HAT-P-58b — HAT-P-64b: Seven Planets Transiting Bright Stars. (arXiv:2007.05528v1 [astro-ph.EP])

HAT-P-58b — HAT-P-64b: Seven Planets Transiting Bright Stars. (arXiv:2007.05528v1 [astro-ph.EP])
<a href="http://arxiv.org/find/astro-ph/1/au:+Bakos_G/0/1/0/all/0/1">G. &#xc1;. Bakos</a> (1), <a href="http://arxiv.org/find/astro-ph/1/au:+Hartman_J/0/1/0/all/0/1">J. D. Hartman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bhatti_W/0/1/0/all/0/1">W. Bhatti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Csubry_Z/0/1/0/all/0/1">Z. Csubry</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Penev_K/0/1/0/all/0/1">K. Penev</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bieryla_A/0/1/0/all/0/1">A. Bieryla</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Latham_D/0/1/0/all/0/1">D. W. Latham</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Quinn_S/0/1/0/all/0/1">S. Quinn</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Buchhave_L/0/1/0/all/0/1">L. A. Buchhave</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kovacs_G/0/1/0/all/0/1">G. Kov&#xe1;cs</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Torres_G/0/1/0/all/0/1">G. Torres</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Noyes_R/0/1/0/all/0/1">R. W. Noyes</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Falco_E/0/1/0/all/0/1">E. Falco</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Beky_B/0/1/0/all/0/1">B. B&#xe9;ky</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Szklenar_T/0/1/0/all/0/1">T. Szklen&#xe1;r</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Esquerdo_G/0/1/0/all/0/1">G. A. Esquerdo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Howard_A/0/1/0/all/0/1">A. W. Howard</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Isaacson_H/0/1/0/all/0/1">H. Isaacson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Marcy_G/0/1/0/all/0/1">G. Marcy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sato_B/0/1/0/all/0/1">B. Sato</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Boisse_I/0/1/0/all/0/1">I. Boisse</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Santerne_A/0/1/0/all/0/1">A. Santerne</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hebrard_G/0/1/0/all/0/1">G. H&#xe9;brard</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rabus_M/0/1/0/all/0/1">M. Rabus</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Harbeck_D/0/1/0/all/0/1">D. Harbeck</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+McCully_C/0/1/0/all/0/1">C. McCully</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Everett_M/0/1/0/all/0/1">M. E. Everett</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Horch_E/0/1/0/all/0/1">E. P. Horch</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hirsch_L/0/1/0/all/0/1">L. Hirsch</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Howell_S/0/1/0/all/0/1">S. B. Howell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Huang_C/0/1/0/all/0/1">C. X. Huang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lazar_J/0/1/0/all/0/1">J. L&#xe1;z&#xe1;r</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Papp_I/0/1/0/all/0/1">I. Papp</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sari_P/0/1/0/all/0/1">P. S&#xe1;ri</a> (1: Department Astrophysical Sciences, Princeton University)

We report the discovery and characterization of 7 transiting exoplanets from
the HATNet survey. The planets, which are hot Jupiters and Saturns transiting
bright sun-like stars, include: HAT-P-58b (with mass Mp = 0.37 MJ, radius Rp =
1.33 RJ, and orbital period P = 4.0138 days), HAT-P-59b (Mp = 1.54 MJ, Rp =
1.12 RJ, P = 4.1420 days), HAT-P-60b (Mp = 0.57 MJ, Rp = 1.63 RJ, P = 4.7948
days), HAT-P-61b (Mp = 1.06 MJ, Rp = 0.90 RJ, P = 1.9023 days), HAT-P-62b (Mp =
0.76 MJ, Rp = 1.07 RJ, P = 2.6453 days), HAT-P-63b (Mp = 0.61 MJ, Rp = 1.12 RJ,
P = 3.3777 days), and HAT-P-64b (Mp = 0.58 MJ, Rp = 1.70 RJ, P = 4.0072 days).
The typical errors on these quantities are 0.06 MJ, 0.03 RJ, and 0.2seconds,
respectively. We also provide accurate stellar parameters for each of the hosts
stars. With V = 9.710+/-0.050mag, HAT-P-60 is an especially bright transiting
planet host, and an excellent target for additional follow-up observations.
With Rp = 1.703+/-0.070 RJ, HAT-P-64b is a highly inflated hot Jupiter around a
star nearing the end of its main-sequence lifetime, and is among the largest
known planets. Five of the seven systems have long-cadence observations by TESS
which are included in the analysis. Of particular note is HAT-P-59
(TOI-1826.01) which is within the Northern continuous viewing zone of the TESS
mission, and HAT-P-60, which is the TESS candidate TOI-1580.01.

We report the discovery and characterization of 7 transiting exoplanets from
the HATNet survey. The planets, which are hot Jupiters and Saturns transiting
bright sun-like stars, include: HAT-P-58b (with mass Mp = 0.37 MJ, radius Rp =
1.33 RJ, and orbital period P = 4.0138 days), HAT-P-59b (Mp = 1.54 MJ, Rp =
1.12 RJ, P = 4.1420 days), HAT-P-60b (Mp = 0.57 MJ, Rp = 1.63 RJ, P = 4.7948
days), HAT-P-61b (Mp = 1.06 MJ, Rp = 0.90 RJ, P = 1.9023 days), HAT-P-62b (Mp =
0.76 MJ, Rp = 1.07 RJ, P = 2.6453 days), HAT-P-63b (Mp = 0.61 MJ, Rp = 1.12 RJ,
P = 3.3777 days), and HAT-P-64b (Mp = 0.58 MJ, Rp = 1.70 RJ, P = 4.0072 days).
The typical errors on these quantities are 0.06 MJ, 0.03 RJ, and 0.2seconds,
respectively. We also provide accurate stellar parameters for each of the hosts
stars. With V = 9.710+/-0.050mag, HAT-P-60 is an especially bright transiting
planet host, and an excellent target for additional follow-up observations.
With Rp = 1.703+/-0.070 RJ, HAT-P-64b is a highly inflated hot Jupiter around a
star nearing the end of its main-sequence lifetime, and is among the largest
known planets. Five of the seven systems have long-cadence observations by TESS
which are included in the analysis. Of particular note is HAT-P-59
(TOI-1826.01) which is within the Northern continuous viewing zone of the TESS
mission, and HAT-P-60, which is the TESS candidate TOI-1580.01.

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