The NEID Port Adapter at WIYN: on-sky fast guiding performance

Dan Li; Sarah E. Logsdon; William McBride; Jayadev Rajagopal; Marsha J. Wolf; Jeffrey W. Percival; Kurt P. Jaehnig; Michael P. Smith; Qian Gong; Michael W. McElwain; Heidi Schweiker; Eli Golub; Jesus Higuera; Jessica Klusmeyer; Emily Hunting; Erik Timmermann; Mark Everett; Wilson Liu; Susan Ridgway; Ming Liang; Christian Schwab; Suvrath Mahadevan

doi:10.1117/12.2629020

The NEID Port Adapter at WIYN: on-sky fast guiding performance

Dan Li^*, Sarah E. Logsdon, William McBride, Jayadev Rajagopal, Marsha J. Wolf, Jeffrey W. Percival, Kurt P. Jaehnig, Michael P. Smith, Qian Gong, Michael W. McElwain, Heidi Schweiker, Eli Golub, Jesus Higuera, Jessica Klusmeyer, Emily Hunting, Erik Timmermann, Mark Everett, Wilson Liu, Susan Ridgway, Ming LiangChristian Schwab, Suvrath Mahadevan

^*Corresponding author for this work

Australian Astronomical Optics

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

3 Citations (Scopus)

Abstract

NEID (NN-explore Exoplanet Investigations with Doppler spectroscopy) is an optical, fiber-fed spectrometer installed on the WIYN 3.5m Telescope. The radial velocity precision that NEID is expected to reach requires the stellar jitter (i.e., the slight irregular movement of the stellar image induced by atmospheric turbulence, wind-shake, etc.) to be controlled within 0.05 arc-seconds 90% of the time in nominal observing conditions (i.e., 0.8-arcsecond seeing and mild winds). To achieve that, the NEID Port Adapter incorporates a fast, first-order wavefront correction system, which implements an Electron-Multiplying CCD camera and a tip/tilt piezo stage to capture and stabilize the stellar image. Here, we use on-sky data to demonstrate the performance of this system under various observing conditions.

Original language	English
Title of host publication	Ground-based and Airborne Instrumentation for Astronomy IX
Editors	Christopher J. Evans, Julia J. Bryant, Kentaro Motohara
Place of Publication	Washington, DC
Publisher	SPIE
Pages	1-9
Number of pages	9
ISBN (Electronic)	9781510653504
ISBN (Print)	9781510653498
DOIs	https://doi.org/10.1117/12.2629020
Publication status	Published - 2022
Event	Conference on Ground-based and Airborne Instrumentation for Astronomy IX - Montreal, Canada Duration: 17 Jul 2022 → 22 Jul 2022

Publication series

Name	Proceedings of SPIE
Publisher	SPIE
Volume	12184
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Conference on Ground-based and Airborne Instrumentation for Astronomy IX
Country/Territory	Canada
City	Montreal
Period	17/07/22 → 22/07/22

Keywords

Optical spectrometers
Fiber-fed spectrometers
Wavefront Correction
Radial-velocity techiniques
Extrasolar Planets

Access to Document

10.1117/12.2629020

Cite this

Li, D., Logsdon, S. E., McBride, W., Rajagopal, J., Wolf, M. J., Percival, J. W., Jaehnig, K. P., Smith, M. P., Gong, Q., McElwain, M. W., Schweiker, H., Golub, E., Higuera, J., Klusmeyer, J., Hunting, E., Timmermann, E., Everett, M., Liu, W., Ridgway, S., ... Mahadevan, S. (2022). The NEID Port Adapter at WIYN: on-sky fast guiding performance. In C. J. Evans, J. J. Bryant, & K. Motohara (Eds.), Ground-based and Airborne Instrumentation for Astronomy IX (pp. 1-9). Article 121844O (Proceedings of SPIE; Vol. 12184). SPIE. https://doi.org/10.1117/12.2629020

@inproceedings{65271bb75f4442c58527bfc936e84f1b,

title = "The NEID Port Adapter at WIYN: on-sky fast guiding performance",

abstract = "NEID (NN-explore Exoplanet Investigations with Doppler spectroscopy) is an optical, fiber-fed spectrometer installed on the WIYN 3.5m Telescope. The radial velocity precision that NEID is expected to reach requires the stellar jitter (i.e., the slight irregular movement of the stellar image induced by atmospheric turbulence, wind-shake, etc.) to be controlled within 0.05 arc-seconds 90% of the time in nominal observing conditions (i.e., 0.8-arcsecond seeing and mild winds). To achieve that, the NEID Port Adapter incorporates a fast, first-order wavefront correction system, which implements an Electron-Multiplying CCD camera and a tip/tilt piezo stage to capture and stabilize the stellar image. Here, we use on-sky data to demonstrate the performance of this system under various observing conditions.",

keywords = "Optical spectrometers, Fiber-fed spectrometers, Wavefront Correction, Radial-velocity techiniques, Extrasolar Planets",

author = "Dan Li and Logsdon, {Sarah E.} and William McBride and Jayadev Rajagopal and Wolf, {Marsha J.} and Percival, {Jeffrey W.} and Jaehnig, {Kurt P.} and Smith, {Michael P.} and Qian Gong and McElwain, {Michael W.} and Heidi Schweiker and Eli Golub and Jesus Higuera and Jessica Klusmeyer and Emily Hunting and Erik Timmermann and Mark Everett and Wilson Liu and Susan Ridgway and Ming Liang and Christian Schwab and Suvrath Mahadevan",

year = "2022",

doi = "10.1117/12.2629020",

language = "English",

isbn = "9781510653498",

series = "Proceedings of SPIE",

publisher = "SPIE",

pages = "1--9",

editor = "Evans, {Christopher J.} and Bryant, {Julia J.} and Kentaro Motohara",

booktitle = "Ground-based and Airborne Instrumentation for Astronomy IX",

address = "United States",

note = "Conference on Ground-based and Airborne Instrumentation for Astronomy IX ; Conference date: 17-07-2022 Through 22-07-2022",

