Search Results - "Dannert, Felix A."

Mid-infrared Spectrum of the Disk around the Forming Companion GQ Lup B Revealed by JWST/MIRI by Cugno, Gabriele, Patapis, Polychronis, Banzatti, Andrea, Meyer, Michael, Dannert, Felix A., Stolker, Tomas, MacDonald, Ryan J., Pontoppidan, Klaus M.

“…GQ Lup B is a forming brown dwarf companion ( M ∼ 10–30 M J ) showing evidence for an infrared excess associated with a disk surrounding the companion itself…”
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Comparing Apples with Apples: Robust Detection Limits for Exoplanet High-contrast Imaging in the Presence of Non-Gaussian Noise by Bonse, Markus J., Garvin, Emily O., Gebhard, Timothy D., Dannert, Felix A., Cantalloube, Faustine, Cugno, Gabriele, Absil, Olivier, Hayoz, Jean, Milli, Julien, Kasper, Markus, Quanz, Sascha P.

“…Over the past decade, hundreds of nights have been spent on the world’s largest telescopes to search for and directly detect new exoplanets using high-contrast…”
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Use the 4S (Signal-Safe Speckle Subtraction): Explainable Machine Learning reveals the Giant Exoplanet AF Lep b in High-Contrast Imaging Data from 2011 by Bonse, Markus J, Gebhard, Timothy D, Dannert, Felix A, Absil, Olivier, Cantalloube, Faustine, Christiaens, Valentin, Cugno, Gabriele, Garvin, Emily O, Hayoz, Jean, Kasper, Markus, Matthews, Elisabeth, Schölkopf, Bernhard, Quanz, Sascha P

“…The main challenge of exoplanet high-contrast imaging (HCI) is to separate the signal of exoplanets from their host stars, which are many orders of magnitude…”
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Mid-Infrared Spectrum of the Disk around the Forming Companion GQ Lup B Revealed by JWST/MIRI by Cugno, Gabriele, Patapis, Polychronis, Banzatti, Andrea, Meyer, Michael, Dannert, Felix A, Stolker, Tomas, MacDonald, Ryan J, Pontoppidan, Klaus M

“…GQ Lup B is a forming brown dwarf companion ($M\sim10-30~M_J$) showing evidence for an infrared excess associated with a disk surronding the companion itself…”
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Comparing Apples with Apples: Robust Detection Limits for Exoplanet High-Contrast Imaging in the Presence of non-Gaussian Noise by Bonse, Markus J, Garvin, Emily O, Gebhard, Timothy D, Dannert, Felix A, Cantalloube, Faustine, Cugno, Gabriele, Absil, Olivier, Hayoz, Jean, Milli, Julien, Kasper, Markus, Quanz, Sascha P

“…Over the past decade, hundreds of nights have been spent on the worlds largest telescopes to search for and directly detect new exoplanets using high-contrast…”
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CROCODILE \\ Incorporating medium-resolution spectroscopy of close-in directly imaged exoplanets into atmospheric retrievals via cross-correlation by Hayoz, Jean, Cugno, Gabriele, Quanz, Sascha P, Patapis, Polychronis, Alei, Eleonora, Bonse, Markus J, Dannert, Felix A, Garvin, Emily O, Gebhard, Timothy D, Konrad, Björn S, Sartori, Lia F

“…A&A 678, A178 (2023) The investigation of the atmospheres of closely separated, directly imaged gas giant exoplanets is challenging due to the presence of…”
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Asgard/NOTT: L-band nulling interferometry at the VLTI I. Simulating the expected high-contrast performance by Laugier, Romain, Defrère, Denis, Courtney-Barrer, Benjamin, Dannert, Felix A, Matter, Alexis, Dandumont, Colin, Gross, Simon, Absil, Olivier, Bigioli, Azzurra, Garreau, Germain, Labadie, Lucas, Loicq, Jérôme, Martinod, Marc-Antoine, Mazzoli, Alexandra, Raskin, Gert, Sanny, Ahmed

“…A&A 671, A110 (2023) Context: NOTT (formerly Hi-5) is a new high-contrast L' band (3.5-4.0 \textmu m) beam combiner for the VLTI with the ambitious goal to be…”
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Large Interferometer For Exoplanets (LIFE). XIV. Finding terrestrial protoplanets in the galactic neighborhood by Cesario, Lorenzo, Lichtenberg, Tim, Alei, Eleonora, Carrión-González, Óscar, Dannert, Felix A, Defrère, Denis, Ertel, Steve, Fortier, Andrea, Muñoz, A. García, Glauser, Adrian M, Hansen, Jonah T, Helled, Ravit, Huber, Philipp A, Ireland, Michael J, Kammerer, Jens, Laugier, Romain, Lillo-Box, Jorge, Menti, Franziska, Meyer, Michael R, Noack, Lena, Quanz, Sascha P, Quirrenbach, Andreas, Rugheimer, Sarah, van der Tak, Floris, Wang, Haiyang S, Anger, Marius, Balsalobre-Ruza, Olga, Bhattarai, Surendra, Braam, Marrick, Castro-González, Amadeo, Cockell, Charles S, Constantinou, Tereza, Cugno, Gabriele, Davoult, Jeanne, Güdel, Manuel, Hernitschek, Nina, Hinkley, Sasha, Itoh, Satoshi, Janson, Markus, Johansen, Anders, Jones, Hugh R. A, Kane, Stephen R, van Kempen, Tim A, Kislyakova, Kristina G, Korth, Judith, Kovacevic, Andjelka B, Kraus, Stefan, Kuiper, Rolf, Mathew, Joice, Matsuo, Taro, Miguel, Yamila, Min, Michiel, Navarro, Ramon, Ramirez, Ramses M, Rauer, Heike, Ricketti, Berke Vow, Romagnolo, Amedeo, Schlecker, Martin, Sneed, Evan L, Squicciarini, Vito, Stassun, Keivan G, Tamura, Motohide, Viudez-Moreiras, Daniel, Wordsworth, Robin D, Collaboration, the LIFE

“…The increased brightness temperature of young rocky protoplanets during their magma ocean epoch makes them potentially amenable to atmospheric characterization…”
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