Search Results - "Langlois, Maud"

Fast-moving features in the debris disk around AU Microscopii by Boccaletti, Anthony, Thalmann, Christian, Lagrange, Anne-Marie, Janson, Markus, Augereau, Jean-Charles, Schneider, Glenn, Milli, Julien, Grady, Carol, Debes, John, Langlois, Maud, Mouillet, David, Henning, Thomas, Dominik, Carsten, Maire, Anne-Lise, Beuzit, Jean-Luc, Carson, Joseph, Dohlen, Kjetil, Engler, Natalia, Feldt, Markus, Fusco, Thierry, Ginski, Christian, Girard, Julien H., Hines, Dean, Kasper, Markus, Mawet, Dimitri, Ménard, François, Meyer, Michael R., Moutou, Claire, Olofsson, Johan, Rodigas, Timothy, Sauvage, Jean-Francois, Schlieder, Joshua, Schmid, Hans Martin, Turatto, Massimo, Udry, Stephane, Vakili, Farrokh, Vigan, Arthur, Wahhaj, Zahed, Wisniewski, John

“…High-contrast imaging of the nearby, young, active late-type star AU Microscopii reveals five mysterious large-scale features in the southeast side of its…”
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REXPACO ASDI: joint unmixing and deconvolution of the circumstellar environment by angular and spectral differential imaging by Flasseur, Olivier, Denis, Loïc, Thiébaut, Éric, Langlois, Maud

“…ABSTRACT Angular and spectral differential imaging is an observational technique of choice to investigate the immediate vicinity of stars. By leveraging the…”
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MODEL&CO: exoplanet detection in angular differential imaging by learning across multiple observations by Bodrito, Théo, Flasseur, Olivier, Mairal, Julien, Ponce, Jean, Langlois, Maud, Lagrange, Anne-Marie

“…ABSTRACT Direct imaging of exoplanets is particularly challenging due to the high contrast between the planet and the star luminosities, and their small…”
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deep PACO: combining statistical models with deep learning for exoplanet detection and characterization in direct imaging at high contrast by Flasseur, Olivier, Bodrito, Théo, Mairal, Julien, Ponce, Jean, Langlois, Maud, Lagrange, Anne-Marie

“…ABSTRACT Direct imaging is an active research topic in astronomy for the detection and the characterization of young substellar objects. The very high contrast…”
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Spirals, shadows, and precession in HD 100453 – I. The orbit of the binary by Gonzalez, Jean-François, van der Plas, Gerrit, Pinte, Christophe, Cuello, Nicolás, Nealon, Rebecca, Ménard, François, Revol, Alexandre, Rodet, Laetitia, Langlois, Maud, Maire, Anne-Lise

“…ABSTRACT In recent years, several protoplanetary discs have been observed to exhibit spirals, both in scattered light and (sub)millimetre continuum data. The…”
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A wide-orbit giant planet in the high-mass b Centauri binary system by Janson, Markus, Gratton, Raffaele, Rodet, Laetitia, Vigan, Arthur, Bonnefoy, Mickaël, Delorme, Philippe, Mamajek, Eric E., Reffert, Sabine, Stock, Lukas, Marleau, Gabriel-Dominique, Langlois, Maud, Chauvin, Gaël, Desidera, Silvano, Ringqvist, Simon, Mayer, Lucio, Viswanath, Gayathri, Squicciarini, Vito, Meyer, Michael R., Samland, Matthias, Petrus, Simon, Helled, Ravit, Kenworthy, Matthew A., Quanz, Sascha P., Biller, Beth, Henning, Thomas, Mesa, Dino, Engler, Natalia, Carson, Joseph C.