}

Li, D, Logsdon, SE, McBride, W, Rajagopal, J, Wolf, MJ, Percival, JW, Jaehnig, KP, Smith, MP, Gong, Q, McElwain, MW, Schweiker, H, Golub, E, Higuera, J, Klusmeyer, J, Hunting, E, Timmermann, E, Everett, M, Liu, W, Ridgway, S, Liang, M, Schwab, C & Mahadevan, S 2022, The NEID Port Adapter at WIYN: on-sky fast guiding performance. in CJ Evans, JJ Bryant & K Motohara (eds), Ground-based and Airborne Instrumentation for Astronomy IX., 121844O, Proceedings of SPIE, vol. 12184, SPIE, Washington, DC, pp. 1-9, Conference on Ground-based and Airborne Instrumentation for Astronomy IX, Montreal, Canada, 17/07/22. https://doi.org/10.1117/12.2629020

The NEID Port Adapter at WIYN: on-sky fast guiding performance. / Li, Dan; Logsdon, Sarah E.; McBride, William et al.
Ground-based and Airborne Instrumentation for Astronomy IX. ed. / Christopher J. Evans; Julia J. Bryant; Kentaro Motohara. Washington, DC: SPIE, 2022. p. 1-9 121844O (Proceedings of SPIE; Vol. 12184).

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

TY - GEN

T1 - The NEID Port Adapter at WIYN

T2 - Conference on Ground-based and Airborne Instrumentation for Astronomy IX

AU - Li, Dan

AU - Logsdon, Sarah E.

AU - McBride, William

AU - Rajagopal, Jayadev

AU - Wolf, Marsha J.

AU - Percival, Jeffrey W.

AU - Jaehnig, Kurt P.

AU - Smith, Michael P.

AU - Gong, Qian

AU - McElwain, Michael W.

AU - Schweiker, Heidi

AU - Golub, Eli

AU - Higuera, Jesus

AU - Klusmeyer, Jessica

AU - Hunting, Emily

AU - Timmermann, Erik

AU - Everett, Mark

AU - Liu, Wilson

AU - Ridgway, Susan

AU - Liang, Ming

AU - Schwab, Christian

AU - Mahadevan, Suvrath

PY - 2022

Y1 - 2022

N2 - NEID (NN-explore Exoplanet Investigations with Doppler spectroscopy) is an optical, fiber-fed spectrometer installed on the WIYN 3.5m Telescope. The radial velocity precision that NEID is expected to reach requires the stellar jitter (i.e., the slight irregular movement of the stellar image induced by atmospheric turbulence, wind-shake, etc.) to be controlled within 0.05 arc-seconds 90% of the time in nominal observing conditions (i.e., 0.8-arcsecond seeing and mild winds). To achieve that, the NEID Port Adapter incorporates a fast, first-order wavefront correction system, which implements an Electron-Multiplying CCD camera and a tip/tilt piezo stage to capture and stabilize the stellar image. Here, we use on-sky data to demonstrate the performance of this system under various observing conditions.

AB - NEID (NN-explore Exoplanet Investigations with Doppler spectroscopy) is an optical, fiber-fed spectrometer installed on the WIYN 3.5m Telescope. The radial velocity precision that NEID is expected to reach requires the stellar jitter (i.e., the slight irregular movement of the stellar image induced by atmospheric turbulence, wind-shake, etc.) to be controlled within 0.05 arc-seconds 90% of the time in nominal observing conditions (i.e., 0.8-arcsecond seeing and mild winds). To achieve that, the NEID Port Adapter incorporates a fast, first-order wavefront correction system, which implements an Electron-Multiplying CCD camera and a tip/tilt piezo stage to capture and stabilize the stellar image. Here, we use on-sky data to demonstrate the performance of this system under various observing conditions.

KW - Optical spectrometers

KW - Fiber-fed spectrometers

KW - Wavefront Correction

KW - Radial-velocity techiniques

KW - Extrasolar Planets

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U2 - 10.1117/12.2629020

DO - 10.1117/12.2629020

M3 - Conference proceeding contribution

SN - 9781510653498

T3 - Proceedings of SPIE

SP - 1

EP - 9

BT - Ground-based and Airborne Instrumentation for Astronomy IX

A2 - Evans, Christopher J.

A2 - Bryant, Julia J.

A2 - Motohara, Kentaro

PB - SPIE

CY - Washington, DC

Y2 - 17 July 2022 through 22 July 2022

ER -

The NEID Port Adapter at WIYN: on-sky fast guiding performance

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Keywords

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