Search Results - "Schuhler, N"

NAOMI: the adaptive optics system of the Auxiliary Telescopes of the VLTI by J, Woillez, A, Abad J, R, Abuter, E, Aller Carpentier, J, Alonso, L, Andolfato, P, Barriga, -P, Berger J, -L, Beuzit J, H, Bonnet, G, Bourdarot, P, Bourget, R, Brast, L, Caniguante, E, Cottalorda, P, Darré, B, Delabre, A, Delboulbé, F, Delplancke-Ströbele, R, Dembet, R, Donaldson, R, Dorn, J, Dupeyron, C, Dupuy, S, Egner, F, Eisenhauer, G, Fischer, C, Frank, E, Fuenteseca, P, Gitton, F, Gonté, T, Guerlet, S, Guieu, P, Gutierrez, P, Haguenauer, A, Haimerl, X, Haubois, C, Heritier, S, Huber, N, Hubin, P, Jolley, L, Jocou, -P, Kirchbauer J, J, Kolb, J, Kosmalski, P, Krempl, -B, Le Bouquin J, M, Le Louarn, P, Lilley, B, Lopez, Y, Magnard, S, Mclay, A, Meilland, A, Meister, A, Merand, T, Moulin, L, Pasquini, J, Paufique, I, Percheron, L, Pettazzi, O, Pfuhl, D, Phan, W, Pirani, J, Quentin, A, Rakich, R, Ridings, M, Riedel, J, Reyes, S, Rochat, G, Santos Tomás, C, Schmid, N, Schuhler, P, Shchekaturov, M, Seidel, C, Soenke, E, Stadler, C, Stephan, M, Suárez, M, Todorovic, G, Valdes, C, Verinaud, G, Zins, S, Zúñiga-Fernández

“…The tip-tilt stabilisation system of the 1.8 m Auxiliary Telescopes of the Very Large Telescope Interferometer was never dimensioned for robust fringe…”
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Plasma-deposited silicon oxide and silicon nitride films on poly(ethylene terephthalate): A multitechnique study of the interphase regions by da Silva Sobrinho, A. S., Schühler, N., Klemberg-Sapieha, J. E., Wertheimer, M. R., Andrews, M., Gujrathi, S. C.

“…The “interphase” region between the deposited layer [e.g., plasma-enhanced chemically vapor deposited (PECVD) SiO 2 or SiN] and the poly(ethylene…”
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Integrated Optics Evanescent Wave Surface Enhanced Raman Scattering (IO-EWSERS) of Mercaptopyridines on a Planar Optical Chemical Bench:  Binding of Hydrogen and Copper Ion by Baldwin, Jean, Schühler, Norbert, Butler, Ian S, Andrews, Mark P

“…Chemical interactions at molecular interfaces have been studied by integrated optics evanescent wave surface-enhanced Raman spectroscopy (IO-EWSERS). We…”
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Ion beam deposition of a-C:H on niobium and tungsten: in situ investigations using photoelectron spectroscopy by Schühler, N., Oelhafen, P.

“…a-C:H films have been deposited on tungsten and niobium by means of ion beam deposition, using methane as process gas. Step-by-step depositions have been…”
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Investigation of the Cu/BCB and Cu/PPQ interfaces by photoelectron spectroscopy by Schühler, N., Oelhafen, P.

“…Polyphenylquinoxaline (PPQ) and divinylsiloxane bis-benzocyclobutene (BCB) are of great technological interest concerning the fabrication of electronic…”
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GRAVITY for MATISSE -- Improving the MATISSE performance with the GRAVITY fringe tracker by Woillez, J, Petrov, R, Abuter, R, Allouche, F, Berio, P, Dembet, R, Eisenhauer, F, Frahm, R, Gonté, F, Haubois, X, Houllé, M, Jaffe, W, Lacour, S, Lagarde, S, Leftley, J, Lopez, B, Matter, A, Meilland, A, Millour, F, Nowak, M, Paladini, C, Rivinius, T, Salabert, D, Schuhler, N, Varga, J, Zins, G

“…A&A 688, A190 (2024) Context: MATISSE, the mid-infrared spectro-imaging instrument of VLTI, was designed to deliver its advertised performance when paired with…”
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Surface study of plasma- and UV-polymerized styrene films using scanning force microscopy and in-situ photoelectron spectroscopy by Schelz, S., Schühler, N., Richmond, T., Oelhafen, P.

