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Radial velocity (RV) surveys supported by high precision wavelengthreferences (notably ThAr lamps and I2 cells) have successfully identifiedhundreds of exoplanets; however, as the search for exoplanets moves to cooler,lower mass stars, the optimum wave band for observation for these objects movesinto the near infrared (NIR) and new wavelength standards are required. Toaddress this need we are following up our successful deployment of an Hband(1.45-1.7{\mu}m) laser frequency comb based wavelength reference with acomb working in the Y and J bands (0.98-1.3{\mu}m). This comb will be optimizedfor use with a 50,000 resolution NIR spectrograph such as the Penn StateHabitable Zone Planet Finder. We present design and performance details of thecurrent Y+J band comb.

A near infrared frequency comb for Y+J band astronomical spectroscopy