Zobrazeno 1 - 10
of 165
pro vyhledávání: '"Van Boekel, Roy"'
Autor:
Absil, Olivier, Kenworthy, Matthew, Delacroix, Christian, de Xivry, Gilles Orban, König, Lorenzo, Pathak, Prashant, Doelman, David, Por, Emiel, Snik, Frans, Born, Joost van den, Cantalloube, Faustine, Carlotti, Alexis, Courtney-Barrer, Benjamin, Forsberg, Pontus, Karlsson, Mikael, Bertram, Thomas, van Boekel, Roy, Dolkens, Dennis, Feldt, Markus, Glauser, Adrian M., Pantin, Eric, Quanz, Sascha P., Bettonvil, Felix, Brandl, Bernhard
Publikováno v:
Proceedings of the SPIE, Volume 13096, id. 13096-192 (2024)
The Mid-infrared ELT Imager and Spectrograph (METIS) is one of the first-generation scientific instruments for the ELT, built under the supervision of ESO by a consortium of research institutes across and beyond Europe. Designed to cover the 3 to 13
Externí odkaz:
http://arxiv.org/abs/2407.10588
Autor:
Bowens, Rory, Meyer, Michael R., Tobin, Taylor L., Viges, Eric, Hart, Dennis, Monnier, John, Leisenring, Jarron, Ives, Derek, van Boekel, Roy
New longwave HgCdTe detectors are critical to upcoming plans for ground-based infrared astronomy. These detectors, with fast-readouts and deep well-depths, will be key components of extremely large telescope instruments and therefore must be well und
Externí odkaz:
http://arxiv.org/abs/2405.20440
Autor:
Ramirez-Tannus, María Claudia, Bik, Arjan, Cuijpers, Lars, Waters, Rens, Goppl, Christiane, Henning, Thomas, Kamp, Inga, Preibisch, Thomas, Getman, Konstantin V., Chaparro, Germán, Cuartas-Restrepo, Pablo, de Koter, Alex, Feigelson, Eric D., Grant, Sierra L., Haworth, Thomas J., Hernández, Sebastián, Kuhn, Michael A., Perotti, Giulia, Povich, Matthew S., Reiter, Megan, Roccatagliata, Veronica, Sabbi, Elena, Tabone, Benoît, Winter, Andrew J., McLeod, Anna F., van Boekel, Roy, van Terwisga, Sierk E.
We present the first results of the eXtreme UV Environments (XUE) James Webb Space Telescope (JWST) program, that focuses on the characterization of planet forming disks in massive star forming regions. These regions are likely representative of the
Externí odkaz:
http://arxiv.org/abs/2310.11074
Autor:
Shi, Yaqing, Wang, Wei, Zhao, Gang, Zhai, Meng, Chen, Guo, Jiang, Zewen, Ouyang, Qinglin, Henning, Thomas, Zhao, Jingkun, Crouzet, Nicolas, van Boekel, Roy
Hot Jupiters, particularly those with temperature higher than 2000 K are the best sample of planets that allow in-depth characterization of their atmospheres. We present here a thermal emission study of the ultra hot Jupiter WASP-103 b observed in tw
Externí odkaz:
http://arxiv.org/abs/2303.13732
Autor:
Yoffe, Gideon, van Boekel, Roy, Li, Aigen, Waters, L. B. F. M, Maaskant, Koen, Siebenmorgen, Ralf, Ancker, Mario van den, de la Roche, D. J. M Petit dit, Lopez, Bruno, Matter, Alexis, Varga, Jozsef, Hogerheijde, M. R, Weigelt, Gerd, Oudmaijer, R. D, Pantin, Eric, Meyer, M. R, Augereau, Jean-Charles, Henning, Thomas
Publikováno v:
A&A 674, A57 (2023)
We use the long-slit spectroscopy mode of the VISIR-NEAR experiment to perform diffraction-limited observations of eight nearby Herbig Ae protoplanetary disks. We extract spectra for various locations along the slit with a spectral resolution of R =
Externí odkaz:
http://arxiv.org/abs/2303.06592
Autor:
Padovani, Paolo, Cirasuolo, Michele, van der Burg, Remco, Cantalloube, Faustine, George, Elizabeth, Kasper, Markus, Leschinski, Kieran, Martins, Carlos, Milli, Julien, Möhler, Sabine, Neeser, Mark, Neichel, Benoit, Otarola, Angel, Sánchez-Janssen, Rubén, Serra, Benoit, Smette, Alain, Valenti, Elena, Verinaud, Christophe, Vernet, Joël, Absil, Olivier, Agapito, Guido, Andersen, Morten, Arcidiacono, Carmelo, Arko, Matej, Baudoz, Pierre, Beltramo-Martin, Olivier, Biancalani, Enrico, Bierwirth, Thomas, Burtscher, Leonard, Carlà, Giulia, Castro-Almazán, Julio A., Cheffot, Anne-Laure, Coccato, Lodovico, Correia, Carlos, Fetick, Romain, Fiorentino, Giuliana, Fusco, Thierry, García-Lorenzo, Begoña, Fusillo, Nicola