The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets

S. Lacour; J. J. Wang; M. Nowak; L. Pueyo; F. Eisenhauer; A. M. Lagrange; P. Mollière; R. Abuter; A. Amorin; R. Asensio-Torres; M. Bauböck; M. Benisty; J. P. Berger; H. Beust; S. Blunt; A. Boccaletti; A. Bohn; M. Bonnefoy; H. Bonnet; W. Brandner; F. Cantalloube; P. Caselli; B. Charnay; G. Chauvin; E. Choquet; V. Christiaens; Y. Clénet; A. Cridland; P. T. De Zeeuw; R. Dembet; J. Dexter; A. Drescher; G. Duvert; F. Gao; P. Garcia; R. Garcia Lopez; T. Gardner; E. Gendron; R. Genzel; S. Gillessen; J. H. Girard; X. Haubois; G. Heißel; T. Henning; S. Hinkley; S. Hippler; M. Horrobin; M. Houllé; Z. Hubert; A. Jiménez-Rosales; L. Jocou; J. Kammerer; M. Keppler; P. Kervella; L. Kreidberg; V. Lapeyrère; J. B. Le Bouquin; P. Léna; D. Lutz; A. L. Maire; A. Mérand; J. D. Monnier; D. Mouillet; A. Muller; E. Nasedkin; T. Ott; G. P.P.L. Otten; C. Paladini; T. Paumard; K. Perraut; G. Perrin; O. Pfuhl; J. Rameau; L. Rodet; G. Rodriguez-Coira; G. Rousset; J. Shangguan; T. Shimizu; J. Stadler; O. Straub; C. Straubmeier; E. Sturm; T. Stolker; E. F. Van Dishoeck; A. Vigan; F. Vincent; S. D. Von Fellenberg; K. Ward-Duong; F. Widmann; E. Wieprecht; E. Wiezorrek; J. Woillez

doi:10.1117/12.2561667

The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets

S. Lacour, J. J. Wang, M. Nowak, L. Pueyo, F. Eisenhauer, A. M. Lagrange, P. Mollière, R. Abuter, A. Amorin, R. Asensio-Torres, M. Bauböck, M. Benisty, J. P. Berger, H. Beust, S. Blunt, A. Boccaletti, A. Bohn, M. Bonnefoy, H. Bonnet, W. BrandnerF. Cantalloube, P. Caselli, B. Charnay, G. Chauvin, E. Choquet, V. Christiaens, Y. Clénet, A. Cridland, P. T. De Zeeuw, R. Dembet, J. Dexter, A. Drescher, G. Duvert, F. Gao, P. Garcia, R. Garcia Lopez, T. Gardner, E. Gendron, R. Genzel, S. Gillessen, J. H. Girard, X. Haubois, G. Heißel, T. Henning, S. Hinkley, S. Hippler, M. Horrobin, M. Houllé, Z. Hubert, A. Jiménez-Rosales, L. Jocou, J. Kammerer, M. Keppler, P. Kervella, L. Kreidberg, V. Lapeyrère, J. B. Le Bouquin, P. Léna, D. Lutz, A. L. Maire, A. Mérand, J. D. Monnier, D. Mouillet, A. Muller, E. Nasedkin, T. Ott, G. P.P.L. Otten, C. Paladini, T. Paumard, K. Perraut, G. Perrin, O. Pfuhl, J. Rameau, L. Rodet, G. Rodriguez-Coira, G. Rousset, J. Shangguan, T. Shimizu, J. Stadler, O. Straub, C. Straubmeier, E. Sturm, T. Stolker, E. F. Van Dishoeck, A. Vigan, F. Vincent, S. D. Von Fellenberg, K. Ward-Duong, F. Widmann, E. Wieprecht, E. Wiezorrek, J. Woillez

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

9 Citations (Scopus)

Abstract

Combining adaptive optics and interferometric observations results in a considerable contrast gain compared to single-telescope, extreme AO systems. Taking advantage of this, the ExoGRAVITY project is a survey of known young giant exoplanets located in the range of 0.1"to 2"from their stars. The observations provide astrometric data of unprecedented accuracy, being crucial for refining the orbital parameters of planets and illuminating their dynamical histories. Furthermore, GRAVITY will measure non-Keplerian perturbations due to planet-planet interactions in multi-planet systems and measure dynamical masses. Over time, repetitive observations of the exoplanets at medium resolution (R = 500) will provide a catalogue of K-band spectra of unprecedented quality, for a number of exoplanets. The K-band has the unique properties that it contains many molecular signatures (CO, H2O, CH4, CO2). This allows constraining precisely surface gravity, metallicity, and temperature, if used in conjunction with self-consistent models like Exo-REM. Further, we will use the parameter-retrieval algorithm petitRADTRANS to constrain the C/O ratio of the planets. Ultimately, we plan to produce the first C/O survey of exoplanets, kick-starting the difficult process of linking planetary formation with measured atomic abundances.

