MARVEL: extracting high-precision radial velocities of exoplanet hosts

N. Jannsen; D. Seynaeve; J. De Ridder; J. Stürmer; J. Pember; C. Schwab; L. A. Buchhave; G. Raskin; B. Vandenbussche; H. Sana; A. Tkachenko; P. Royer; W. De Meester; H. Van Winckel; I. Ribas

doi:10.1117/12.2630748

MARVEL: extracting high-precision radial velocities of exoplanet hosts

N. Jannsen^*, D. Seynaeve, J. De Ridder, J. Stürmer, J. Pember, C. Schwab, L. A. Buchhave, G. Raskin, B. Vandenbussche, H. Sana, A. Tkachenko, P. Royer, W. De Meester, H. Van Winckel, I. Ribas

^*Corresponding author for this work

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

Abstract

The future ESA space mission PLATO aims to detect thousands of exoplanets, including Earth-like planets, and constrain their radius and mean density. To achieve this goal, the space based photometric observations are not enough but need to be complemented by ground-based observations to measure the Radial Velocity (RV) of the exoplanet host stars. MARVEL is such a facility consisting of four 80 cm telescope linked through optical fibers to a single high-resolution echelle spectrograph, designed for high-precision RV measurements with a uncertainty of ∼1 m s^-1. MARVEL is build by a consortium led by the KU Leuven with contributions from the UK, Austria, Australia, Sweden, Denmark, and Spain, and will be commissioned in 2023. To reach such high RV precision, not only ultra-stable hardware is currently being developed, but also a state-of-The-Art data processing pipeline for which we present the first results in this poster.

Original language	English
Title of host publication	Observatory Operations
Subtitle of host publication	Strategies, Processes, and Systems IX
Editors	David S. Adler, Robert L. Seaman, Chris R. Benn
Place of Publication	Bellingham, Washington
Publisher	SPIE
Pages	121861U-1-121861U-11
Number of pages	11
ISBN (Electronic)	9781510653542
ISBN (Print)	9781510653535
DOIs	https://doi.org/10.1117/12.2630748
Publication status	Published - 2022
Event	Observatory Operations: Strategies, Processes, and Systems IX 2022 - Montreal, Canada Duration: 17 Jul 2022 → 22 Jul 2022

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	12186
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Observatory Operations: Strategies, Processes, and Systems IX 2022
Country/Territory	Canada
City	Montreal
Period	17/07/22 → 22/07/22

Keywords

Exoplanets
Pipeline
Radial velocity
Simulations
Spectrograph
Telescopes

Access to Document

10.1117/12.2630748

Cite this

Jannsen, N., Seynaeve, D., De Ridder, J., Stürmer, J., Pember, J., Schwab, C., Buchhave, L. A., Raskin, G., Vandenbussche, B., Sana, H., Tkachenko, A., Royer, P., De Meester, W., Van Winckel, H., & Ribas, I. (2022). MARVEL: extracting high-precision radial velocities of exoplanet hosts. In D. S. Adler, R. L. Seaman, & C. R. Benn (Eds.), Observatory Operations: Strategies, Processes, and Systems IX (pp. 121861U-1-121861U-11). [121861U] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12186). SPIE. https://doi.org/10.1117/12.2630748

Jannsen, N. ; Seynaeve, D. ; De Ridder, J. et al. / MARVEL : extracting high-precision radial velocities of exoplanet hosts. Observatory Operations: Strategies, Processes, and Systems IX. editor / David S. Adler ; Robert L. Seaman ; Chris R. Benn. Bellingham, Washington : SPIE, 2022. pp. 121861U-1-121861U-11 (Proceedings of SPIE - The International Society for Optical Engineering).

@inproceedings{2375a60cb48742bba22099cd3167c9c5,

title = "MARVEL: extracting high-precision radial velocities of exoplanet hosts",

abstract = "The future ESA space mission PLATO aims to detect thousands of exoplanets, including Earth-like planets, and constrain their radius and mean density. To achieve this goal, the space based photometric observations are not enough but need to be complemented by ground-based observations to measure the Radial Velocity (RV) of the exoplanet host stars. MARVEL is such a facility consisting of four 80 cm telescope linked through optical fibers to a single high-resolution echelle spectrograph, designed for high-precision RV measurements with a uncertainty of ∼1 m s-1. MARVEL is build by a consortium led by the KU Leuven with contributions from the UK, Austria, Australia, Sweden, Denmark, and Spain, and will be commissioned in 2023. To reach such high RV precision, not only ultra-stable hardware is currently being developed, but also a state-of-The-Art data processing pipeline for which we present the first results in this poster. ",

keywords = "Exoplanets, Pipeline, Radial velocity, Simulations, Spectrograph, Telescopes",

author = "N. Jannsen and D. Seynaeve and {De Ridder}, J. and J. St{\"u}rmer and J. Pember and C. Schwab and Buchhave, {L. A.} and G. Raskin and B. Vandenbussche and H. Sana and A. Tkachenko and P. Royer and {De Meester}, W. and {Van Winckel}, H. and I. Ribas",

year = "2022",

doi = "10.1117/12.2630748",

language = "English",

isbn = "9781510653535",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

pages = "121861U--1--121861U--11",

editor = "Adler, {David S.} and Seaman, {Robert L.} and Benn, {Chris R.}",

booktitle = "Observatory Operations",

address = "United States",

note = "Observatory Operations: Strategies, Processes, and Systems IX 2022 ; Conference date: 17-07-2022 Through 22-07-2022",