“…Polymeric styrene films with thicknesses ranging from a few nanometres up to 3 μm have been prepared by various techniques, such as UV polymerization, spin…”
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Ion beam deposition of a-C:H on niobium and tungsten: in situ investigations using photoelectron spectroscoppy by Schuhler, N, Oelhafen, P

“…Amorphous C:H films were deposited on tungsten and niobium by means of ion beam deposition, using methane as process gas. Step-by-step depositions were…”
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High contrast at short separation with VLTI/GRAVITY: Bringing Gaia companions to light by Bouquin, J. -B. Le, Lacour, S, Bidot, A, Nowak, M, Maire, A. -L, Mouillet, D, Babusiaux, C, Abuter, R, Amorim, A, Balmer, W. O, Benisty, M, Beust, H, Bonnet, H, Bordoni, M. S, Bourdarot, G, Brandner, W, Cantalloube, F, Charnay, B, Chavez, A, Christiaens, V, Clénet, Y, Cridland, A, Davies, R, Defrère, D, Dembet, R, Dexter, J, Duvert, G, Gendron, E, Genzel, R, Girard, J. H, Gonte, F, Grant, S, Heißel, G, Henning, Th, Hönig, S. F, Jocou, L, Kenworthy, M, Kervella, P, Kreidberg, L, Kurtovic, N. T, Lagrange, A. -M, Mang, F, Marleau, G. -D, Mérand, A, Millour, F, Mollière, P, Monnier, J. D, Mordasini, C, Nasedkin, E, Paumard, T, Perraut, K, Pfuhl, O, Ribeiro, D. C, Rickman, E, Shimizu, T, Stadler, J, Stolker, T, Straub, O, Straubmeier, C, Vincent, F, Wang, J, Yazici, S, Andolfato, L, Barriga, P, Beuzit, J. -L, Brast, R, Caniguante, L, Cottalorda, E, Delboulbé, A, Delplancke-Ströbele, F, Egner, S, Frank, C, Fuenteseca, E, Gitton, P, Guerlet, T, Guieu, S, Haguenauer, P, Haimerl, A, Huber, S, Hubin, N, Jolley, P, Kirchbauer, J. -P, Kolb, J, Kosmalski, J, Louarn, M. Le, Lilley, P, Lopez, B, Mclay, S, Meilland, A, Paufique, J, Quentin, J, Rakich, A, Ridings, R, Shchekaturov, P, Soenke, C, Stadler, E, Todorovic, M, Zins, G, Zúñiga-Fernández, S, Collaboration, the NAOMI

“…Since 2019, GRAVITY has provided direct observations of giant planets and brown dwarfs at separations of down to 95 mas from the host star. Some of these…”
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GRAVITY+ Wide: Towards hundreds of z $\sim$ 2 AGN by Drescher, A, Fabricius, M, Shimizu, T, Woillez, J, Bourget, P, Widmann, F, Shangguan, J, Straubmeier, C, Horrobin, M, Schuhler, N, Eisenhauer, F, Gonté, F, Gillessen, S, Ott, T, Perrin, G, Paumard, T, Brandner, W, Kreidberg, L, Perraut, K, Bouquin, J. -B. Le, Garcia, P, Hönig, S, Defrère, D, Bourdarot, G, Feuchtgruber, H, Genzel, R, Hartl, M, Haussmann, F, Lutz, D, More, N, Rau, C, Sauter, J, Uysal, S, Wessely, P, Wieprecht, E, Wimmer, L, Yazici, S