Gentile, Gonzalez, Oscar, Grazian, Andrea, Gullieuszik, Marco, Hainaut, Olivier, Ivanov, Valentin, Kaasinen, Melanie, Kaddad, Darshan, Kamiński, Tomasz, Kausch, Wolfgang, Kerber, Florian, Kimeswenger, Stefan, Kokotanekova, Rosita, Kuznetsov, Arseniy, Lau, Alexis, Louarn, Miska Le, Lemmel, Frédéric, Liske, Jochen, Curto, Gaspare Lo, Lucsanyi, David, Lundin, Lars, Noll, Stefan, Oberti, Sylvain, Osborn, James, Masciadri, Elena, Milaković, Dinko, Murphy, Michael T., Pedichini, Fernando, Santaella, Miguel Pereira, Piazzesi, Roberto, López, Javier Piqueras, Plantet, Cédric, Prod'homme, Thibaut, Przybilla, Norbert, Puech, Mathieu, Reid, Derryck T., Reiners, Ansgar, Rijnenberg, Rutger, Rodrigues, Myriam, Rossi, Fabio, Routledge, Laurence, Smit, Hans, Tecza, Mathias, Thatte, Niranjan, van Boekel, Roy, Verma, Aprajita, Vigan, Arthur
Publikováno v:
The Messenger, vol. 189, (December 2022) p. 23-30
Since 2005 ESO has been working with its community and industry to develop an extremely large optical/infrared telescope. ESO's Extremely Large Telescope, or ELT for short, is a revolutionary ground-based telescope that will have a 39-metre main mirr
Externí odkaz:
http://arxiv.org/abs/2302.14375
Autor:
Flores-Rivera, Lizxandra, Flock, Mario, Kurtovic, Nicolás, Husemann, Bernd, Banzatti, Andrea, Ringqvist, Simon C., Kamann, Sebastian, Müller, André, Fendt, Christian, Lopez, Rebeca Garcia, Marleau, Gabriel-Dominique, Henning, Thomas, Carrasco-Gonzalez, Carlos, van Boekel, Roy, Keppler, Miriam, Launhardt, Ralf, Aoyama, Yuhiko
Forbidden emission lines in protoplanetary disks are a key diagnostic in studies of the evolution of the disk and the host star. We report spatially resolved emission lines, [OI] 6300, 6363, [NII] 6548, 6583, H$\alpha$, and [SII] 6716, 6730 Angstrom
Externí odkaz:
http://arxiv.org/abs/2301.02559
Autor:
Absil, Olivier, Delacroix, Christian, de Xivry, Gilles Orban, Pathak, Prashant, Willson, Matthew, Berio, Philippe, van Boekel, Roy, Matter, Alexis, Defrere, Denis, Burtscher, Leo, Woillez, Julien, Brandl, Bernhard
Publikováno v:
Proceedings of the SPIE, Volume 12185, id. 1218511 (2022)
The high-speed variability of the local water vapor content in the Earth atmosphere is a significant contributor to ground-based wavefront quality throughout the infrared domain. Unlike dry air, water vapor is highly chromatic, especially in the mid-
Externí odkaz:
http://arxiv.org/abs/2210.12412
Autor:
Drevon, Julien, Millour, Florentin, Cruzalèbes, Pierre, Paladini, Claudia, Hron, Josef, Meilland, A., Allouche, F., Hofmann, K. -H., Lagarde, S., Lopez, B., Matter, A., Petrov, R., Robbe-Dubois, S., Schertl, D., Wittkowski, M., Zins, G., Ábrahám, P., Antonelli, P., Beckmann, U., Berio, P., Bettonvil, F., Glindemann, A., Graser, U., Heininger, M., Henning, Thomas, Isbell, Jacob W., Jaffe, Walter, Labadie, Lucas, Leinert, Christoph, Lehmitz, Michael, Morel, Sébastien, Meisenheimer, Klaus, Soulain, Anthony, Varga, Josef, Weigelt, Gerd, Woillez, Julien, Augereau, Jean-Charles, van Boekel, Roy, Burtscher, Leonard, Danchi, William, Dominik, Carsten, Gamez-Rosas, Violetta, Hocdé, Vincent, Hogerheijde, M., Klarmann, Lucia, Kokoulina, Elena, Leftley, James, Stee, Ph., Vakili, Farrokh, Waters, Rens, Wolf, Sebastian, Yoffe, Gideon
AGB stars are one of the main sources of dust production in the Galaxy. However, it is not clear what this process looks like and where the dust is condensing in the circumstellar environment. By characterizing the location of the dust and the molecu
Externí odkaz:
http://arxiv.org/abs/2208.10845
We present a new optical transmission spectrum of the hot Jupiter HAT-P-1b based on two transits observed with the Double Spectrograph (DBSP) on the Palomar 200-inch (P200) telescope. The DBSP transmission spectrum, covering a wavelength range from 3
Externí odkaz:
http://arxiv.org/abs/2207.12563