Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets

Cyprien Lanthermann; Joris De Ridder; Hugues Sana; Pierre Royer; Denis Defrère; Gert Raskin; Bart Vandenbussche; Andrew Tkachenko; Christian Schwab; Hans Van Winckel

doi:10.1117/12.2562486

Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets

Cyprien Lanthermann^*, Joris De Ridder, Hugues Sana, Pierre Royer, Denis Defrère, Gert Raskin, Bart Vandenbussche, Andrew Tkachenko, Christian Schwab, Hans Van Winckel

^*Corresponding author for this work

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

Abstract

The space missions TESS and PLATO plan to double the number of 4000 exoplanets already discovered and will measure the size of thousands of exoplanets around the brightest stars in the sky, allowing ground-based radial velocity spectroscopy follow-up to determine the orbit and mass of the detected planets. The new facility we are developing, MARVEL (Raskin et al. this conference¹), will enable the ground-based follow-up of large numbers of exoplanet detections expected from TESS and PLATO, which cannot be carried out only by the current facilities that achieve the necessary radial velocity accuracy of 1 ms^-1 or less. This paper presents the MARVEL observation strategy and performance analysis based on predicted PLATO transit detection yield simulations. The resulting observation scenario baseline will help in the instrument design choices and demonstrate the effectiveness of MARVEL as a TESS and PLATO science enabling facility.

Original language	English
Title of host publication	Observatory Operations
Subtitle of host publication	Strategies, Processes, and Systems VIII
Editors	David S. Adler, Robert L. Seaman, Chris R. Benn
Place of Publication	Bellingham, Washington
Publisher	SPIE
Pages	1-7
Number of pages	7
ISBN (Electronic)	9781510636866
ISBN (Print)	9781510636859
DOIs	https://doi.org/10.1117/12.2562486
Publication status	Published - 13 Dec 2020
Event	Observatory Operations: Strategies, Processes, and Systems VIII 2020 - Virtual, Online, United States Duration: 14 Dec 2020 → 22 Dec 2020

Publication series

Name	Proceedings of SPIE
Publisher	SPIE
Volume	11449
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Observatory Operations: Strategies, Processes, and Systems VIII 2020
Country/Territory	United States
City	Virtual, Online
Period	14/12/20 → 22/12/20

Keywords

Exoplanets
Observation strategy
Radial Velocity
Spectrograph
Telescopes

Access to Document

10.1117/12.2562486

Cite this

Lanthermann, C., De Ridder, J., Sana, H., Royer, P., Defrère, D., Raskin, G., Vandenbussche, B., Tkachenko, A., Schwab, C., & Van Winckel, H. (2020). Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets. In D. S. Adler, R. L. Seaman, & C. R. Benn (Eds.), Observatory Operations: Strategies, Processes, and Systems VIII (pp. 1-7). [1144913] (Proceedings of SPIE; Vol. 11449). SPIE. https://doi.org/10.1117/12.2562486

Lanthermann, Cyprien ; De Ridder, Joris ; Sana, Hugues ; Royer, Pierre ; Defrère, Denis ; Raskin, Gert ; Vandenbussche, Bart ; Tkachenko, Andrew ; Schwab, Christian ; Van Winckel, Hans. / Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets. Observatory Operations: Strategies, Processes, and Systems VIII. editor / David S. Adler ; Robert L. Seaman ; Chris R. Benn. Bellingham, Washington : SPIE, 2020. pp. 1-7 (Proceedings of SPIE).

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abstract = "The space missions TESS and PLATO plan to double the number of 4000 exoplanets already discovered and will measure the size of thousands of exoplanets around the brightest stars in the sky, allowing ground-based radial velocity spectroscopy follow-up to determine the orbit and mass of the detected planets. The new facility we are developing, MARVEL (Raskin et al. this conference1), will enable the ground-based follow-up of large numbers of exoplanet detections expected from TESS and PLATO, which cannot be carried out only by the current facilities that achieve the necessary radial velocity accuracy of 1 ms-1 or less. This paper presents the MARVEL observation strategy and performance analysis based on predicted PLATO transit detection yield simulations. The resulting observation scenario baseline will help in the instrument design choices and demonstrate the effectiveness of MARVEL as a TESS and PLATO science enabling facility. ",

keywords = "Exoplanets, Observation strategy, Radial Velocity, Spectrograph, Telescopes",

author = "Cyprien Lanthermann and {De Ridder}, Joris and Hugues Sana and Pierre Royer and Denis Defr{\`e}re and Gert Raskin and Bart Vandenbussche and Andrew Tkachenko and Christian Schwab and {Van Winckel}, Hans",

