Search Results - "Xompero, M."

A high-resolution image of the inner shell of the P Cygni nebula in the infrared [Fe ii] line by Arcidiacono, C., Ragazzoni, R., Morossi, C., Franchini, M., Marcantonio, P. Di, Kulesa, C., McCarthy, D., Briguglio, R., Xompero, M., Busoni, L., Quirós-Pacheco, F., Pinna, E., Boutsia, K., Paris, D.

“…Using the adaptive optics system of the Large Binocular Telescope, we have obtained near-infrared camera PISCES images of the inner shell of the nebula around…”
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HIGH RESOLUTION Hα IMAGES OF THE BINARY LOW-MASS PROPLYD LV 1 WITH THE MAGELLAN AO SYSTEM by Wu, Y-L, Close, L M, Males, J R, Follette, K, Morzinski, K, KOPON, D, RODIGAS, T J, Hinz, P, Puglisi, A, Esposito, S, Pinna, E, Riccardi, A, Xompero, M, Briguglio, R

“…We utilize the new Magellan adaptive optics system (MagAO) to image the binary proplyd LV 1 in the Orion Trapezium at H alpha . This is among the first AO…”
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HIGH-RESOLUTION IMAGES OF ORBITAL MOTION IN THE ORION TRAPEZIUM CLUSTER WITH THE LBT AO SYSTEM by CLOSE, L. M, PUGLISI, A, RICCARDI, A, MCCARTHY, D. W, XOMPERO, M, KULESA, C, QUIROS-PACHECO, F, ARGOMEDO, J, BRYNNEL, J, ESPOSITO, S, MANNUCCI, F, BOUTSIA, K, MALES, J. R, FINI, L, THOMPSON, D. J, HILL, J. M, WOODWARD, C. E, BRIGUGLIO, R, RODIGAS, T. J, STEFANINI, P, AGAPITO, G, HINZ, P, ARCIDIACONO, C, FOLLETTE, K, GREEN, R, SKEMER, A, GUERRA, J. C, BUSONI, L, BRUSA, G, PINNA, E, MILLER, D. L

“…The new 8.4 m LBT adaptive secondary AO system, with its novel pyramid wavefront sensor, was used to produce very high Strehl ([> ~]75% at 2.16 mu m)…”
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DIFFRACTION-LIMITED VISIBLE LIGHT IMAGES OF ORION TRAPEZIUM CLUSTER WITH THE MAGELLAN ADAPTIVE SECONDARY ADAPTIVE OPTICS SYSTEM (MagAO) by Close, L M, Males, J R, Morzinski, K, KOPON, D, Follette, K, RODIGAS, T J, Hinz, P, Wu, Y-L, Puglisi, A, Esposito, S

“…We utilized the new high-order (250-378 mode) Magellan Adaptive Optics system (MagAO) to obtain very high spatial resolution observations in "visible light"…”
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THE ABSOLUTE AGE OF THE GLOBULAR CLUSTER M15 USING NEAR-INFRARED ADAPTIVE OPTICS IMAGES FROM PISCES/LBT by Monelli, M, Testa, V, Bono, G, Ferraro, I, Iannicola, G, Fiorentino, G, Arcidiaconct, C, Massari, D, Boutsia, K, Briguglio, R

“…We present deep near-infrared J, K sub(s) photometry of the old, metal-poor Galactic globular cluster M15 obtained with images collected with the LUCI1 and…”
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THE ABSOLUTE AGE OF THE GLOBULAR CLUSTER M15 USING NEAR-INFRARED ADAPTIVE OPTICS IMAGES FROM PISCES/LBT Observations were carried out using the Large Binocular Telescope at Mount Graham, AZ. The LBT is an international collaboration among institutions in the United States, Italy, and Germany. LBT Corporation partners are the University of Arizona on behalf of the Arizona university system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max-Planc by Monelli, M., Testa, V., Bono, G., Ferraro, I., Iannicola, G., Fiorentino, G., Arcidiacono, C., Massari, D., Boutsia, K., Briguglio, R., Busoni, L., Carini, R., Close, L., Cresci, G., Esposito, S., Fini, L., Fumana, M., Guerra, J. C., Hill, J., Kulesa, C., Mannucci, F., McCarthy, D., Pinna, E., Puglisi, A., Quiros-Pacheco, F., Ragazzoni, R., Riccardi, A., Skemer, A., Xompero, M.

“…ABSTRACT We present deep near-infrared J, photometry of the old, metal-poor Galactic globular cluster M15 obtained with images collected with the LUCI1 and…”
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HIGH RESOLUTION H{alpha} IMAGES OF THE BINARY LOW-MASS PROPLYD LV 1 WITH THE MAGELLAN AO SYSTEM by Wu, Y.-L., Close, L. M., Males, J. R., Follette, K., Morzinski, K., Kopon, D., Rodigas, T. J., Hinz, P., Puglisi, A., Esposito, S., Pinna, E., Riccardi, A., Xompero, M., Briguglio, R.