“…As part of the GRAVITY$^{+}$ project, the near-infrared beam combiner GRAVITY and the VLTI are currently undergoing a series of significant upgrades to further…”
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A dynamical measure of the black hole mass in a quasar 11 billion years ago by Allouche, F, Amorim, A, Berdeu, A, Berio, P, Bigioli, A, Boebion, O, Bolzer, M. -L, Bonnet, H, Bourdarot, G, Bourget, P, Brandner, W, Cao, Y, Conzelmann, R, Comin, M, Clénet, Y, Courtney-Barrer, B, Davies, R, Defrère, D, Delplancke-Ströbele, F, Dembet, R, Dexter, J, Drescher, A, Eckart, A, Édouard, C, Eisenhauer, F, Feuchtgruber, H, Finger, G, Schreiber, N. M. Förster, Gao, F, Gendron, E, Genzel, R, Gillessen, S, Gomes, T, Gonté, F, Gouvret, C, Guajardo, P, Guieu, S, Hackenberg, W, Hartl, M, Heißel, G, Henning, Th, Hippler, S, Horrobin, M, Hubin, N, Jacqmart, E, Jocou, L, Kaufer, A, Kervella, P, Kolb, J, Korhonen, H, Lacour, S, Lagarde, S, Lai, O, Lapeyrère, V, Laugier, R, Bouquin, J. -B. Le, Leftley, J, Léna, P, Lewis, S, Liu, D, Lutz, D, Magnard, Y, Marcotto, A, Maurel, D, Mérand, A, Millour, F, More, N, Nowak, M, Oberti, S, Ott, T, Pallanca, L, Paumard, T, Perraut, K, Perrin, G, Petrov, R, Pfuhl, O, Pourré, N, Rabien, S, Robbe-Dubois, S, Salman, M, Sanchez-Bermudez, J, Scheithauer, S, Schöller, M, Schubert, J, Schuhler, N, Shangguan, J, Shimizu, T. T, Soulez, F, Spang, A, Stadler, E, Sternberg, A, Straubmeier, C, Tacconi, L. J, Tristram, K. R. W, Vincent, F, von Fellenberg, S, Uysal, S, Widmann, F, Wieprecht, E, Wiezorrek, E

“…Tight relationships exist in the local universe between the central stellar properties of galaxies and the mass of their supermassive black hole. These suggest…”
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First Light for GRAVITY Wide: Large Separation Fringe Tracking for the Very Large Telescope Interferometer by Collaboration, GRAVITY+, :, Abuter, R, Allouche, F, Bailet, C, Bauböck, M, Berio, P, Bigioli, A, Boebion, O, Bonnet, H, Bourdarot, G, Bourget, P, Brandner, W, Clénet, Y, Courtney-Barrer, B, Dallilar, Y, Davies, R, Delplancke, F, Dembet, R, Drescher, A, Eckart, A, Édouard, C, Eisenhauer, F, Fabricius, M, Finger, G, Schreiber, N. M. Förster, Garcia, E, Garcia, P, Gao, F, Gendron, E, Genzel, R, Gil, J. P, Gomes, T, Gonté, F, Guieu, S, Hartl, M, Haußmann, F, Heißel, G, Henning, Th, Hippler, S, Hönig, S, Horrobin, M, Hubin, N, Jacqmart, E, Jochum, L, Jocou, L, Kaufer, A, Kervella, P, Korhonen, H, Kreidberg, L, Lacour, S, Lagarde, S, Lai, O, Lapeyrère, V, Laugier, R, Bouquin, J. -B. Le, Leftley, J, Léna, P, Lutz, D, Mang, F, Marcotto, A, Maurel, D, Mérand, A, More, N, Nowacki, H, Oberti, S, Ott, T, Paumard, T, Perraut, K, Petrov, R, Pfuhl, O, Pourré, N, Rabien, S, Rau, C, Robbe-Dubois, S, Rochat, S, Salman, M, Schöller, M, Schubert, J, Schuhler, N, Shangguan, J, Shimizu, T, Scheithauer, S, Sevin, A, Soulez, F, Spang, A, Stadler, E, Straubmeier, C, Sturm, E, Tacconi, L. J, Tristram, K. R. W, Vincent, F, von Fellenberg, S, Uysal, S, Widmann, F, Wiezorrek, E, Woillez, J, Yazici, S, Young, A, Zins, G

