Nielsen; T. Nishiumi; N. Narita; E. Palle; H. M. Relles; R. Sefako; T. G. Tan; M. Davies; Robert F. Goeke; N. Guerrero; K. Haworth; S. Villanueva

doi:10.3847/1538-3881/ab36b5

Two New HATNet Hot Jupiters around A Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS

G. Zhou^*, C. X. Huang, G. Á. Bakos, J. D. Hartman, David W. Latham, S. N. Quinn, K. A. Collins, J. N. Winn, I. Wong, G. Kovács, Z. Csubry, W. Bhatti, K. Penev, A. Bieryla, G. A. Esquerdo, P. Berlind, M. L. Calkins, M. de Val-Borro, R. W. Noyes, J. LázárI. Papp, P. Sári, T. Kovács, Lars A. Buchhave, T. Szklenar, B. Béky, M. C. Johnson, W. D. Cochran, A. Y. Kniazev, K. G. Stassun, B. J. Fulton, A. Shporer, N. Espinoza, D. Bayliss, M. Everett, S. B. Howell, C. Hellier, D. R. Anderson, A. Collier Cameron, R. G. West, D. J. A. Brown, N. Schanche, K. Barkaoui, F. Pozuelos, M. Gillon, E. Jehin, Z. Benkhaldoun, A. Daassou, G. Ricker, R. Vanderspek, S. Seager, J. M. Jenkins, Jack J. Lissauer, J. D. Armstrong, K. I. Collins, T. Gan, R. Hart, K. Horne, J. F. Kielkopf, L. D. Nielsen, T. Nishiumi, N. Narita, E. Palle, H. M. Relles, R. Sefako, T. G. Tan, M. Davies, Robert F. Goeke, N. Guerrero, K. Haworth, S. Villanueva

^*Corresponding author for this work

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Abstract

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.

Original language	English
Article number	141
Journal	Astrophysical Journal
Volume	158
Issue number	4
Number of pages	24
ISSN	0004-637X
DOIs	https://doi.org/10.3847/1538-3881/ab36b5
Publication status	Published - 2019

Keywords

Planetary systems
Stars: individual (HAT-P-69,HAT-P-70, TIC379929661, TIC399870368)
Techniques: photometric
Techniques: spectroscopic

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Zhou, G., Huang, C. X., Bakos, G. Á., Hartman, J. D., Latham, D. W., Quinn, S. N., Collins, K. A., Winn, J. N., Wong, I., Kovács, G., Csubry, Z., Bhatti, W., Penev, K., Bieryla, A., Esquerdo, G. A., Berlind, P., Calkins, M. L., Val-Borro, M. D., Noyes, R. W., ... Villanueva, S. (2019). Two New HATNet Hot Jupiters around A Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS. Astrophysical Journal, 158(4), Article 141. https://doi.org/10.3847/1538-3881/ab36b5

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title = "Two New HATNet Hot Jupiters around A Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS",

abstract = "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.",

keywords = "Planetary systems, Stars: individual (HAT-P-69,HAT-P-70, TIC379929661, TIC399870368), Techniques: photometric, Techniques: spectroscopic",

author = "G. Zhou and Huang, {C. X.} and Bakos, {G. {\'A}.} and Hartman, {J. D.} and Latham, {David W.} and Quinn, {S. N.} and Collins, {K. A.} and Winn, {J. N.} and I. Wong and G. Kov{\'a}cs and Z. Csubry and W. Bhatti and K. Penev and A. Bieryla and Esquerdo, {G. A.} and P. Berlind and Calkins, {M. L.} and Val-Borro, {M. de} and Noyes, {R. W.} and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri and T. Kov{\'a}cs and Buchhave, {Lars A.} and T. Szklenar and B. B{\'e}ky and Johnson, {M. C.} and Cochran, {W. D.} and Kniazev, {A. Y.} and Stassun, {K. G.} and Fulton, {B. J.} and A. Shporer and N. Espinoza and D. Bayliss and M. Everett and Howell, {S. B.} and C. Hellier and Anderson, {D. R.} and Cameron, {A. Collier} and West, {R. G.} and Brown, {D. J. A.} and N. Schanche and K. Barkaoui and F. Pozuelos and M. Gillon and E. Jehin and Z. Benkhaldoun and A. Daassou and G. Ricker and R. Vanderspek and S. Seager and Jenkins, {J. M.} and Lissauer, {Jack J.} and Armstrong, {J. D.} and Collins, {K. I.} and T. Gan and R. Hart and K. Horne and Kielkopf, {J. F.} and Nielsen, {L. D.} and T. Nishiumi and N. Narita and E. Palle and Relles, {H. M.} and R. Sefako and Tan, {T. G.} and M. Davies and Goeke, {Robert F.} and N. Guerrero and K. Haworth and S. Villanueva",

