The NEID Earth Twin Survey. III. Survey Performance After Three Years on Sky

Fuente: arXiv
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Autores principales: Gupta, Arvind F., Fitzmaurice, Evan, Mahadevan, Suvrath, Robertson, Paul, Luhn, Jacob K., Wright, Jason T., Logsdon, Sarah E., Krolikowski, Daniel M., Paredes, Leonardo A., Bender, Chad F., Giovinazzi, Mark R., Lin, Andrea S., Blake, Cullen H., Cañas, Caleb I., Ford, Eric B., Halverson, Samuel P., Kanodia, Shubham, McElwain, Michael W., Monson, Andrew, Ninan, Joe P., Rajagopal, Jayadev, Roy, Arpita, Schwab, Christian, Stefánsson, Guðmundur, Terrien, Ryan C.
Formato: Preprint
Publicado: 2025
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author Gupta, Arvind F.
Fitzmaurice, Evan
Mahadevan, Suvrath
Robertson, Paul
Luhn, Jacob K.
Wright, Jason T.
Logsdon, Sarah E.
Krolikowski, Daniel M.
Paredes, Leonardo A.
Bender, Chad F.
Giovinazzi, Mark R.
Lin, Andrea S.
Blake, Cullen H.
Cañas, Caleb I.
Ford, Eric B.
Halverson, Samuel P.
Kanodia, Shubham
McElwain, Michael W.
Monson, Andrew
Ninan, Joe P.
Rajagopal, Jayadev
Roy, Arpita
Schwab, Christian
Stefánsson, Guðmundur
Terrien, Ryan C.
author_facet Gupta, Arvind F.
Fitzmaurice, Evan
Mahadevan, Suvrath
Robertson, Paul
Luhn, Jacob K.
Wright, Jason T.
Logsdon, Sarah E.
Krolikowski, Daniel M.
Paredes, Leonardo A.
Bender, Chad F.
Giovinazzi, Mark R.
Lin, Andrea S.
Blake, Cullen H.
Cañas, Caleb I.
Ford, Eric B.
Halverson, Samuel P.
Kanodia, Shubham
McElwain, Michael W.
Monson, Andrew
Ninan, Joe P.
Rajagopal, Jayadev
Roy, Arpita
Schwab, Christian
Stefánsson, Guðmundur
Terrien, Ryan C.
contents The NEID Earth Twin Survey (NETS) has been delivering a rich set of precise radial velocity (RV) measurements for 41 bright, nearby main sequence stars. Here, we describe the status of the survey after three years on sky and we present the full set of RV measurements and accompanying stellar activity indicators. We discuss intermediate survey diagnostics, including calibration of the known RV zero point offset introduced following the Contreras fire in 2022 and the identification of an undiagnosed and previously unknown zero point offset in 2021. An analysis of our data set using RVSearch demonstrates that for these target stars, NEID is independently sensitive to nearly all known planets with periods shorter than the NETS observing baseline. We also highlight a number of newly detected RV signals, which present exciting opportunities for future investigations.
format Preprint
id arxiv_https___arxiv_org_abs_2506_23704
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The NEID Earth Twin Survey. III. Survey Performance After Three Years on Sky
Gupta, Arvind F.
Fitzmaurice, Evan
Mahadevan, Suvrath
Robertson, Paul
Luhn, Jacob K.
Wright, Jason T.
Logsdon, Sarah E.
Krolikowski, Daniel M.
Paredes, Leonardo A.
Bender, Chad F.
Giovinazzi, Mark R.
Lin, Andrea S.
Blake, Cullen H.
Cañas, Caleb I.
Ford, Eric B.
Halverson, Samuel P.
Kanodia, Shubham
McElwain, Michael W.
Monson, Andrew
Ninan, Joe P.
Rajagopal, Jayadev
Roy, Arpita
Schwab, Christian
Stefánsson, Guðmundur
Terrien, Ryan C.
Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
The NEID Earth Twin Survey (NETS) has been delivering a rich set of precise radial velocity (RV) measurements for 41 bright, nearby main sequence stars. Here, we describe the status of the survey after three years on sky and we present the full set of RV measurements and accompanying stellar activity indicators. We discuss intermediate survey diagnostics, including calibration of the known RV zero point offset introduced following the Contreras fire in 2022 and the identification of an undiagnosed and previously unknown zero point offset in 2021. An analysis of our data set using RVSearch demonstrates that for these target stars, NEID is independently sensitive to nearly all known planets with periods shorter than the NETS observing baseline. We also highlight a number of newly detected RV signals, which present exciting opportunities for future investigations.
title The NEID Earth Twin Survey. III. Survey Performance After Three Years on Sky
topic Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2506.23704