Zobrazeno 1 - 10
of 311
pro vyhledávání: '"P. Fedou"'
Autor:
Perrin, G., Jocou, L., Perraut, K., Berger, J. Ph., Dembet, R., Fédou, P., Lacour, S., Chapron, F., Collin, C., Poulain, S., Cardin, V., Joulain, F., Eisenhauer, F., Haubois, X., Gillessen, S., Haug, M., Hausmann, F., Kervella, P., Léna, P., Lippa, M., Pfuh, O., Rabien, S., Amorim, A., Brandner, W., Straubmeier, C.
Publikováno v:
A&A 681, A26 (2024)
The 2nd generation VLTI instrument GRAVITY is a two-field infrared interferometer operating in the K band between 1.97 and 2.43 $\mu$m with either the four 8 m or the four 1.8 m telescopes of the Very Large Telescope (VLT). Beams collected by the tel
Externí odkaz:
http://arxiv.org/abs/2401.10613
Autor:
Ana-Sofia Eria-Oliveira, Mathilde Folacci, Anne Amandine Chassot, Sandrine Fedou, Nadine Thézé, Dmitrii Zabelskii, Alexey Alekseev, Ernst Bamberg, Valentin Gordeliy, Guillaume Sandoz, Michel Vivaudou
Publikováno v:
Nature Communications, Vol 15, Iss 1, Pp 1-11 (2024)
Abstract Rhodopsins are ubiquitous light-driven membrane proteins with diverse functions, including ion transport. Widely distributed, they are also coded in the genomes of giant viruses infecting phytoplankton where their function is not settled. He
Externí odkaz:
https://doaj.org/article/0cda7eb402034abe872f92cb1c70f4e5
Peering into the formation history of beta Pictoris b with VLTI/GRAVITY long baseline interferometry
Autor:
GRAVITY Collaboration, Nowak, M., Lacour, S., Mollière, P., Wang, J., Charnay, B., van Dishoeck, E. F., Abuter, R., Amorim, A., Berger, J. P., Beust, H., Bonnefoy, M., Bonnet, H., Brandner, W., Buron, A., Cantalloube, F., Collin, C., Chapron, F., Clenet, Y., Foresto, V. Coude du, de Zeeuw, P. T., Dembet, R., Dexter, J., Duvert, G., Eckart, A., Eisenhauer, F., Schreiber, N. M. Forster, Fédou, P., Lopez, R. Garcia, Gao, F., Gendron, E., Genzel, R., Gillessen, S., Haußmann, F., Henning, T., Hippler, S., Hubert, Z., Jocou, L., Kervella, P., Lagrange, A. -M., Lapeyrere, V., Bouquin, J. -B. Le, Lena, P., Maire, A. -L., Ott, T., Paumard, T., Paladini, C., Perraut, K., Perrin, G., Pueyo, L., Pfuhl, O., Rabien, S., Rau, C., Rodriguez-Coira, G., Rousset, G., Scheithauer, S., Shangguan, J., Straub, O., Straubmeier, C., Sturm, E., Tacconi, L. J., Vincent, F., Widmann, F., Wieprecht, E., Wiezorrek, E., Woillez, J., Yazici, S., Ziegler, D.
Publikováno v:
A&A 633, A110 (2020)
Our objective is to estimate the C/O ratio in the atmosphere of beta Pictoris b and obtain an estimate of the dynamical mass of the planet, as well as to refine its orbital parameters using high-precision astrometry. We used the GRAVITY instrument wi
Externí odkaz:
http://arxiv.org/abs/1912.04651
Autor:
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 of high contrast observations, enabling the direct observation of exoplanets. We demonstra
Externí odkaz:
http://arxiv.org/abs/1903.11903
Autor:
Lacour, S., Dembet, R., Abuter, R., Fedou, P., Perrin, G., Choquet, E., Pfuhl, O., Eisenhauer, F., Woillez, J., Cassaing, F., Wieprecht, E., Ott, T., Wiezorrek, E., Wolff, B., Ramirez, A., Haubois, X., Perraut, K., Straubmeier, C., Brandner, W., Amorim, A.