“…A&A 665, A75 (2022) GRAVITY+ is the upgrade of GRAVITY and the Very Large Telescope Interferometer (VLTI) with wide-separation fringe tracking, new adaptive…”
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MATISSE, the VLTI mid-infrared imaging spectro-interferometer by Lopez, B, Lagarde, S, Petrov, R. G, Jaffe, W, Antonelli, P, Allouche, F, Berio, P, Millour, F, Robbe-Dubois, S, Henning, Th, Weigelt, G, Glindemann, A, Agocs, T, Bailet, Ch, Beckmann, U, Bettonvil, F, van Boekel, R, Bresson, Y, Cruzalèbes, P, Herrera, J. C. González, Heininger, M, Hofmann, K. -H, Laun, W, Lehmitz, M, Leinert, C, Morel, S, Neumann, U, Paladini, C, Percheron, I, Schoeller, M, Stee, Ph, Venema, L, Woillez, J, Zins, G, Abuter, R, Adler, T, Alonso, J, Böhm, A, Beltran, J, Boland, W, Brast, R, Burtscher, L, Castillo, R, Chelli, A, Clausse, J. -M, Connot, C, Danchi, W. -C, Drevon, J, Ebert, M, Eisenhauer, F, Flament, S, Frahm, R, Rosas, V. Gámez, Gabasch, A, Garces, E, Girard, P, Guitton, F, de Haan, M, Haubois, X, Hocdé, V, Hogerheijde, M, ter Horst, R, Hummel, C. A, Idserda, J, Isbell, J. W, Ives, D, Kragt, J, Kuindersma, S, Kokoulina, E, Labadie, L, Lacour, S, Leftley, J, Lizon, J. -L, Lopez, M, Mérand, A, Marcotto, A, Mauclert, N, Maurer, T, Mehrgan, L. H, Meisner, J, Meixner, K, Mellein, M, Mohr, L, Navarro, R, Pallanca, L, Pasquini, L, Pott, J. -U, Pozna, E, Richichi, A, Ridinger, A, Roelfsema, R, Salabert, D, Schertl, D, Schuil, M, Soulain, A, Stephan, C, Tristram, K, Tromp, N, Waters, L. B. F. M, Wolf, S

“…A&A 659, A192 (2022) Context:Optical interferometry is at a key development stage. ESO's VLTI has established a stable, robust infrastructure for long-baseline…”
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Mid-infrared circumstellar emission of the long-period Cepheid l Carinae resolved with VLTI/MATISSE by Hocdé, V, Nardetto, N, Lagadec, E, Mérand, A, Cruzalèbes, P, Meilland, A, Lopez, B, Berio, P, Weigelt, G, Petrov, R, Isbell, J. W, Schöller, M, Allouche, F, Gallenne, A, Niccolini, G, Kokoulina, E, Varga, J, Bristow, P, Henning, Th, Hofmann, K. -H, Delbo, M, Dominik, C, Rosas, V. Gámez, Klarmann, L, Hron, J, Hogerheijde, M. R, Pantin, E, Paladini, C, Schertl, D, Stee, P, Waters, R, Woillez, J, Yoffe, G, Szabados, L, Borgniet, S, Breuval, L, Javanmardi, B, Abadie, S, Accardo, M, Adler, T, Alonso, J, Antonelli, P, Böhm, A, Bailet, C, Bazin, G, Beltran, J, Boland, W, Bourget, P, Brast, R, Bresson, Y, Buter, R, Chelli, A, Cid, C, Conzelmann, R. D, Ebert, M, Elswijk, E, Garces, E, Glazenborg, A, Gonté, F. Y. J, Herrera, J. C. González, Guajardo, P, Guitton, F, Hanenburg, H, Haubois, X, Huerta, R, Idserda, J, Ives, D, Jakob, G, Jaskó, A, Klein, R, Kuindersma, S, Labadie, L, Laun, W, Poole, R. Le, Leinert, C, Lizon, J. -L, Lopez, M, Mauclert, N, Maurer, T, Mehrgan, L. H, Meisner, J, Mellein, M, Morel, S, Mosoni, L, Navarro, R, Pasquini, L, Duc, T. Phan, Pott, J. -U, Pozna, E, Rigal, F, Riquelme, M, Rivinius, Th, Rohloff, R. -R, Rousseau, S, Schuhler, N, Soulain, A, Tromp, N, Venema, L. B, Wittkowski, M, Wrhel, F