Original language	English
Title of host publication	Optical and Infrared Interferometry and Imaging VII
Editors	Peter G. Tuthill, Antoine Merand, Stephanie Sallum
Publisher	SPIE
ISBN (Electronic)	9781510636798
DOIs	https://doi.org/10.1117/12.2561667
Publication status	Published - 2020
Event	Optical and Infrared Interferometry and Imaging VII 2020 - Virtual, Online, United States Duration: 14 Dec 2020 → 22 Dec 2020

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11446
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Optical and Infrared Interferometry and Imaging VII 2020
Country/Territory	United States
City	Virtual, Online
Period	14/12/20 → 22/12/20

Access to Document

10.1117/12.2561667

Cite this

Lacour, S., Wang, J. J., Nowak, M., Pueyo, L., Eisenhauer, F., Lagrange, A. M., Mollière, P., Abuter, R., Amorin, A., Asensio-Torres, R., Bauböck, M., Benisty, M., Berger, J. P., Beust, H., Blunt, S., Boccaletti, A., Bohn, A., Bonnefoy, M., Bonnet, H., ... Woillez, J. (2020). The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets. In P. G. Tuthill, A. Merand, & S. Sallum (Eds.), Optical and Infrared Interferometry and Imaging VII Article 114460O (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11446). SPIE. https://doi.org/10.1117/12.2561667

@inproceedings{0d525b18b71f4f0fa25c38f06776fac1,

title = "The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets",

abstract = "Combining adaptive optics and interferometric observations results in a considerable contrast gain compared to single-telescope, extreme AO systems. Taking advantage of this, the ExoGRAVITY project is a survey of known young giant exoplanets located in the range of 0.1{"}to 2{"}from their stars. The observations provide astrometric data of unprecedented accuracy, being crucial for refining the orbital parameters of planets and illuminating their dynamical histories. Furthermore, GRAVITY will measure non-Keplerian perturbations due to planet-planet interactions in multi-planet systems and measure dynamical masses. Over time, repetitive observations of the exoplanets at medium resolution (R = 500) will provide a catalogue of K-band spectra of unprecedented quality, for a number of exoplanets. The K-band has the unique properties that it contains many molecular signatures (CO, H2O, CH4, CO2). This allows constraining precisely surface gravity, metallicity, and temperature, if used in conjunction with self-consistent models like Exo-REM. Further, we will use the parameter-retrieval algorithm petitRADTRANS to constrain the C/O ratio of the planets. Ultimately, we plan to produce the first C/O survey of exoplanets, kick-starting the difficult process of linking planetary formation with measured atomic abundances.",

keywords = "Exoplanets, Optical interferometry, Planet formation",

author = "S. Lacour and Wang, {J. J.} and M. Nowak and L. Pueyo and F. Eisenhauer and Lagrange, {A. M.} and P. Molli{\`e}re and R. Abuter and A. Amorin and R. Asensio-Torres and M. Baub{\"o}ck and M. Benisty and Berger, {J. P.} and H. Beust and S. Blunt and A. Boccaletti and A. Bohn and M. Bonnefoy and H. Bonnet and W. Brandner and F. Cantalloube and P. Caselli and B. Charnay and G. Chauvin and E. Choquet and V. Christiaens and Y. Cl{\'e}net and A. Cridland and {De Zeeuw}, {P. T.} and R. Dembet and J. Dexter and A. Drescher and G. Duvert and F. Gao and P. Garcia and {Garcia Lopez}, R. and T. Gardner and E. Gendron and R. Genzel and S. Gillessen and Girard, {J. H.} and X. Haubois and G. Hei{\ss}el and T. Henning and S. Hinkley and S. Hippler and M. Horrobin and M. Houll{\'e} and Z. Hubert and A. Jim{\'e}nez-Rosales and L. Jocou and J. Kammerer and M. Keppler and P. Kervella and L. Kreidberg and V. Lapeyr{\`e}re and {Le Bouquin}, {J. B.} and P. L{\'e}na and D. Lutz and Maire, {A. L.} and A. M{\'e}rand and Monnier, {J. D.} and D. Mouillet and A. Muller and E. Nasedkin and T. Ott and Otten, {G. P.P.L.} and C. Paladini and T. Paumard and K. Perraut and G. Perrin and O. Pfuhl and J. Rameau and L. Rodet and G. Rodriguez-Coira and G. Rousset and J. Shangguan and T. Shimizu and J. Stadler and O. Straub and C. Straubmeier and E. Sturm and T. Stolker and {Van Dishoeck}, {E. F.} and A. Vigan and F. Vincent and {Von Fellenberg}, {S. D.} and K. Ward-Duong and F. Widmann and E. Wieprecht and E. Wiezorrek and J. Woillez",