Publikováno v:
A&A 624, A99 (2019)
The GRAVITY instrument has been commissioned on the VLTI during 2016 and is now available to the astronomical community. It is the first optical interferometer capable of observing sources as faint as magnitude 19 in K-band. This is possible thanks t
Externí odkaz:
http://arxiv.org/abs/1901.03202
Akademický článek
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Autor:
GRAVITY collaboration, Karl, Martina, Pfuhl, Oliver, Eisenhauer, Frank, Genzel, Reinhard, Grellmann, Rebekka, Habibi, Maryam, Abuter, Roberto, Accardo, Matteo, Amorim, António, Anugu, Narsireddy, Ávila, Gerardo, Benisty, Myriam, Berger, Jean-Philippe, Bland, Nicolas, Bonnet, Henri, Bourget, Pierre, Brandner, Wolfgang, Brast, Roland, Buron, Alexander, Garatti, Alessio Caratti o, Chapron, Frédéric, Clénet, Yann, Collin, Claude, Foresto, Vincent Coudé du, de Wit, Willem-Jan, de Zeeuw, Tim, Deen, Casey, Delplancke-Ströbele, Françoise, Dembet, Roderick, Derie, Frédéric, Dexter, Jason, Duvert, Gilles, Ebert, Monica, Eckart, Andreas, Esselborn, Michael, Fédou, Pierre, Finger, Gert, Garcia, Paulo, Dabo, Cesar Enrique Garcia, Lopez, Rebeca Garcia, Gao, Feng, Gandron, Éric, Gillessen, Stefan, Gonté, Frédéric, Gordo, Paulo, Grözinger, Ulrich, Guajardo, Patricia, Guieu, Sylvain, Haguenauer, Pierre, Hans, Oliver, Haubois, Xavier, Haug, Marcus, Haußmann, Frank, Henning, Thomas, Hippler, Stefan, Horrobin, Matthew, Huber, Armin, Hubert, Zoltan, Hubin, Norbert, Hummel, Christian A., Jakob, Gerd, Jochum, Lieselotte, Jocou, Laurent, Kaufer, Andreas, Kellner, Stefan, Kandrew, Sarah, Kern, Lothar, Kervella, Pierre, Kiekebusch, Mario, Klein, Ralf, Köhler, Rainer, Kolb, Johan, Kulas, Martin, Lacour, Sylvestre, Lapeyrère, Vincent, Lazareff, Bernard, Bouquin, Jean-Baptiste Le, Léna, Pierre, Lenzen, Rainer, Lévêque, Samuel, Lin, Chien-Cheng, Lippa, Magdalena, Magnard, Yves, Mehrgan, Leander, Mérand, Antoine, Moulin, Thibaut, Müller, Eric, Müller, Friedrich, Neumann, Udo, Oberti, Sylvain, Ott, Thomas, Pallanca, Laurent, Panduro, Johana, Pasquini, Luca, Paumard, Thibaut, Percheron, Isabelle, Perraut, Karine, Perrin, Guy, Pflüger, Andreas, Duc, Thanh Phan, Plewa, Philipp M., Popovic, Dan, Rabien, Sebastian, Ramírez, Andrés, Ramos, Jose, Rau, Christian, Riquelme, Miguel, Rodríguez-Coira, Gustavo, Rohloff, Ralf-Rainer, Rosales, Alejandra, Rousset, Gérard, Sanchez-Bermudez, Joel, Scheithauer, Silvia, Schöller, Markus, Schuhler, Nicolas, Spyromilio, Jason, Straub, Odele, Straubmeier, Christian, Sturm, Eckhard, Suarez, Marcos, Tristram, Konrad R. W., Ventura, Noel, Vincent, Frédéric, Waisberg, Idel, Wank, Imke, Widmann, Felix, Wieprecht, Ekkehard, Wiest, Michael, Wiezorrek, Erich, Wittkowski, Markus, Woillez, Julien, Wolff, Burkhard, Yazici, Senol, Ziegler, Denis, Zins, Gérard
Publikováno v:
A&A 620, A116 (2018)
