Zobrazeno 1 - 10
of 424
pro vyhledávání: '"Brusa, G"'
Autor:
Crowe, S., Fedriani, R., Tan, J. C., Whittle, M., Zhang, Y., Garatti, A. Caratti o, Farias, J. P., Gautam, A., Telkamp, Z., Rothberg, B., Grudic, M., Andersen, M., Cosentino, G., Garcia-Lopez, R., Rosero, V., Tanaka, K., Pinna, E., Rossi, F., Miller, D., Agapito, G., Plantet, C., Ghose, E., Christou, J., Power, J., Puglisi, A., Briguglio, R., Brusa, G., Taylor, G., Zhang, X., Mazzoni, T., Bonaglia, M., Esposito, S., Veillet, C.
Methods: Broad- and narrow-band imaging of AFGL 5180 was made in the NIR with the LBT, in both seeing-limited ($\sim0.5\arcsec$) and high angular resolution ($\sim0.09\arcsec$) Adaptive Optics (AO) modes, as well as with HST. Archival ALMA continuum
Externí odkaz:
http://arxiv.org/abs/2311.11909
Autor:
Christou, J. C., Brusa, G., Conrad, A., Esposito, S., Herbst, T., Hinz, P., Hill, J. M., Miller, D. L., Rabien, S., Rahmer, G., Taylor, G. E., Veillet, C., Zhang, X.
We present an overview of the current and future adaptive optics systems at the LBTO along with the current and planned science instruments they feed. All the AO systems make use of the two 672 actuator adaptive secondary mirrors. They are (1) FLAO (
Externí odkaz:
http://hdl.handle.net/10150/622008
http://arizona.openrepository.com/arizona/handle/10150/622008
http://arizona.openrepository.com/arizona/handle/10150/622008
Autor:
Defrère, D., Hinz, P. M., Mennesson, B., Hoffmann, W. F., Millan-Gabet, R., Skemer, A. J., Bailey, V., Danchi, W. C., Downey, E. C., Durney, O., Grenz, P., Hill, J. M., McMahon, T. J., Montoya, M., Spalding, E., Vaz, A., Absil, O., Arbo, P., Bailey, H., Brusa, G., Bryden, G., Esposito, S., Gaspar, A., Haniff, C. A., Kennedy, G. M., Leisenring, J. M., Marion, L., Nowak, M., Pinna, E., Powell, K., Puglisi, A., Rieke, G., Roberge, A., Serabyn, E., Sosa, R., Stapeldfeldt, K., Su, K., Weinberger, A. J., Wyatt, M. C.
The Large Binocular Telescope Interferometer (LBTI) is a versatile instrument designed for high angular resolution and high-contrast infrared imaging (1.5-13 mu m). In this paper, we focus on the mid-infrared (8-13 mu m) nulling mode and present its
Externí odkaz:
http://hdl.handle.net/10150/621383
http://arizona.openrepository.com/arizona/handle/10150/621383
http://arizona.openrepository.com/arizona/handle/10150/621383
Autor:
Defrère, D., Hinz, P. M., Kennedy, G. M., Stone, J., Rigley, J., Ertel, S., Gaspar, A., Bailey, V. P., Hoffmann, W. F., Mennesson, B., Millan-Gabet, R., Danchi, W. C., Absil, O., Arbo, P., Beichman, C., Bonavita, M., Brusa, G., Bryden, G., Downey, E. C., Esposito, S., Grenz, P., Haniff, C., Hill, J. M., Leisenring, J. M., Males, J. R., McMahon, T. J., Montoya, M., Morzinski, K. M., Pinna, E., Puglisi, A., Rieke, G., Roberge, A., Rousseau, H., Serabyn, E., Spalding, E., Skemer, A. J., Stapelfeldt, K., Su, K., Vaz, A., Weinberger, A. J., Wyatt, M. C.
The young (50-400 Myr) A3V star $\beta$ Leo is a primary target to study the formation history and evolution of extrasolar planetary systems as one of the few stars with known hot ($\sim$1600$^\circ$K), warm ($\sim$600$^\circ$K), and cold ($\sim$120$
Externí odkaz:
http://arxiv.org/abs/2103.03268
Autor:
Antonello, M., Belov, A., Brusa, G. Bonomi R. S., Caccia, M., Camper, A., Caravita, R., Castelli, F., Comparat, D., Consolati, G., Di Noto, L., Doser, M., Fani, M., Ferragut, R., Fesel, J., Gerber, S., Gligorova, A., Glöggler, L. T., Guatieri, F., Haider, S., Hinterberger, A., Khalidova, O., Krasnicky, D., Lagomarsino, V., Malbrunot, C., Mariazzi, S., Matveev, V., Müller, S. R., Nebbia, G., Nedelec, P., Nowak, L., Oberthaler, M., Oswald, E., Pagano, D., Penasa, L., Petracek, V., Prelz, F., Rienäcker, B., Røhne, O. M., Rotondi, A., Sandaker, H., Santoro, R., Testera, G., Tietje, I. C., Wolz, T., Zimmer, C., Zurlo, N.