}

Jannsen, N, Seynaeve, D, De Ridder, J, Stürmer, J, Pember, J , Schwab, C, Buchhave, LA, Raskin, G, Vandenbussche, B, Sana, H, Tkachenko, A, Royer, P, De Meester, W, Van Winckel, H & Ribas, I 2022, MARVEL: extracting high-precision radial velocities of exoplanet hosts. in DS Adler, RL Seaman & CR Benn (eds), Observatory Operations: Strategies, Processes, and Systems IX., 121861U, Proceedings of SPIE - The International Society for Optical Engineering, vol. 12186, SPIE, Bellingham, Washington, pp. 121861U-1-121861U-11, Observatory Operations: Strategies, Processes, and Systems IX 2022, Montreal, Canada, 17/07/22. https://doi.org/10.1117/12.2630748

MARVEL: extracting high-precision radial velocities of exoplanet hosts. / Jannsen, N.; Seynaeve, D.; De Ridder, J. et al.
Observatory Operations: Strategies, Processes, and Systems IX. ed. / David S. Adler; Robert L. Seaman; Chris R. Benn. Bellingham, Washington: SPIE, 2022. p. 121861U-1-121861U-11 121861U (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12186).

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

TY - GEN

T1 - MARVEL

T2 - Observatory Operations: Strategies, Processes, and Systems IX 2022

AU - Jannsen, N.

AU - Seynaeve, D.

AU - De Ridder, J.

AU - Stürmer, J.

AU - Pember, J.

AU - Schwab, C.

AU - Buchhave, L. A.

AU - Raskin, G.

AU - Vandenbussche, B.

AU - Sana, H.

AU - Tkachenko, A.

AU - Royer, P.

AU - De Meester, W.

AU - Van Winckel, H.

AU - Ribas, I.

PY - 2022

Y1 - 2022

N2 - The future ESA space mission PLATO aims to detect thousands of exoplanets, including Earth-like planets, and constrain their radius and mean density. To achieve this goal, the space based photometric observations are not enough but need to be complemented by ground-based observations to measure the Radial Velocity (RV) of the exoplanet host stars. MARVEL is such a facility consisting of four 80 cm telescope linked through optical fibers to a single high-resolution echelle spectrograph, designed for high-precision RV measurements with a uncertainty of ∼1 m s-1. MARVEL is build by a consortium led by the KU Leuven with contributions from the UK, Austria, Australia, Sweden, Denmark, and Spain, and will be commissioned in 2023. To reach such high RV precision, not only ultra-stable hardware is currently being developed, but also a state-of-The-Art data processing pipeline for which we present the first results in this poster.

AB - The future ESA space mission PLATO aims to detect thousands of exoplanets, including Earth-like planets, and constrain their radius and mean density. To achieve this goal, the space based photometric observations are not enough but need to be complemented by ground-based observations to measure the Radial Velocity (RV) of the exoplanet host stars. MARVEL is such a facility consisting of four 80 cm telescope linked through optical fibers to a single high-resolution echelle spectrograph, designed for high-precision RV measurements with a uncertainty of ∼1 m s-1. MARVEL is build by a consortium led by the KU Leuven with contributions from the UK, Austria, Australia, Sweden, Denmark, and Spain, and will be commissioned in 2023. To reach such high RV precision, not only ultra-stable hardware is currently being developed, but also a state-of-The-Art data processing pipeline for which we present the first results in this poster.

KW - Exoplanets

KW - Pipeline

KW - Radial velocity

KW - Simulations

KW - Spectrograph

KW - Telescopes

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U2 - 10.1117/12.2630748

DO - 10.1117/12.2630748

M3 - Conference proceeding contribution

AN - SCOPUS:85140073498

SN - 9781510653535

T3 - Proceedings of SPIE - The International Society for Optical Engineering

SP - 121861U-1-121861U-11

BT - Observatory Operations

A2 - Adler, David S.

A2 - Seaman, Robert L.

A2 - Benn, Chris R.

PB - SPIE

CY - Bellingham, Washington

Y2 - 17 July 2022 through 22 July 2022

ER -

Jannsen N, Seynaeve D, De Ridder J, Stürmer J, Pember J , Schwab C et al. MARVEL: extracting high-precision radial velocities of exoplanet hosts. In Adler DS, Seaman RL, Benn CR, editors, Observatory Operations: Strategies, Processes, and Systems IX. Bellingham, Washington: SPIE. 2022. p. 121861U-1-121861U-11. 121861U. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2630748

MARVEL: extracting high-precision radial velocities of exoplanet hosts

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Keywords

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