year = "2019",

doi = "10.3847/1538-3881/ab36b5",

language = "English",

volume = "158",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "4",

}

Zhou, G, Huang, CX, Bakos, GÁ, Hartman, JD, Latham, DW, Quinn, SN, Collins, KA, Winn, JN, Wong, I, Kovács, G, Csubry, Z, Bhatti, W, Penev, K, Bieryla, A, Esquerdo, GA, Berlind, P, Calkins, ML, Val-Borro, MD, Noyes, RW, Lázár, J, Papp, I, Sári, P, Kovács, T, Buchhave, LA, Szklenar, T, Béky, B, Johnson, MC, Cochran, WD, Kniazev, AY, Stassun, KG, Fulton, BJ, Shporer, A, Espinoza, N, Bayliss, D, Everett, M, Howell, SB, Hellier, C, Anderson, DR, Cameron, AC, West, RG, Brown, DJA, Schanche, N, Barkaoui, K, Pozuelos, F, Gillon, M, Jehin, E, Benkhaldoun, Z, Daassou, A, Ricker, G, Vanderspek, R, Seager, S, Jenkins, JM, Lissauer, JJ, Armstrong, JD, Collins, KI, Gan, T, Hart, R, Horne, K, Kielkopf, JF, Nielsen, LD, Nishiumi, T, Narita, N, Palle, E, Relles, HM, Sefako, R, Tan, TG, Davies, M, Goeke, RF, Guerrero, N, Haworth, K & Villanueva, S 2019, 'Two New HATNet Hot Jupiters around A Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS', Astrophysical Journal, vol. 158, no. 4, 141. https://doi.org/10.3847/1538-3881/ab36b5

TY - JOUR

T1 - Two New HATNet Hot Jupiters around A Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS

AU - Zhou, G.

AU - Huang, C. X.

AU - Bakos, G. Á.

AU - Hartman, J. D.

AU - Latham, David W.

AU - Quinn, S. N.

AU - Collins, K. A.

AU - Winn, J. N.

AU - Wong, I.

AU - Kovács, G.

AU - Csubry, Z.

AU - Bhatti, W.

AU - Penev, K.

AU - Bieryla, A.

AU - Esquerdo, G. A.

AU - Berlind, P.

AU - Calkins, M. L.

AU - Val-Borro, M. de

AU - Noyes, R. W.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

AU - Kovács, T.

AU - Buchhave, Lars A.

AU - Szklenar, T.

AU - Béky, B.

AU - Johnson, M. C.

AU - Cochran, W. D.

AU - Kniazev, A. Y.

AU - Stassun, K. G.

AU - Fulton, B. J.

AU - Shporer, A.

AU - Espinoza, N.

AU - Bayliss, D.

AU - Everett, M.

AU - Howell, S. B.

AU - Hellier, C.

AU - Anderson, D. R.

AU - Cameron, A. Collier

AU - West, R. G.

AU - Brown, D. J. A.

AU - Schanche, N.

AU - Barkaoui, K.

AU - Pozuelos, F.

AU - Gillon, M.

AU - Jehin, E.

AU - Benkhaldoun, Z.

AU - Daassou, A.

AU - Ricker, G.

AU - Vanderspek, R.

AU - Seager, S.

AU - Jenkins, J. M.

AU - Lissauer, Jack J.

AU - Armstrong, J. D.

AU - Collins, K. I.

AU - Gan, T.

AU - Hart, R.

AU - Horne, K.

AU - Kielkopf, J. F.

AU - Nielsen, L. D.

AU - Nishiumi, T.

AU - Narita, N.

AU - Palle, E.

AU - Relles, H. M.

AU - Sefako, R.

AU - Tan, T. G.

AU - Davies, M.

AU - Goeke, Robert F.

AU - Guerrero, N.

AU - Haworth, K.

AU - Villanueva, S.

PY - 2019

Y1 - 2019

N2 - 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.

AB - 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.

KW - Planetary systems

KW - Stars: individual (HAT-P-69,HAT-P-70, TIC379929661, TIC399870368)

KW - Techniques: photometric

KW - Techniques: spectroscopic

U2 - 10.3847/1538-3881/ab36b5

DO - 10.3847/1538-3881/ab36b5

M3 - Journal article

SN - 0004-637X

VL - 158

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 4

M1 - 141

ER -

Two New HATNet Hot Jupiters around A Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS

Abstract

Keywords

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