Publikováno v:
Phys. Rev. A 102, 013101 (2020)
We characterized the pulsed Rydberg-positronium production inside the AEgIS (Antimatter Experiment: Gravity, Interferometry, Spectroscopy) apparatus in view of antihydrogen formation by means of a charge exchange reaction between cold antiprotons and
Externí odkaz:
http://arxiv.org/abs/1911.04342
Autor:
Defrère, D., Hinz, P., Downey, E., Ashby, D., Bailey, V., Brusa, G., Christou, J., Danchi, W. C., Grenz, P., Hill, J. M., Hoffmann, W. F., Leisenring, J., Lozi, J., McMahon, T., Mennesson, B., Millan-Gabet, R., Montoya, M., Powell, K., Skemer, A., Vaitheeswaran, V., Vaz, A., Veillet, C.
Publikováno v:
Proc. SPIE 9146, Optical and Infrared Interferometry IV, 914609 (July 24, 2014)
The Large Binocular Telescope Interferometer is a NASA-funded nulling and imaging instrument designed to coherently combine the two 8.4-m primary mirrors of the LBT for high-sensitivity, high-contrast, and high-resolution infrared imaging (1.5-13 um)
Externí odkaz:
http://arxiv.org/abs/1501.04142
Autor:
Defrère, D., Hinz, P. M., Skemer, A. J., Kennedy, G. M., Bailey, V. P., Hoffmann, W. F., Mennesson, B., Millan-Gabet, R., Danchi, W. C., Absil, O., Arbo, P., Beichman, C., Brusa, G., Bryden, G., Downey, E. C., Durney, O., Esposito, S., Gaspar, A., Grenz, P., Haniff, C., Hill, J. M., Lebreton, J., Leisenring, J. M., Males, J. R., Marion, L., McMahon, T. J., Montoya, M., Morzinski, K. M., Pinna, E., Puglisi, A., Rieke, G., Roberge, A., Serabyn, E., Sosa, R., Stapeldfeldt, K., Su, K., Vaitheeswaran, V., Vaz, A., Weinberger, A. J., Wyatt, M. C.
Publikováno v:
The Astrophysical Journal, 799:42 (9pp), 2015 January 20
We report on the first nulling interferometric observations with the Large Binocular Telescope Interferometer (LBTI), resolving the N' band (9.81 - 12.41 um) emission around the nearby main-sequence star eta Crv (F2V, 1-2 Gyr). The measured source nu
Externí odkaz:
http://arxiv.org/abs/1501.04144
Autor:
Esposito, S., Mesa, D., Skemer, A., Arcidiacono, C., Claudi, R. U., Desidera, S., Gratton, R., Mannucci, F., Marzari, F., Masciadri, E., Close, L., Hinz, P., Kulesa, C., McCarthy, D., Males, J., Agapito, G., Argomedo, J., Boutsia, K., Briguglio, R., Brusa, G., Busoni, L., Cresci, G., Fini, L., Fontana, A., Guerra, J. C., Hill, J. M., Miller, D., Paris, D., Pinna, E., Puglisi, A., Quiros-Pacheco, F., Riccardi, A., Stefanini, P., Testa, V., Xompero, M., Woodward, C.
We have performed H and Ks band observations of the planetary system around HR 8799 using the new AO system at the Large Binocular Telescope and the PISCES Camera. The excellent instrument performance (Strehl ratios up to 80% in H band) enabled detec
Externí odkaz:
http://arxiv.org/abs/1203.2735
Autor:
Close, L. M., Puglisi, A., Males, J. R., Arcidiacono, C., Skemer, A., Guerra, J. C., Busoni, L., Brusa, G., Pinna, E., Miller, D. L., Riccardi, A., McCarthy, D. W., Xompero, M., Kulesa, C., Quiros-Pacheco, F., Argomedo, J., Brynnel, J., Esposito, S., Mannucci, F., Boutsia, K., Fini, L., Thompson, D. J., Hill, J. M., Woodward, C. E., Briguglio, R., Rodigas, T. J., Stefanini, P., Agapito, G., Hinz, P., Follette, K., Green, R.
The new 8.4m LBT adaptive secondary AO system, with its novel pyramid wavefront sensor, was used to produce very high Strehl (75% at 2.16 microns) near infrared narrowband (Br gamma: 2.16 microns and [FeII]: 1.64 microns) images of 47 young (~1 Myr)
Externí odkaz:
http://arxiv.org/abs/1203.2638
Autor:
Jackson, Kathryn J., Schmidt, Dirk, Vernet, Elise, Brusa, G., Zhang, X., Lefebvre, M., Tintori, M., Smithwright, M., Guerra, J. C., Miller, D., Taylor, G., Ragland, S.
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13097 Issue: 1 p130972M-130972M-10, 12966239p
