Zobrazeno 1 - 10
of 1 350
pro vyhledávání: '"Furió P"'
Publikováno v:
J. Chem. Phys. 161, 034901 (2024)
Patchy particles are an intriguing subject of study and indeed a model system in the field of soft matter physics. In recent years, patchy particle models have been applied to describe a wide variety of systems, including colloidal crystals, macromol
Externí odkaz:
http://arxiv.org/abs/2409.18929
Recent advancements in deep learning have led to widespread use of techniques for audio content generation, notably employing Denoising Diffusion Probabilistic Models (DDPM) across various tasks. Among these, Foley Sound Synthesis is of particular in
Externí odkaz:
http://arxiv.org/abs/2409.09162
Autor:
Surfaro, Furio, Maier, Ralph, Pastryk, Kai-Florian, Zhang, Fajun, Schreiber, Frank, Roth, Roland
Publikováno v:
The Journal of Chemical Physics, 2023, 158.16
The osmotic second virial coefficient B2 is an important parameter to describe the interactions and phase behavior of protein solutions, including colloidal systems and macromolecular solutions. Another key parameter to describe the driving force of
Externí odkaz:
http://arxiv.org/abs/2409.15347
Autor:
De Furio, Matthew, Meyer, Michael R., Greene, Thomas, Hodapp, Klaus, Johnstone, Doug, Leisenring, Jarron, Rieke, Marcia, Robberto, Massimo, Roellig, Thomas, Cugno, Gabriele, Fiorellino, Eleonora, Manara, Carlo, Raileanu, Roberta, van Terwisga, Sierk
A successful theory of star formation should predict the number of objects as a function of their mass produced through star-forming events. Previous studies in star-forming regions and the solar neighborhood identify a mass function increasing from
Externí odkaz:
http://arxiv.org/abs/2409.04624
Autor:
Langeveld, Adam B., Scholz, Aleks, Mužić, Koraljka, Jayawardhana, Ray, Capela, Daniel, Albert, Loïc, Doyon, René, Flagg, Laura, de Furio, Matthew, Johnstone, Doug, Lafrèniere, David, Meyer, Michael
The discovery and characterization of free-floating planetary-mass objects (FFPMOs) is fundamental to our understanding of star and planet formation. Here we report results from an extremely deep spectroscopic survey of the young star cluster NGC1333
Externí odkaz:
http://arxiv.org/abs/2408.12639
Autor:
Lawson, Kellen, Schlieder, Joshua E., Leisenring, Jarron M., Bogat, Ell, Beichman, Charles A., Bryden, Geoffrey, Gáspár, András, Groff, Tyler D., McElwain, Michael W., Meyer, Michael R., Barclay, Thomas, Calissendorff, Per, De Furio, Matthew, Li, Yiting, Rieke, Marcia J., Ygouf, Marie, Greene, Thomas P., Girard, Julien H., Gennaro, Mario, Kammerer, Jens, Rest, Armin, Roellig, Thomas L., Sunnquist, Ben
Observations of debris disks offer important insights into the formation and evolution of planetary systems. Though M dwarfs make up approximately 80% of nearby stars, very few M-dwarf debris disks have been studied in detail -- making it unclear how
Externí odkaz:
http://arxiv.org/abs/2405.00573
Autor:
Blakely, Dori, Johnstone, Doug, Cugno, Gabriele, Sivaramakrishnan, Anand, Tuthill, Peter, Dong, Ruobing, Pope, Benjamin J. S., Albert, Loïc, Charles, Max, Cooper, Rachel A., De Furio, Matthew, Desdoigts, Louis, Doyon, René, Francis, Logan, Greenbaum, Alexandra Z., Lafrenière, David, Lloyd, James P., Meyer, Michael R., Pueyo, Laurent, Ray, Shrishmoy, Sánchez-Bermúdez, Joel, Soulain, Anthony, Thatte, Deepashri, Vandal, Thomas
We observed the planet-hosting system PDS 70 with the James Webb Interferometer, JWST's Aperture Masking Interferometric (AMI) mode within NIRISS. Observing with the F480M filter centered at 4.8 $\mu$m, we simultaneously fit a geometric model to the