“…Planet formation occurs around a wide range of stellar masses and stellar system architectures 1 . An improved understanding of the formation process can be…”
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High-contrast and resolution near-infrared photometry of the core of R136 by Khorrami, Zeinab, Langlois, Maud, Clark, Paul C, Vakili, Farrokh, Buckner, Anne S M, Gonzalez, Marta, Crowther, Paul, Wünsch, Richard, Palouš, Jan, Lumsden, Stuart, Moraux, Estelle

“…ABSTRACT We present the sharpest and deepest near-infrared photometric analysis of the core of R136, a newly formed massive star cluster at the centre of the…”
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A multiwavelength study of the debris disc around 49 Cet by Pawellek, Nicole, Moór, Attila, Milli, Julien, Kóspál, Ágnes, Olofsson, Johan, Ábrahám, Péter, Keppler, Miriam, Kral, Quentin, Pohl, Adriana, Augereau, Jean-Charles, Boccaletti, Anthony, Chauvin, Gaël, Choquet, Élodie, Engler, Natalia, Henning, Thomas, Langlois, Maud, Lee, Eve J, Ménard, François, Thébault, Philippe, Zurlo, Alice

“…Abstract In a multiwavelength study of thermal emission and scattered light images we analyse the dust properties and structure of the debris disc around the…”
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An Unsupervised Patch-Based Approach for Exoplanet Detection by Direct Imaging by Flasseur, Olivier, Denis, Loic, Thiebaut, Eric, Langlois, Maud

“…The search for exoplanet is a very active topic in astronomy. Exoplanet detection by direct imaging requires both dedicated instruments to mask out the host…”
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Workshop Summary: Exoplanet Orbits and Dynamics by Maire, Anne-Lise, Delrez, Laetitia, Pozuelos, Francisco J., Becker, Juliette, Espinoza, Nestor, Lillo-Box, Jorge, Revol, Alexandre, Absil, Olivier, Agol, Eric, Almenara, José M., Anglada-Escudé, Guillem, Beust, Hervé, Blunt, Sarah, Bolmont, Emeline, Bonavita, Mariangela, Brandner, Wolfgang, Mirek Brandt, G., Brandt, Timothy D., Brown, Garett, Cantero Mitjans, Carles, Charalambous, Carolina, Chauvin, Gaël, Correia, Alexandre C. M., Cranmer, Miles, Defrère, Denis, Deleuil, Magali, Demory, Brice-Olivier, De Rosa, Robert J., Desidera, Silvano, Dévora-Pajares, Martín, Díaz, Rodrigo F., Do Ó, Clarissa, Ducrot, Elsa, Dupuy, Trent J., Ferrer-Chávez, Rodrigo, Fontanive, Clémence, Gillon, Michaël, Giuppone, Cristian, Gkouvelis, Leonardos, de Oliveira Gomes, Gabriel, Gomes, Sérgio R. A., Günther, Maximilian N., Hadden, Sam, Han, Yinuo, Hernandez, David M., Jehin, Emmanuel, Kane, Stephen R., Kervella, Pierre, Kiefer, Flavien, Konopacky, Quinn M., Langlois, Maud, Lanssens, Benjamin, Lazzoni, Cecilia, Lendl, Monika, Li, Yiting, Libert, Anne-Sophie, Lovos, Flavia, Miculán, Romina G., Murray, Zachary, Pallé, Enric, Rein, Hanno, Rodet, Laetitia, Roisin, Arnaud, Sahlmann, Johannes, Siverd, Robert, Stalport, Manu, Carlos Suárez, Juan, Tamayo, Daniel, Teyssandier, Jean, Thuillier, Antoine, Timmermans, Mathilde, Triaud, Amaury H. M. J., Trifonov, Trifon, Valente, Ema F. S., Van Grootel, Valérie, Vasist, Malavika, Wang, Jason J., Wyatt, Mark C., Xuan, Jerry, Young, Steven, Zimmerman, Neil T.

“…Abstract Exoplanetary systems show a wide variety of architectures, which can be explained by different formation and dynamical evolution processes. Precise…”
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Imaging radial velocity planets with SPHERE by Zurlo, A, Mesa, D, Desidera, S, Messina, S, Gratton, R, Moutou, C, Beuzit, J-L, Biller, B, Boccaletti, A, Bonavita, M, Bonnefoy, M, Bhowmik, T, Brandner, W, Buenzli, E, Chauvin, G, Cudel, M, D’Orazi, V, Feldt, M, Hagelberg, J, Janson, M, Lagrange, A-M, Langlois, M, Lannier, J, Lavie, B, Lazzoni, C, Maire, A-L, Meyer, M, Mouillet, D, Peretti, S, Perrot, C, Potiron, P J, Salter, G, Schmidt, T, Sissa, E, Vigan, A, Delboulbé, A, Petit, C, Ramos, J, Rigal, F, Rochat, S

