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 M _ { p } = 0.37 M _ { J } , radius R _ { p } = 1.33 R _ { J } , and orbital period P = 4.0138 days ) , HAT-P-59b ( M _ { p } = 1.54 M _ { J } , R _ { p } = 1.12 R _ { J } , P = 4.1420 days ) , HAT-P-60b ( M _ { p } = 0.57 M _ { J } , R _ { p } = 1.63 R _ { J } , P = 4.7948 days ) , HAT-P-61b ( M _ { p } = 1.06 M _ { J } , R _ { p } = 0.90 R _ { J } , P = 1.9023 days ) , HAT-P-62b ( M _ { p } = 0.76 M _ { J } , R _ { p } = 1.07 R _ { J } , P = 2.6453 days ) , HAT-P-63b ( M _ { p } = 0.61 M _ { J } , R _ { p } = 1.12 R _ { J } , P = 3.3777 days ) , and HAT-P-64b ( M _ { p } = 0.58 M _ { J } , R _ { p } = 1.70 R _ { J } , P = 4.0072 days ) . The typical errors on these quantities are 0.06 M _ { J } , 0.03 R _ { J } , and 0.2seconds , respectively . We also provide accurate stellar parameters for each of the hosts stars . With V = 9.710 \pm 0.050 mag , HAT-P-60 is an especially bright transiting planet host , and an excellent target for additional follow-up observations . With R _ { p } = 1.703 \pm 0.070 R _ { J } , 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 .