e report a latest generation of the laser frequency comb (LFC) for astronomy. The new features include all fiber coupled, alignment-free filter cavities; specially designed photonic crystal fiber for spectral broadening; reflective spectral flattening systems. All the features ensure the long-term stability of the whole LFC system. The LFC is designed to operate in two modes. The visible mode generates a supercontinuum from 445 nm to 870 nm, that covers 100 % spectral range of the Keck Planet Finder (KPF) spectrograph. The near-infrared mode offers a flat-top supercontinuum from 915 nm to 1450 nm, is prepared as a calibration source of the short-wavelength part of a near infrared (NIR) spectrograph