note = "Publisher Copyright: {\textcopyright} COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.; Optical and Infrared Interferometry and Imaging VII 2020 ; Conference date: 14-12-2020 Through 22-12-2020",

year = "2020",

doi = "10.1117/12.2561667",

language = "English",

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

publisher = "SPIE",

editor = "Tuthill, {Peter G.} and Antoine Merand and Stephanie Sallum",

booktitle = "Optical and Infrared Interferometry and Imaging VII",

address = "United States",

}

Lacour, S, Wang, JJ, Nowak, M, Pueyo, L, Eisenhauer, F, Lagrange, AM, Mollière, P, Abuter, R, Amorin, A, Asensio-Torres, R, Bauböck, M, Benisty, M, Berger, JP, Beust, H, Blunt, S, Boccaletti, A, Bohn, A, Bonnefoy, M, Bonnet, H, Brandner, W, Cantalloube, F, Caselli, P, Charnay, B, Chauvin, G, Choquet, E, Christiaens, V, Clénet, Y, Cridland, A, De Zeeuw, PT, Dembet, R, Dexter, J, Drescher, A, Duvert, G, Gao, F, Garcia, P, Garcia Lopez, R, Gardner, T, Gendron, E, Genzel, R, Gillessen, S, Girard, JH, Haubois, X, Heißel, G, Henning, T, Hinkley, S, Hippler, S, Horrobin, M, Houllé, M, Hubert, Z, Jiménez-Rosales, A, Jocou, L, Kammerer, J, Keppler, M, Kervella, P, Kreidberg, L, Lapeyrère, V, Le Bouquin, JB, Léna, P, Lutz, D, Maire, AL, Mérand, A, Monnier, JD, Mouillet, D, Muller, A, Nasedkin, E, Ott, T, Otten, GPPL, Paladini, C, Paumard, T, Perraut, K, Perrin, G, Pfuhl, O, Rameau, J, Rodet, L, Rodriguez-Coira, G, Rousset, G, Shangguan, J, Shimizu, T, Stadler, J, Straub, O, Straubmeier, C, Sturm, E, Stolker, T, Van Dishoeck, EF, Vigan, A, Vincent, F, Von Fellenberg, SD, Ward-Duong, K, Widmann, F, Wieprecht, E, Wiezorrek, E & Woillez, J 2020, The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets. in PG Tuthill, A Merand & S Sallum (eds), Optical and Infrared Interferometry and Imaging VII., 114460O, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11446, SPIE, Optical and Infrared Interferometry and Imaging VII 2020, Virtual, Online, United States, 14/12/20. https://doi.org/10.1117/12.2561667

The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets. / Lacour, S.; Wang, J. J.; Nowak, M. et al.
Optical and Infrared Interferometry and Imaging VII. ed. / Peter G. Tuthill; Antoine Merand; Stephanie Sallum. SPIE, 2020. 114460O (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11446).

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

TY - GEN

T1 - The ExoGRAVITY project

T2 - Optical and Infrared Interferometry and Imaging VII 2020

AU - Lacour, S.

AU - Wang, J. J.

AU - Nowak, M.

AU - Pueyo, L.

AU - Eisenhauer, F.

AU - Lagrange, A. M.

AU - Mollière, P.

AU - Abuter, R.

AU - Amorin, A.

AU - Asensio-Torres, R.

AU - Bauböck, M.

AU - Benisty, M.

AU - Berger, J. P.

AU - Beust, H.

AU - Blunt, S.

AU - Boccaletti, A.

AU - Bohn, A.

AU - Bonnefoy, M.

AU - Bonnet, H.

AU - Brandner, W.

AU - Cantalloube, F.

AU - Caselli, P.

AU - Charnay, B.

AU - Chauvin, G.

AU - Choquet, E.

AU - Christiaens, V.

AU - Clénet, Y.

AU - Cridland, A.

AU - De Zeeuw, P. T.

AU - Dembet, R.

AU - Dexter, J.

AU - Drescher, A.

AU - Duvert, G.

AU - Gao, F.

AU - Garcia, P.

AU - Garcia Lopez, R.

AU - Gardner, T.

AU - Gendron, E.

AU - Genzel, R.

AU - Gillessen, S.

AU - Girard, J. H.

AU - Haubois, X.

AU - Heißel, G.

AU - Henning, T.

AU - Hinkley, S.