Externí odkaz:
http://arxiv.org/abs/2404.13032
We show that the principal types of the closed terms of the affine fragment of $\lambda$-calculus, with respect to a simple type discipline, are structurally isomorphic to their interpretations, as partial involutions, in a natural Geometry of Intera
Externí odkaz:
http://arxiv.org/abs/2402.07230
Autor:
Lew, Ben W. P., Roellig, Thomas, Batalha, Natasha E., Line, Michael, Greene, Thomas, Murkherjee, Sagnick, Freedman, Richard, Meyer, Michael, Beichman, Charles, De Oliveira, Catarina Alves, De Furio, Matthew, Johnstone, Doug, Greenbaum, Alexandra Z., Marley, Mark, Fortney, Jonathan J., Young, Erick T., Leisenring, Jarron, Boyer, Martha, Hodapp, Klaus, Misselt, Karl, Stansberry, John, Rieke, Marcia
The launch of the James Webb Space Telescope (JWST) marks a pivotal moment for precise atmospheric characterization of Y dwarfs, the coldest brown dwarf spectral type. In this study, we leverage moderate spectral resolution observations (R $\sim$ 270
Externí odkaz:
http://arxiv.org/abs/2402.05900
Autor:
Petrus, Simon, Whiteford, Niall, Patapis, Polychronis, Biller, Beth A., Skemer, Andrew, Hinkley, Sasha, Suárez, Genaro, Lueber, Anna, Palma-Bifani, Paulina, Stone, Jordan M., Vos, Johanna M., Morley, Caroline V., Tremblin, Pascal, Charnay, Benjamin, Helling, Christiane, Miles, Brittany E., Carter, Aarynn L., Wang, Jason J., Janson, Markus, Gonzales, Eileen C., Sutlieff, Ben, Hoch, Kielan K. W., Bonnefoy, Mickaël, Chauvin, Gaël, Absil, Olivier, Balmer, William O., Boccaletti, Anthony, Bonavita, Mariangela, Booth, Mark, Bowler, Brendan P., Briesemeister, Zackery W., Bryan, Marta L., Calissendorff, Per, Cantalloube, Faustine, Chen, Christine H., Choquet, Elodie, Christiaens, Valentin, Cugno, Gabriele, Currie, Thayne, Danielski, Camilla, De Furio, Matthew, Dupuy, Trent J., Factor, Samuel M., Faherty, Jacqueline K., Fitzgerald, Michael P., Fortney, Jonathan J., Franson, Kyle, Girard, Julien H., Grady, Carol A., Henning, Thomas, Hines, Dean C., Hood, Callie E., Howe, Alex R., Kalas, Paul, Kammerer, Jens, Kennedy, Grant M., Kenworthy, Matthew A., Kervella, Pierre, Kim, Minjae, Kitzmann, Daniel, Kraus, Adam L., Kuzuhara, Masayuki, Lagage, Pierre-Olivier, Lagrange, Anne-Marie, Lawson, Kellen, Lazzoni, Cecilia, Leisenring, Jarron M., Lew, Ben W. P., Liu, Michael C., Liu, Pengyu, Llop-Sayson, Jorge, Lloyd, James P., Macintosh, Bruce, Mâlin, Mathilde, Manjavacas, Elena, Marino, Sebastián, Marley, Mark S., Marois, Christian, Martinez, Raquel A., Matthews, Elisabeth C., Matthews, Brenda C., Mawet, Dimitri, Mazoyer, Johan, McElwain, Michael W., Metchev, Stanimir, Meyer, Michael R., Millar-Blanchaer, Maxwell A., Mollière, Paul, Moran, Sarah E., Mukherjee, Sagnick, Pantin, Eric, Perrin, Marshall D., Pueyo, Laurent, Quanz, Sascha P., Quirrenbach, Andreas, Ray, Shrishmoy, Rebollido, Isabel, Redai, Jea Adams, Ren, Bin B., Rickman, Emily, Sallum, Steph, Samland, Matthias, Sargent, Benjamin, Schlieder, Joshua E., Stapelfeldt, Karl R., Tamura, Motohide, Tan, Xianyu, Theissen, Christopher A., Uyama, Taichi, Vasist, Malavika, Vigan, Arthur, Wagner, Kevin, Ward-Duong, Kimberly, Wolff, Schuyler G., Worthen, Kadin, Wyatt, Mark C., Ygouf, Marie, Zurlo, Alice, Zhang, Xi, Zhang, Keming, Zhan, Zhoujian, Zhou, Yifan
The unprecedented medium-resolution (R~1500-3500) near- and mid-infrared (1-18um) spectrum provided by JWST for the young (140+/-20Myr) low-mass (12-20MJup) L-T transition (L7) companion VHS1256b gives access to a catalogue of molecular absorptions.
Externí odkaz:
http://arxiv.org/abs/2312.03852