“…We present observations with the planet finder Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) of a selected sample of the most promising radial…”
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A multi-wavelength study of the debris disc around 49 Cet by Pawellek, Nicole, Moór, Attila, Milli, Julien, Kóspál, Ágnes, Olofsson, Johan, Ábrahám, Péter, Keppler, Miriam, Kral, Quentin, Pohl, Adriana, Augereau, Jean-Charles, Boccaletti, Anthony, Chauvin, Gael, Choquet, Elodie, Engler, Natalia, Henning, Thomas, Langlois, Maud, Lee, Eve J, Ménard, François, Thebault, Philippe, Zurlo, Alice

“…In a multi-wavelength study of thermal emission and scattered light images we analyse the dust properties and structure of the debris disc around the A1-type…”
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UV Spectropolarimetry With Polstar: Protoplanetary Disks by Wisniewski, John P, Berdyugin, Andrei V, Berdyugina, Svetlana V, Danchi, William C, Dong, Ruobing, Oudmaijer, René D, Airapetian, Vladimir, Brittain, Sean D, Gayley, Ken, Ignace, Richard, Langlois, Maude, Lawson, Kellen D, Lomax, Jamie R, Rich, Evan A, Tamura, Motohide, Vink, Jorick S, Scowen, Paul A

“…Polstar is a proposed NASA MIDEX mission that carries a high resolution UV spectropolarimeter capable of measure all four Stokes parameters onboard a 60 cm…”
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Shrinkage MMSE Estimators of Covariances Beyond the Zero-Mean and Stationary Variance Assumptions by Flasseur, Olivier, Thiebaut, Eric, Denis, Loic, Langlois, Maud

“…We tackle covariance estimation in low-sample scenarios, employing a structured covariance matrix with shrinkage methods. These involve convexly combining a…”
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Shrinkage MMSE estimators of covariances beyond the zero-mean and stationary variance assumptions by Flasseur, Olivier, Thiébaut, Eric, Denis, Loïc, Langlois, Maud

“…We tackle covariance estimation in low-sample scenarios, employing a structured covariance matrix with shrinkage methods. These involve convexly combining a…”
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First observation of a quadruple asteroid -- Detection of a third moon around (130) Elektra with SPHERE/IFS by Berdeu, Anthony, Langlois, Maud, Vachier, Frédéric

“…A&A 658 L4 (2022) Aims. We aim to increase the contrast limits to detect new satellites orbiting known asteroids. We use cutting-edge data reduction techniques…”
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PACOME: Optimal multi-epoch combination of direct imaging observations for joint exoplanet detection and orbit estimation by Dallant, Jules, Langlois, Maud, Flasseur, Olivier, Thiébaut, Éric

“…A&A 679, A38 (2023) Exoplanet detections and characterizations via direct imaging require high contrast and high angular resolution. These requirements…”
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Analytical modelling of adaptive optics systems: Role of the influence function by Berdeu, Anthony, Tallon, Michel, Thiébaut, Éric, Langlois, Maud

“…Astronomy and Astrophysics - A&A, 2023, 674, pp.A112 Context. Adaptive optics (AO) is now a tool commonly deployed in astronomy. The real time correction of…”
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Blind and robust reconstruction of adaptive optics point spread functions for asteroid deconvolution and moon detection by Berdeu, Anthony, Soulez, Férréol, Minker, Kate, Carry, Benoit, Bourdarot, Guillaume, Kaszczyc, Antoine, Langlois, Maud

“…Adaptive Optics Systems IX, Jun 2024, Yokohama, Japan. pp.235 Initially designed to detect and characterize exoplanets, extreme adaptive optics systems (AO)…”
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MODEL&CO: Exoplanet detection in angular differential imaging by learning across multiple observations by Bodrito, Théo, Flasseur, Olivier, Mairal, Julien, Ponce, Jean, Langlois, Maud, Lagrange, Anne-Marie

“…Direct imaging of exoplanets is particularly challenging due to the high contrast between the planet and the star luminosities, and their small angular…”
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