no code implementations • 9 Mar 2021 • R. Asensio-Torres, Th. Henning, F. Cantalloube, P. Pinilla, D. Mesa, A. Garufi, S. Jorquera, R. Gratton, G. Chauvin, J. Szulagyi, R. van Boekel, R. Dong, G. -D. Marleau, M. Benisty, M. Villenave, C. Bergez-Casalou, C. Desgrange, M. Janson, M. Keppler, M. Langlois, F. Menard, E. Rickman, T. Stolker, M. Feldt, T. Fusco, L. Gluck, A. Pavlov, J. Ramos
The detection of a wide range of substructures such as rings, cavities and spirals has become a common outcome of high spatial resolution imaging of protoplanetary disks, both in the near-infrared scattered light and in the thermal millimetre continuum emission.
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics
no code implementations • 21 Dec 2020 • J. Kammerer, M. Kasper, M. J. Ireland, R. Köhler, R. Laugier, F. Martinache, R. Siebenmorgen, M. E. van den Ancker, R. van Boekel, T. M. Herbst, E. Pantin, H. -U. Käufl, D. J. M. Petit dit de la Roche, V. D. Ivanov
We aim to measure the brightness of all three components of the T Tauri system (T Tau N, T Tau Sa, T Tau Sb) in the mid-infrared in order to obtain photometry around the $\sim 9. 7~\mu m$ silicate feature.
Solar and Stellar Astrophysics
no code implementations • 10 Dec 2020 • J. Varga, M. Hogerheijde, R. van Boekel, L. Klarmann, R. Petrov, L. B. F. M. Waters, S. Lagarde, E. Pantin, Ph. Berio, G. Weigelt, S. Robbe-Dubois, B. Lopez, F. Millour, J. -C. Augereau, H. Meheut, A. Meilland, Th. Henning, W. Jaffe, F. Bettonvil, P. Bristow, K. -H. Hofmann, A. Matter, G. Zins, S. Wolf, F. Allouche, F. Donnan, D. Schertl, C. Dominik, M. Heininger, M. Lehmitz, P. Cruzalèbes, A. Glindemann, K. Meisenheimer, C. Paladini, M. Schöller, J. Woillez, L. Venema, E. Kokoulina, G. Yoffe, P. Ábrahám, S. Abadie, R. Abuter, M. Accardo, T. Adler, T. Agócs, P. Antonelli, A. Böhm, C. Bailet, G. Bazin, U. Beckmann, J. Beltran, W. Boland, P. Bourget, R. Brast, Y. Bresson, L. Burtscher, R. Castillo, A. Chelli, C. Cid, J. -M. Clausse, C. Connot, R. D. Conzelmann, W. -C. Danchi, M. De Haan, M. Delbo, M. Ebert, E. Elswijk, Y. Fantei, R. Frahm, V. Gámez Rosas, A. Gabasch, A. Gallenne, E. Garces, P. Girard, F. Y. J. Gonté, J. C. González Herrera, U. Graser, P. Guajardo, F. Guitton, X. Haubois, J. Hron, N. Hubin, R. Huerta, J. W. Isbell, D. Ives, G. Jakob, A. Jaskó, L. Jochum, R. Klein, J. Kragt, G. Kroes, S. Kuindersma, L. Labadie, W. Laun, R. Le Poole, C. Leinert, J. -L. Lizon, M. Lopez, A. Mérand, A. Marcotto, N. Mauclert, T. Maurer, L. H. Mehrgan, J. Meisner, K. Meixner, M. Mellein, L. Mohr, S. Morel, L. Mosoni, R. Navarro, U. Neumann, E. Nußbaum, L. Pallanca, L. Pasquini, I. Percheron, J. -U. Pott, E. Pozna, A. Ridinger, F. Rigal, M. Riquelme, Th. Rivinius, R. Roelfsema, R. -R. Rohloff, S. Rousseau, N. Schuhler, M. Schuil, A. Soulain, P. Stee, C. Stephan, R. ter Horst, N. Tromp, F. Vakili, A. van Duin, J. Vinther, M. Wittkowski, F. Wrhel
In this study we aim to characterize the mid-infrared brightness distribution of the inner disk of the young intermediate-mass star HD 163296, from VLTI/MATISSE observations.
Solar and Stellar Astrophysics Earth and Planetary Astrophysics
3 code implementations • 25 Apr 2019 • P. Mollière, J. P. Wardenier, R. van Boekel, Th. Henning, K. Molaverdikhani, I. A. G. Snellen
The code is fast, accurate, and versatile; it can calculate both transmission and emission spectra within a few seconds at low resolution ($\lambda/\Delta\lambda$ = 1000; correlated-k method) and high resolution ($\lambda/\Delta\lambda = 10^6$; line-by-line method), using only a few lines of input instruction.
Earth and Planetary Astrophysics
