13 December 2020Time-variable differences between H2RG readout channels in high precision spectroscopy: a case study with the Habitable-zone Planet Finder
Ryan C. Terrien,1 Joe Ninan,2 Chad Benderhttps://orcid.org/0000-0003-4384-7220,3 Suvrath Mahadevan,2 Scott Diddams,4,5 Connor Fredrick,5 Samuel Halverson,6,7 Andrew J. Metcalf,8 Andrew Monson,2 Arpita Roy,9 Guðmundur Stefánsson,10 Lawrence Ramsey2
1Carleton College (United States) 2The Pennsylvania State Univ. (United States) 3The Univ. of Arizona (United States) 4National Institute of Standards and Technology (United States) 5The Univ. of Colorado (United States) 6Massachusetts Institute of Technology (United States) 7Jet Propulsion Lab. (United States) 8Air Force Research Lab. (United States) 9Caltech (United States) 10Princeton Univ. (United States)
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High precision Doppler spectroscopy hinges on an accurate understanding of the wavelength-to-pixel mapping (wavelength solution) of the spectrograph, including particularly systematics related to the detector. Herein, we describe the uniformity and stability of the wavelength solution of the Habitable-zone Planet Finder (HPF), a near-infrared spectrograph that utilizes a Hawaii-2RG (H2RG) hybrid CMOS detector. We focus on time-varying discontinuities equivalent to approximately 10 m/s in the otherwise-smooth wavelength solution, corresponding to the boundaries between H2RG readout channels. This behavior is revealed by calibration with dedicated laser frequency comb and white light-illuminated Fabry-Perot systems over a ~1 year baseline. These findings will inform the usage of similar near-infrared CMOS devices for high-precision applications including Doppler exoplanet and gravitational lensing WFIRST surveys.
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Ryan C. Terrien, Joe Ninan, Chad Bender, Suvrath Mahadevan, Scott Diddams, Connor Fredrick, Samuel Halverson, Andrew J. Metcalf, Andrew Monson, Arpita Roy, Guðmundur Stefánsson, Lawrence Ramsey, "Time-variable differences between H2RG readout channels in high precision spectroscopy: a case study with the Habitable-zone Planet Finder," Proc. SPIE 11454, X-Ray, Optical, and Infrared Detectors for Astronomy IX, 114541T (13 December 2020); https://doi.org/10.1117/12.2576318