This work presents an interferometric study of the massive-binary fraction in the Orion Trapezium Cluster with the recently comissioned GRAVITY instrument. We observe a total of 16 stars of mainly OB spectral type. We find three previously unknown co
Externí odkaz:
http://arxiv.org/abs/1809.10376
Autor:
GRAVITY Collaboration, Sanchez-Bermudez, J., Weigelt, G., Bestenlehner, J. M., Kervella, P., Brandner, W., Henning, Th., Müller, A., Perrin, G., Pott, J. -U., Schöller, M., van Boekel, R., Abuter, R., Accardo, M., Amorim, A., 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., Foresto, V. Coudé du, de Wit, W., de Zeeuw, T., Deen, C., Delplancke-Ströbele, F., Dembet, R., Derie, F., Dexter, J., Duvert, G., Ebert, M., Eckart, A., Eisenhauer, F., Esselborn, M., Fédou, P., Garcia, P. J. V., Dabo, C. E. Garcia, Lopez, R. Garcia, Gao, F., Gendron, E., Genzel, R., Gillessen, S., Haubois, X., Haug, M., Haussmann, F., Hippler, S., Horrobin, M., Huber, A., Hubert, Z., Hubin, N., Hummel, C. A., Jakob, G., Jochum, L., Jocou, L., Karl, M., Kaufer, A., Kellner, S., Kendrew, S., Kern, L., Kiekebusch, M., Klein, R., Kolb, J., Kulas, M., Lacour, S., Lapeyrère, V., Lazareff, B., Bouquin, J. -B. Le, Léna, P., Lenzen, R., Levêque, S., Lippa, M., Magnard, Y., Mehrgan, L., Mellein, M., Mérand, A., Moreno-Ventas, J., Moulin, T., Müller, E., Müller, F., Neumann, U., Oberti, S., Ott, T., Pallanca, L., Panduro, J., Pasquini, L., Paumard, T., Percheron, I., Perraut, K., Petrucci, P. -O., Pflüger, A., Pfuhl, O., Duc, T. P., Plewa, P. M., Popovic, D., Rabien, S., Ramirez, A., Ramos, J., Rau, C., Riquelme, M., Rodríguez-Coira, G., Rohloff, R. -R., Rosales, A., Rousset, G., Scheithauer, S., Schuhler, N., Spyromilio, J., Straub, O., Straubmeier, C., Sturm, E., Suarez, M., Tristram, K. R. W., Ventura, N., Vincent, F., Waisberg, I., Wank, I., Widmann, F., Wieprecht, E., Wiest, M., Wiezorrek, E., Wittkowski, M., Woillez, J., Wolff, B., Yazici, S., 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 5.54 yr period residing in its core. 2D and 3D radiative transfer and hydrodynamic simulatio
Externí odkaz:
http://arxiv.org/abs/1808.02141
Autor:
Davies, Richard, Alves, João, Clénet, Yann, Lang-Bardl, Florian, Nicklas, Harald, Pott, Jörg-Uwe, Ragazzoni, Roberto, Tolstoy, Eline, Amico, Paola, Anwand-Heerwart, Heiko, Barboza, Santiago, Barl, Lothar, Baudoz, Pierre, Bender, Ralf, Bezawada, Naidu, Bizenberger, Peter, Boland, Wilfried, Bonifacio, Piercarlo, Borgo, Bruno, Buey, Tristan, Chapron, Frédéric, Chemla, Fanny, Cohen, Mathieu, Czoske, Oliver, Deo, Vincent, Disseau, Karen, Dreizler, Stefan, Dupuis, Olivier, Fabricius, Maximilian, Falomo, Renato, Fedou, Pierre, Schreiber, Natascha Foerster, Garrel, Vincent, Geis, Norbert, Gemperlein, Hans, Gendron, Eric, Genzel, Reinhard, Gillessen, Stefan, Glück, Martin, Grupp, Frank, Hartl, Michael, Häuser, Marco, Hess, Hans-Joachim, Hofferbert, Ralf, Hopp, Ulrich, Hörmann, Veronika, Hubert, Zoltan, Huby, Elsa, Huet, Jean-Michel, Hutterer, Victoria, Ives, Derek, Janssen, Annemieke, Jellema, Willem, Kausch, Wolfgang, Kerber, Florian, Kravcar, Helmut, Ruyet, Bertrand