HAT-P-58b–HAT-P-64b: Seven Planets Transiting Bright Stars*

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