The NEID precision radial velocity spectrometer

port adapter overview, requirements, and test plan

Sarah E. Logsdon*, Michael W. McElwain, Qian Gong, Ming Liang, Fernando Santoro, Christian Schwab, Chad Bender, Cullen Blake, Samuel Halverson, Fred Hearty, Emily Hunting, Kurt P. Jaehnig, Suvrath Mahadevan, Andrew J. Monson, Jeffrey W. Percival, Jayadev Rajagopal, Lawrence Ramsey, Arpita Roy, Michael P. Smith, Ryan C. Terrien & 4 others Erik Timmerman, Phil Willems, Marsha J. Wolf, Jason Wright

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution

2 Citations (Scopus)

Abstract

The NEID spectrometer is an optical (380-930 nm), fiber-fed, precision Doppler spectrometer currently in de- velopment for the WIYN 3.5 m telescope at Kitt Peak National Observatory as part of the NN-EXPLORE partnership. Designed to achieve a radial velocity precision of < 30 cm/s, NEID will be sensitive enough to detect terrestrial-mass exoplanets around low-mass stars. Light from the target stars is focused by the telescope to a bent Cassegrain port at the edge of the primary mirror mechanical support. The specialized NEID "Port Adapter" system is mounted at this bent Cassegrain port and is responsible for delivering the incident light from the telescope to the NEID fibers. In order to provide stable, high-quality images to the science instrument, the Port Adapter houses several sub-components designed to acquire the target stars, correct for atmospheric dis- persion, stabilize the light onto the science fibers, and calibrate the spectrometer by injecting known wavelength sources such as a laser frequency comb. Here we provide an overview of the overall opto-mechanical design and system requirements of the Port Adapter. We also describe the development of system error budgets and test plans to meet those requirements.

Original languageEnglish
Title of host publicationGround-based and Airborne Instrumentation for Astronomy VII
EditorsChristopher J. Evans, Luc Simard, Hideki Takami
Place of PublicationBellingham, Washington
PublisherSPIE
Pages1-10
Number of pages10
ISBN (Electronic)9781510619586
ISBN (Print)9781510619579
DOIs
Publication statusPublished - 27 Jul 2018
EventGround-based and Airborne Instrumentation for Astronomy VII 2018 - Austin, United States
Duration: 10 Jun 201814 Jun 2018

Publication series

NameProceedings of SPIE
PublisherSPIE
Volume10702
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceGround-based and Airborne Instrumentation for Astronomy VII 2018
CountryUnited States
CityAustin
Period10/06/1814/06/18

Keywords

  • exoplanets
  • radial velocity instrumentation
  • systems engineering

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