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Lanthermann, C, De Ridder, J, Sana, H, Royer, P, Defrère, D, Raskin, G, Vandenbussche, B, Tkachenko, A, Schwab, C & Van Winckel, H 2020, Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets. in DS Adler, RL Seaman & CR Benn (eds), Observatory Operations: Strategies, Processes, and Systems VIII., 1144913, Proceedings of SPIE, vol. 11449, SPIE, Bellingham, Washington, pp. 1-7, Observatory Operations: Strategies, Processes, and Systems VIII 2020, Virtual, Online, United States, 14/12/20. https://doi.org/10.1117/12.2562486

Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets. / Lanthermann, Cyprien; De Ridder, Joris; Sana, Hugues; Royer, Pierre; Defrère, Denis; Raskin, Gert; Vandenbussche, Bart; Tkachenko, Andrew; Schwab, Christian; Van Winckel, Hans.

Observatory Operations: Strategies, Processes, and Systems VIII. ed. / David S. Adler; Robert L. Seaman; Chris R. Benn. Bellingham, Washington : SPIE, 2020. p. 1-7 1144913 (Proceedings of SPIE; Vol. 11449).

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

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T1 - Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets

AU - Lanthermann, Cyprien

AU - De Ridder, Joris

AU - Sana, Hugues

AU - Royer, Pierre

AU - Defrère, Denis

AU - Raskin, Gert

AU - Vandenbussche, Bart

AU - Tkachenko, Andrew

AU - Schwab, Christian

AU - Van Winckel, Hans

PY - 2020/12/13

Y1 - 2020/12/13

N2 - The space missions TESS and PLATO plan to double the number of 4000 exoplanets already discovered and will measure the size of thousands of exoplanets around the brightest stars in the sky, allowing ground-based radial velocity spectroscopy follow-up to determine the orbit and mass of the detected planets. The new facility we are developing, MARVEL (Raskin et al. this conference1), will enable the ground-based follow-up of large numbers of exoplanet detections expected from TESS and PLATO, which cannot be carried out only by the current facilities that achieve the necessary radial velocity accuracy of 1 ms-1 or less. This paper presents the MARVEL observation strategy and performance analysis based on predicted PLATO transit detection yield simulations. The resulting observation scenario baseline will help in the instrument design choices and demonstrate the effectiveness of MARVEL as a TESS and PLATO science enabling facility.

AB - The space missions TESS and PLATO plan to double the number of 4000 exoplanets already discovered and will measure the size of thousands of exoplanets around the brightest stars in the sky, allowing ground-based radial velocity spectroscopy follow-up to determine the orbit and mass of the detected planets. The new facility we are developing, MARVEL (Raskin et al. this conference1), will enable the ground-based follow-up of large numbers of exoplanet detections expected from TESS and PLATO, which cannot be carried out only by the current facilities that achieve the necessary radial velocity accuracy of 1 ms-1 or less. This paper presents the MARVEL observation strategy and performance analysis based on predicted PLATO transit detection yield simulations. The resulting observation scenario baseline will help in the instrument design choices and demonstrate the effectiveness of MARVEL as a TESS and PLATO science enabling facility.

KW - Exoplanets

KW - Observation strategy

KW - Radial Velocity

KW - Spectrograph

KW - Telescopes

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DO - 10.1117/12.2562486

M3 - Conference proceeding contribution

AN - SCOPUS:85099288280

SN - 9781510636859

T3 - Proceedings of SPIE

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BT - Observatory Operations

A2 - Adler, David S.

A2 - Seaman, Robert L.

A2 - Benn, Chris R.

PB - SPIE

CY - Bellingham, Washington

T2 - Observatory Operations: Strategies, Processes, and Systems VIII 2020

Y2 - 14 December 2020 through 22 December 2020

ER -

Lanthermann C, De Ridder J, Sana H, Royer P, Defrère D, Raskin G et al. Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets. In Adler DS, Seaman RL, Benn CR, editors, Observatory Operations: Strategies, Processes, and Systems VIII. Bellingham, Washington: SPIE. 2020. p. 1-7. 1144913. (Proceedings of SPIE). https://doi.org/10.1117/12.2562486

Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets

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