AU - Hippler, S.

AU - Horrobin, M.

AU - Houllé, M.

AU - Hubert, Z.

AU - Jiménez-Rosales, A.

AU - Jocou, L.

AU - Kammerer, J.

AU - Keppler, M.

AU - Kervella, P.

AU - Kreidberg, L.

AU - Lapeyrère, V.

AU - Le Bouquin, J. B.

AU - Léna, P.

AU - Lutz, D.

AU - Maire, A. L.

AU - Mérand, A.

AU - Monnier, J. D.

AU - Mouillet, D.

AU - Muller, A.

AU - Nasedkin, E.

AU - Ott, T.

AU - Otten, G. P.P.L.

AU - Paladini, C.

AU - Paumard, T.

AU - Perraut, K.

AU - Perrin, G.

AU - Pfuhl, O.

AU - Rameau, J.

AU - Rodet, L.

AU - Rodriguez-Coira, G.

AU - Rousset, G.

AU - Shangguan, J.

AU - Shimizu, T.

AU - Stadler, J.

AU - Straub, O.

AU - Straubmeier, C.

AU - Sturm, E.

AU - Stolker, T.

AU - Van Dishoeck, E. F.

AU - Vigan, A.

AU - Vincent, F.

AU - Von Fellenberg, S. D.

AU - Ward-Duong, K.

AU - Widmann, F.

AU - Wieprecht, E.

AU - Wiezorrek, E.

AU - Woillez, J.

PY - 2020

Y1 - 2020

N2 - Combining adaptive optics and interferometric observations results in a considerable contrast gain compared to single-telescope, extreme AO systems. Taking advantage of this, the ExoGRAVITY project is a survey of known young giant exoplanets located in the range of 0.1"to 2"from their stars. The observations provide astrometric data of unprecedented accuracy, being crucial for refining the orbital parameters of planets and illuminating their dynamical histories. Furthermore, GRAVITY will measure non-Keplerian perturbations due to planet-planet interactions in multi-planet systems and measure dynamical masses. Over time, repetitive observations of the exoplanets at medium resolution (R = 500) will provide a catalogue of K-band spectra of unprecedented quality, for a number of exoplanets. The K-band has the unique properties that it contains many molecular signatures (CO, H2O, CH4, CO2). This allows constraining precisely surface gravity, metallicity, and temperature, if used in conjunction with self-consistent models like Exo-REM. Further, we will use the parameter-retrieval algorithm petitRADTRANS to constrain the C/O ratio of the planets. Ultimately, we plan to produce the first C/O survey of exoplanets, kick-starting the difficult process of linking planetary formation with measured atomic abundances.

AB - Combining adaptive optics and interferometric observations results in a considerable contrast gain compared to single-telescope, extreme AO systems. Taking advantage of this, the ExoGRAVITY project is a survey of known young giant exoplanets located in the range of 0.1"to 2"from their stars. The observations provide astrometric data of unprecedented accuracy, being crucial for refining the orbital parameters of planets and illuminating their dynamical histories. Furthermore, GRAVITY will measure non-Keplerian perturbations due to planet-planet interactions in multi-planet systems and measure dynamical masses. Over time, repetitive observations of the exoplanets at medium resolution (R = 500) will provide a catalogue of K-band spectra of unprecedented quality, for a number of exoplanets. The K-band has the unique properties that it contains many molecular signatures (CO, H2O, CH4, CO2). This allows constraining precisely surface gravity, metallicity, and temperature, if used in conjunction with self-consistent models like Exo-REM. Further, we will use the parameter-retrieval algorithm petitRADTRANS to constrain the C/O ratio of the planets. Ultimately, we plan to produce the first C/O survey of exoplanets, kick-starting the difficult process of linking planetary formation with measured atomic abundances.

KW - Exoplanets

KW - Optical interferometry

KW - Planet formation

UR - http://www.scopus.com/inward/record.url?scp=85099192724&partnerID=8YFLogxK

U2 - 10.1117/12.2561667

DO - 10.1117/12.2561667

M3 - Conference contribution

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

BT - Optical and Infrared Interferometry and Imaging VII

A2 - Tuthill, Peter G.

A2 - Merand, Antoine

A2 - Sallum, Stephanie

PB - SPIE

Y2 - 14 December 2020 through 22 December 2020

ER -

Lacour S, Wang JJ, Nowak M, Pueyo L, Eisenhauer F, Lagrange AM et al. The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets. In Tuthill PG, Merand A, Sallum S, editors, Optical and Infrared Interferometry and Imaging VII. SPIE. 2020. 114460O. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2561667

The ExoGRAVITY project: Using single mode interferometry to characterize exoplanets

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