“…The nature of circumstellar envelopes (CSE) around Cepheids is still a matter of debate. The physical origin of their infrared (IR) excess could be either a…”
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The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex? by Varga, J, Hogerheijde, M, van Boekel, R, Klarmann, L, Petrov, R, Lagarde, S, Pantin, E, Berio, Ph, Weigelt, G, Lopez, B, Augereau, J. -C, Meheut, H, Jaffe, W, Bettonvil, F, Bristow, P, Matter, A, Zins, G, Allouche, F, Donnan, F, Schertl, D, Dominik, C, Heininger, M, Lehmitz, M, Cruzalèbes, P, Glindemann, A, Meisenheimer, K, Paladini, C, Schöller, M, Venema, L, Kokoulina, E, Yoffe, G, Abadie, S, Abuter, R, Accardo, M, Adler, T, Agócs, T, Antonelli, P, Böhm, A, Bailet, C, Bazin, G, Beltran, J, Boland, W, Brast, R, Bresson, Y, Burtscher, L, Castillo, R, Chelli, A, Cid, C, Clausse, J. -M, Connot, C, Conzelmann, R. D, Danchi, W. -C, Ebert, M, Elswijk, E, Fantei, Y, Rosas, V. Gámez, Gabasch, A, Gallenne, A, Garces, E, Gonté, F. Y. J, Herrera, J. C. González, Guajardo, P, Guitton, F, Haubois, X, Hron, J, Ives, D, Jakob, G, Jaskó, A, Jochum, L, Kragt, J, Labadie, L, Laun, W, Leinert, C, Lizon, J. -L, Mérand, A, Mauclert, N, Maurer, T, Meisner, J, Mellein, M, Mohr, L, Morel, S, Mosoni, L, Navarro, R, Pott, J. -U, Ridinger, A, Rigal, F, Roelfsema, R, Rohloff, R. -R, Rousseau, S, Schuhler, N, Schuil, M, Soulain, A, Stee, P, Stephan, C, Tromp, N, Vakili, F, van Duin, A, Vinther, J, Wittkowski, M, Wrhel, F

“…A&A 647, A56 (2021) Context. The inner few au region of planet-forming disks is a complex environment. High angular resolution observations have a key role in…”
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Extinction controlled adaptive phase-mask coronagraph by Bourget, P, Schuhler, N, Mawet, D, Haguenauer, P

“…Context. Phase-mask coronagraphy is advantageous in terms of inner working angle and discovery space. It is however still plagued by drawbacks such as…”
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First direct detection of an exoplanet by optical interferometry; Astrometry and K-band spectroscopy of HR8799 e by Lacour, S, Nowak, M, Wang, J, Pfuhl, O, Eisenhauer, F, Abuter, R, Amorim, A, Anugu, N, Benisty, M, Berger, J. P, Beust, H, Blind, N, Bonnefoy, M, Bonnet, H, Bourget, P, Brandner, W, Buron, A, Collin, C, Charnay, B, Chapron, F, Clénet, Y, Foresto, V. Coudé du, de Zeeuw, P. T, Deen, C, Dembet, R, Dexter, J, Duvert, G, Eckart, A, Schreiber, N. M. Förster, Fédou, P, Garcia, P, Lopez, R. Garcia, Gao, F, Gendron, E, Genzel, R, Gillessen, S, Gordo, P, Greenbaum, A, Habibi, M, Haubois, X, Haußmann, F, Henning, Th, Hippler, S, Horrobin, M, Hubert, Z, Rosales, A. Jimenez, Jocou, L, Kendrew, S, Kervella, P, Kolb, J, Lagrange, A. -M, Lapeyrère, V, Bouquin, J. -B. Le, Léna, P, Lippa, M, Lenzen, R, Maire, A. -L, Mollière, P, Ott, T, Paumard, T, Perraut, K, Perrin, G, Pueyo, L, Rabien, S, Ramirez, A, Rau, C, Rodriguez-Coira, G, Rousset, G, Sanchez-Bermudez, J, Scheithauer, S, Schuhler, N, Straub, O, Straubmeier, C, Sturm, E, Tacconi, L. J, Vincent, F, van Dishoeck, E. F, von Fellenberg, S, Wank, I, Waisberg, I, Widmann, F, Wieprecht, E, Wiest, M, Wiezorrek, E, Woillez, J, Yazici, S, Ziegler, D, Zins, G

