Andrea Lin,1 Chad F. Benderhttps://orcid.org/0000-0003-4384-7220,2 Eric Ford,1 Zhao Guo,1 Samuel Halverson,3 Fred Hearty,1 Emily Huntinghttps://orcid.org/0009-0007-3512-7705,4 Shubham Kanodia,1 Kyle Kaplan,5 Suvrath Mahadevan,1 Michael W. McElwain,6 Andrew Monson,1 Joe Ninan,1 Colin Nitroy,1 Jayadev Rajagopal,4 Lawrence Ramsey,1 Paul Robertson,7 Arpita Roy,8 Christian Schwab,9 Gudmundur Stefansson,10 Daniel J. Stevens,1 Ryan Terrien,11 Jason Wright1
1The Pennsylvania State Univ. (United States) 2The Univ. of Arizona (United States) 3Jet Propulsion Lab. (United States) 4NSF’s National Optical-Infrared Astronomy Research Lab. (United States) 5NASA Ames Research Ctr. (United States) 6NASA Goddard Space Flight Ctr. (United States) 7Univ. of California, Irvine (United States) 8Caltech (United States) 9Macquarie Univ. (Australia) 10Princeton Univ. (United States) 11Carleton College (United States)
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NEID is a radial velocity (RV) instrument including an ultra-stabilized fiber-fed spectrograph, installed in 2019 at the 3.5m WIYN telescope at Kitt Peak National Observatory. Accompanying it is a solar feed system built to supply the spectrograph with disk-integrated sunlight. Observing the Sun “as a star” is essential for developing and validating mitigation strategies for RV variations due to stellar activity and instrument systematics, thus enabling more-effective detections of lower-mass exoplanets. In this paper, we will detail the design of the NEID solar feed system and showcase early results addressing NEID systematics and solar RV variability.
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Andrea Lin, Chad F. Bender, Eric Ford, Zhao Guo, Samuel Halverson, Fred Hearty, Emily Hunting, Shubham Kanodia, Kyle Kaplan, Suvrath Mahadevan, Michael W. McElwain, Andrew Monson, Joe Ninan, Colin Nitroy, Jayadev Rajagopal, Lawrence Ramsey, Paul Robertson, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Daniel J. Stevens, Ryan Terrien, Jason Wright, "A solar feed for NEID," Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 114473L (13 December 2020); https://doi.org/10.1117/12.2561520