The Penn State Pathfinder is a prototype warm fiber-fed Echelle spectrograph with a Hawaii-1 NIR detector that has
already demonstrated 7-10 m/s radial velocity precision on integrated sunlight. The Pathfinder testbed was initially setup
for the Gemini PRVS design study to enable a systematic exploration of the challenges of achieving high radial velocity
precision in the near-infrared, as well as to test possible solutions to these calibration challenges. The current version of
the Pathfinder has an R3 echelle grating, and delivers a resolution of R~50,000 in the Y, J or H bands of the spectrum.
We will discuss the on sky-performance of the Pathfinder during an engineering test run at the Hobby Eberly Telescope
as well the results of velocity observations of M dwarfs. We will also discuss the unique calibration techniques we have
explored, like Uranium-Neon hollow cathode lamps, notch filter, and modal noise mitigation to enable high precision
radial velocity observation in the NIR. The Pathfinder is a prototype testbed precursor of a cooled high-resolution NIR
spectrograph capable of high radial velocity precision and of finding low mass planets around mid-late M dwarfs.
|