“…To date, infrared interferometry at best achieved contrast ratios of a few times $10^{-4}$ on bright targets. GRAVITY, with its dual-field mode, is now capable…”
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GRAVITY chromatic imaging of Eta Car's core by GRAVITY Collaboration, Sanchez-Bermudez, J, Kervella, P, Müller, A, Perrin, G, Pott, J. -U, Schöller, M, Accardo, M, Anugu, N, Ávila, G, Benisty, M, Berger, J. P, Blind, N, Bonnet, H, Bourget, P, Brast, R, Buron, A, Cantalloube, F, Garatti, A. Caratti o, Cassaing, F, Chapron, F, Choquet, E, Clénet, Y, Collin, C, de Wit, W, de Zeeuw, T, Deen, C, Delplancke-Ströbele, F, Dembet, R, Derie, F, Dexter, J, Duvert, G, Eckart, A, Eisenhauer, F, Esselborn, M, Fédou, P, Gao, F, Gendron, E, Gillessen, S, Haubois, X, Haug, M, Haussmann, F, Hippler, S, Horrobin, M, Huber, A, Hummel, C. A, Jakob, G, Jochum, L, Kellner, S, Kendrew, S, Kern, L, Kiekebusch, M, Klein, R, Kolb, J, Kulas, M, Lacour, S, Lapeyrère, V, Lazareff, B, Bouquin, J. -B. Le, Lenzen, R, Mehrgan, L, Mellein, M, Mérand, A, Moreno-Ventas, J, Moulin, T, Müller, E, Oberti, S, Ott, T, Pallanca, L, Panduro, J, Pasquini, L, Paumard, T, Perraut, K, Petrucci, P. -O, Pflüger, A, Duc, T. P, Popovic, D, Rabien, S, Ramirez, A, Ramos, J, Rau, C, Riquelme, M, Rodríguez-Coira, G, Rosales, A, Rousset, G, Schuhler, N, Sturm, E, Suarez, M, Tristram, K. R. W, Vincent, F, Waisberg, I, Wank, I, Widmann, F, Wieprecht, E, Wiest, M, Wiezorrek, E, Woillez, J, Wolff, B, Ziegler, D, Zins, G

“…Eta Car is one of the most intriguing luminous blue variables in the Galaxy. Observations and models at different wavelengths suggest a central binary with a…”
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First Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer by GRAVITY Collaboration, Amorim, A, Ávila, G, Azouaoui, N, Benisty, M, Berger, J. P, Blind, N, Bourget, P, Brandner, W, Brast, R, Buron, A, Burtscher, L, Choquet, É, Clénet, Y, Collin, C, Foresto, V. Coudé du, de Wit, W, de Zeeuw, P. T, Deen, C, Delplancke-Ströbele, F, Dembet, R, Duvert, G, Ebert, M, Eckart, A, Esselborn, M, Fédou, P, Finger, G, Garcia, P, Lopez, R. Garcia, Gendron, E, Genzel, R, Gillessen, S, Gonte, F, Gordo, P, Grözinger, U, Guieu, S, Haguenauer, P, Hans, O, Haug, M, Haussmann, F, Henning, Th, Hippler, S, Huber, A, Hubert, Z, Hubin, N, Hummel, C. A, Janssen, A, Jocou, L, Kaufer, A, Kern, L, Kervella, P, Klein, R, Kok, Y, Kulas, M, Lacour, S, Lazareff, B, Bouquin, J. -B. Le, Lèna, P, Lévêque, S, Lippa, M, Magnard, Y, Mehrgan, L, Mellein, M, Moreno-Ventas, J, Moulin, T, Müller, E, Müller, F, Neumann, U, Ott, T, Pallanca, L, Panduro, J, Paumard, T, Percheron, I, Perraut, K, Pflüger, A, Pfuhl, O, Duc, T. Phan, Plewa, P. M, Rabien, S, Ramírez, A, Ramos, J, Rau, C, Rohloff, R. -R, Scheithauer, S, Schöller, M, Schuhler, N, Spyromilio, J, Straubmeier, C, Sturm, E, Suarez, M, Tristram, K. R. W, Ventura, N, Vincent, F, Wank, I, Wieprecht, E, Wittkowski, M, Woillez, J, Wolff, B, Yazici, S, Ziegler, D

“…A&A 602, A94 (2017) GRAVITY is a new instrument to coherently combine the light of the European Southern Observatory Very Large Telescope Interferometer to…”
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Improving the astrometric performance of VLTI-PRIMA by Woillez, J, Abuter, R, Andolfato, L, Berger, J. P, Bonnet, H, Delplancke, F, Derie, F, Di Lieto, N, Guniat, S, Mérand, A, Duc, T. Phan, Schmid, C, Schuhler, N, Henning, T, Launhardt, R, Pepe, F, Queloz, D, Quirrenbach, A, Reffert, S, Sahlmann, S, Segransan, D

“…Proc. SPIE 9146, 9146-50 (2014) In the summer of 2011, the first on-sky astrometric commissioning of PRIMA-Astrometry delivered a performance of 3 m'' for a 10…”
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