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We present a new comprehensive collection of stellar evolutionary tracks andisochrones for rotating low- and intermediate-mass stars assembled with theupdated version of PARSEC V2.0. This version includes our recent calibration ofthe extra mixing from overshooting and rotation, as well as severalimprovements in nuclear reaction network, treatment of convective zones, massloss and other physical input parameters. The initial mass of the stellarmodels covers the range from 0.09 $M_\odot$ to 14 $M_\odot$, for six sets ofinitial metallicity, from Z=0.004 to Z=0.017. Rotation is considered for starsabove $\sim 1 M_\odot$ with a smooth transition between non rotating andextremely fast-rotating models, based on the initial mass. For stars moremassive than $\sim 1.3~M_\odot$ the full rotation range, from low to thecritical one, is considered. We adopt the solar-scaled chemical mixture byCaffau et al. with Z$_\odot$ = 0.01524. All the evolutionary phases from thepre-main-sequence to the first few thermal-pulses on theasymptotic-giant-branch or central C exhaustion, are considered. Thecorresponding theoretical isochrones are further derived with TRILEGAL code andare converted in several photometric systems, taking into account differentinclination angles. Besides magnitudes, they also offer many other stellarobservables in line with the data that are being provided by current largesurveys. The new collection is fully integrated in a user friendly WEBinterface for the benefit of easily performing stellar population studies.

PARSEC V2.0: Stellar tracks and isochrones of low and intermediate mass stars with rotation