Le, Leschinski, Kieran, Mandla, Christopher, Manhart, Markus, Massari, Davide, Mei, Simona, Merlin, Frédéric, Mohr, Lars, Monna, Anna, Muench, Norbert, Mueller, Friedrich, Musters, Gert, Navarro, Ramon, Neumann, Udo, Neumayer, Nadine, Niebsch, Jenny, Plattner, Markus, Przybilla, Norbert, Rabien, Sebastian, Ramlau, Ronny, Ramos, José, Ramsay, Suzanne, Rhode, Petra, Richter, Amon, Richter, Josef, Rix, Hans-Walter, Rodeghiero, Gabriele, Rohloff, Ralf-Rainer, Rosensteiner, Matthias, Rousset, Gérard, Schlichter, Jörg, Schubert, Josef, Sevin, Arnaud, Stuik, Remko, Sturm, Eckhard, Thomas, Jens, Tromp, Niels, Kleijn, Gijs Verdoes, Vidal, Fabrice, Wagner, Roland, Wegner, Michael, Zeilinger, Werner, Ziegleder, Julian, Ziegler, Bodo, Zins, Gérard
MICADO will enable the ELT to perform diffraction limited near-infrared observations at first light. The instrument's capabilities focus on imaging (including astrometric and high contrast) as well as single object spectroscopy. This contribution loo
Externí odkaz:
http://arxiv.org/abs/1807.10003
Autor:
GRAVITY Collaboration, Abuter, R., Amorim, A., Anugu, N., Bauböck, M., Benisty, M., Berger, J. P., Blind, N., Bonnet, H., Brandner, W., Buron, A., Collin, C., Chapron, F., Clénet, Y., Foresto, V. Coudé du, de Zeeuw, P. T., Deen, C., Delplancke-Ströbele, F., Dembet, R., Dexter, J., Duvert, G., Eckart, A., Eisenhauer, F., Finger, G., Schreiber, N. M. Förster, Fédou, P., Garcia, P., Lopez, R. Garcia, Gao, F., Gendron, E., Genzel, R., Gillessen, S., Gordo, P., Habibi, M., Haubois, X., Haug, M., Haußmann, F., Henning, Th., Hippler, S., Horrobin, M., Hubert, Z., Hubin, N., Rosales, A. Jimenez, Jochum, L., Jocou, L., Kaufer, A., Kellner, S., Kendrew, S., Kervella, P., Kok, Y., Kulas, M., Lacour, S., Lapeyrère, V., Lazareff, B., Bouquin, J. -B. Le, Léna, P., Lippa, M., Lenzen, R., Mérand, A., Müller, E., Neumann, U., Ott, T., Palanca, L., Paumard, T., Pasquini, L., Perraut, K., Perrin, G., Pfuhl, O., Plewa, P. M., Rabien, S., Ramírez, A., Ramos, J., Rau, C., Rodríguez-Coira, G., Rohloff, R. -R., Rousset, G., Sanchez-Bermudez, J., Scheithauer, S., Schöller, M., Schuler, N., Spyromilio, J., Straub, O., Straubmeier, C., Sturm, E., Tacconi, L. J., Tristram, K. R. W., Vincent, F., von Fellenberg, S., Wank, I., Waisberg, I., Widmann, F., Wieprecht, E., Wiest, M., Wiezorrek, E., Woillez, J., Yazici, S., Ziegler, D., Zins, G.
Publikováno v:
A&A 615, L15 (2018)
The highly elliptical, 16-year-period orbit of the star S2 around the massive black hole candidate Sgr A* is a sensitive probe of the gravitational field in the Galactic centre. Near pericentre at 120 AU, ~1400 Schwarzschild radii, the star has an or
Externí odkaz:
http://arxiv.org/abs/1807.09409