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Observing the Sun as a Star: Design and Early Results from the NEID Solar Feed

Lin, Andrea S. J. and Monson, Andrew and Mahadevan, Suvrath and Ninan, Joe P. and Halverson, Samuel and Nitroy, Colin and Bender, Chad F. and Logsdon, Sarah E. and Kanodia, Shubham and Terrien, Ryan C. and Roy, Arpita and Luhn, Jacob K. and Gupta, Arvind F. and Ford, Eric B. and Hearty, Fred and Laher, Russ R. and Hunting, Emily and McBride, William R. and Salazar Rivera, Noah Isaac and Rajagopal, Jayadev and Wolf, Marsha J. and Robertson, Paul and Wright, Jason T. and Blake, Cullen H. and Cañas, Caleb I. and Lubar, Emily and McElwain, Michael W. and Ramsey, Lawrence W. and Schwab, Christian and Stefansson, Gudmundur (2022) Observing the Sun as a Star: Design and Early Results from the NEID Solar Feed. Astronomical Journal, 163 (4). Art. No. 184. ISSN 0004-6256. doi:10.3847/1538-3881/ac5622. https://resolver.caltech.edu/CaltechAUTHORS:20220322-741611000

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Abstract

Efforts with extreme-precision radial velocity (EPRV) instruments to detect small-amplitude planets are largely limited, on many timescales, by the effects of stellar variability and instrumental systematics. One avenue for investigating these effects is the use of small solar telescopes which direct disk-integrated sunlight to these EPRV instruments, observing the Sun at high cadence over months or years. We have designed and built a solar feed system to carry out “Sun-as-a-star” observations with NEID, a very high precision Doppler spectrometer recently commissioned at the WIYN 3.5 m Telescope at Kitt Peak National Observatory. The NEID solar feed has been taking observations nearly every day since 2020 December; data is publicly available at the NASA Exoplanet Science Institute NEID Solar Archive: https://neid.ipac.caltech.edu/search_solar.php. In this paper, we present the design of the NEID solar feed and explanations behind our design intent. We also present early radial velocity (RV) results which demonstrate NEID's RV stability on the Sun over 4 months of commissioning: 0.66 m s⁻¹ rms under good sky conditions and improving to 0.41 m s⁻¹ rms under best conditions.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-3881/ac5622DOIArticle
https://arxiv.org/abs/2112.05711arXivDiscussion Paper
https://neid.ipac.caltech.edu/search_solar.phpRelated ItemNASA Exoplanet Science Institute NEID Solar Archive
ORCID:
AuthorORCID
Lin, Andrea S. J.0000-0002-9082-6337
Monson, Andrew0000-0002-0048-2586
Mahadevan, Suvrath0000-0001-9596-7983
Ninan, Joe P.0000-0001-8720-5612
Halverson, Samuel0000-0003-1312-9391
Nitroy, Colin0000-0001-5747-5064
Bender, Chad F.0000-0003-4384-7220
Logsdon, Sarah E.0000-0002-9632-9382
Kanodia, Shubham0000-0001-8401-4300
Terrien, Ryan C.0000-0002-4788-8858
Roy, Arpita0000-0001-8127-5775
Luhn, Jacob K.0000-0002-4927-9925
Gupta, Arvind F.0000-0002-5463-9980
Ford, Eric B.0000-0001-6545-639X
Hearty, Fred0000-0002-1664-3102
Laher, Russ R.0000-0003-2451-5482
Salazar Rivera, Noah Isaac0000-0002-0289-3135
Rajagopal, Jayadev0000-0002-2488-7123
Wolf, Marsha J.0000-0002-7827-6184
Robertson, Paul0000-0003-0149-9678
Wright, Jason T.0000-0001-6160-5888
Blake, Cullen H.0000-0002-6096-1749
Cañas, Caleb I.0000-0003-4835-0619
Lubar, Emily0000-0003-0790-7492
McElwain, Michael W.0000-0003-0241-8956
Ramsey, Lawrence W.0000-0002-4289-7958
Schwab, Christian0000-0002-0091-7105
Stefansson, Gudmundur0000-0001-7409-5688
Additional Information:© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received 2021 December 10; revised 2022 February 4; accepted 2022 February 15; published 2022 March 22. Based on observations at Kitt Peak National Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. NEID and WIYN Data presented were obtained by the NEID spectrograph built by Penn State University and operated at the WIYN Observatory by NOIRLab, under the NN-EXPLORE partnership of the National Aeronautics and Space Administration and the National Science Foundation. WIYN is a joint facility of the University of Wisconsin–Madison, Indiana University, NSF's NOIRLab, the Pennsylvania State University, Purdue University, University of California, Irvine, and the University of Missouri. The authors are honored to be permitted to conduct astronomical research on Iolkam Du'ag (Kitt Peak), a mountain with particular significance to the Tohono O'odham. This research was supported by Heising-Simons Foundation grant # 2019-1177. This work was partially supported by funding from the Center for Exoplanets and Habitable Worlds. The Center for Exoplanets and Habitable Worlds and the Penn State Extraterrestrial Intelligence Center are supported by the Pennsylvania State University and the Eberly College of Science. CIC acknowledges support by NASA Headquarters under the NASA Earth and Space Science Fellowship Program through grant 80NSSC18K1114. Part of this work was performed for the Jet Propulsion Laboratory, California Institute of Technology, sponsored by the United States Government under the Prime Contract 80NM0018D0004 between Caltech and NASA. Computations for this research were performed on the Pennsylvania State Universitys Institute for Computational and Data Sciences Roar supercomputer. Processing of data included here used an allocation of computer time from the Research Computing High Performance Computing cluster at the University of Arizona, which is gratefully acknowledged. We acknowledge BJ Fulton and colleagues at the NASA Exoplanet Science Institute (NExScI) for their efforts in hosting the NEID Solar Data Archive. This research has made use of NASA's Astrophysics Data System Bibliographic Services. This research made use of Astropy (http://www.astropy.org), a community-developed core Python package for Astronomy Astropy Collaboration et al. (2013), Astropy Collaboration et al. (2018). Facility: NEID/WIYN 3.5 m. - Software: astropy (Astropy Collaboration et al. 2018), barycorrpy (Kanodia & Wright 2018), matplotlib (Hunter 2007), numpy (van der Walt et al. 2011), pandas (McKinney 2010), pvlib (Holmgren et al. 2018), scipy (Virtanen et al. 2020).
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
Heising-Simons Foundation2019-1177
Center for Exoplanets and Habitable WorldsUNSPECIFIED
Pennsylvania State UniversityUNSPECIFIED
Eberly College of ScienceUNSPECIFIED
NASA Earth and Space Science Fellowship80NSSC18K1114
NASA/JPL/Caltech80NM0018D0004
Subject Keywords:Exoplanets; Radial velocity; Solar telescopes; Solar activity
Issue or Number:4
Classification Code:Unified Astronomy Thesaurus concepts: Exoplanets (498); Radial velocity (1332); Solar telescopes (1531); Solar activity (1475)
DOI:10.3847/1538-3881/ac5622
Record Number:CaltechAUTHORS:20220322-741611000
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220322-741611000
Official Citation:Andrea S. J. Lin et al 2022 AJ 163 184
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:113992
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:23 Mar 2022 17:15
Last Modified:23 Mar 2022 17:15

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