“…We utilize the new Magellan adaptive optics system (MagAO) to image the binary proplyd LV 1 in the Orion Trapezium at H{alpha}. This is among the first AO…”
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GMP-selected dual and lensed AGNs: selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, KECK/OSIRIS, and LBT/LUCI by Mannucci, F, Scialpi, M, Ciurlo, A, Yeh, S, Marconcini, C, Tozzi, G, Cresci, G, Marconi, A, Amiri, A, Belfiore, F, Carniani, S, Cicone, C, Nardini, E, Pancino, E, Rubinur, K, Severgnini, P, Ulivi, L, Venturi, G, Vignali, C, Volonteri, M, Pinna, E, Rossi, F, Puglisi, A, Agapito, G, Plantet, C, Ghose, E, Carbonaro, L, Xompero, M, Grani, P, Esposito, S, Power, J, Ramon, J. C. Guerra, Lefebvre, M, Cavallaro, A, Davies, R, Riccardi, A, Macintosh, M, Taylor, W, Dolci, M, Baruffolo, A, Feuchtgruber, H, Kravchenko, K, Rau, C, Sturm, E, Wiezorrek, E, Dallilar, Y, Kenworthy, M

“…The Gaia-Multi-Peak (GMP) technique can be used to identify large numbers of dual or lensed AGN candidates at sub-arcsec separation, allowing us to study both…”
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The Enhanced Resolution Imager and Spectrograph for the VLT by Davies, R, Absil, O, Agapito, G, Berbel, A. Agudo, Baruffolo, A, Biliotti, V, Bonaglia, M, Bonse, M, Briguglio, R, Campana, P, Cao, Y, Carbonaro, L, Cortes, A, Cresci, G, Dallilar, Y, Dannert, F, De Rosa, R. J, Deysenroth, M, Di Antonio, I, Di Cianno, A, Di Rico, G, Doelman, D, Dolci, M, Dorn, R, Eisenhauer, F, Esposito, S, Fantinel, D, Ferruzzi, D, Feuchtgruber, H, Finger, G, Schreiber, N. M. Förster, Gao, X, Gemperlein, H, Genzel, R, Gillessen, S, Ginski, C, Glauser, A. M, Glindemann, A, Grani, P, Hartl, M, Hayoz, J, Heida, M, Henry, D, Hofmann, R, Huber, H, Kasper, M, Keller, C, Kenworthy, M, Kravchenko, K, Kuntschner, H, Lacour, S, Lightfoot, J, Lunney, D, Lutz, D, Macintosh, M, Mannucci, F, Marsset, M, Modigliani, A, Neeser, M, de Xivry, G. Orban, Ott, T, Pallanca, L, Patapis, P, Pearson, D, Peña, E, Percheron, I, Puglisi, A, Quanz, S. P, Rabien, S, Rau, C, Riccardi, A, Salasnich, B, Schmid, H. -M, Schubert, J, Serra, B, Shimizu, T, Snik, F, Sturm, E, Tacconi, L, Taylor, W, Valentini, A, Waring, C, Wiezorrek, E, Xompero, M

“…ERIS, the Enhanced Resolution Imager and Spectrograph, is an instrument that both extends and enhances the fundamental diffraction limited imaging and…”
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The ERIS Adaptive Optics System by Riccardi, A, Esposito, S, Agapito, G, Antichi, J, Biliotti, V, Blain, C, Briguglio, R, Busoni, L, Carbonaro, L, Di Rico, G, Giordano, C, Pinna, E, Puglisi, A, Spanò, P, Xompero, M, Baruffolo, A, Kasper, M, Egner, S, Valles, M. Suàrez, Soenke, C, Downing, M, Reyes, J

“…Proc. SPIE Vol. 9909 (2016) ERIS is the new AO instrument for VLT-UT4 led by a Consortium of Max-Planck Institut fuer Extraterrestrische Physik, UK-ATC,…”
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The absolute age of the globular cluster M15 using near-infrared adaptive optics images from PISCES/LBT by Monelli, M, Testa, V, Bono, G, Ferraro, I, Iannicola, G, Fiorentino, G, Arcidiacono, C, Massari, D, Boutsia, K, Briguglio, R, Busoni, L, Carini, R, Close, L, Cresci, G, Esposito, S, Fini, L, Fumana, M, Guerra, J. C, Hill, J, Kulesa, C, Mannucci, F, McCarthy, D, Pinna, E, Puglisi, A, Quiros-Pacheco, F, Ragazzoni, R, Riccardi, A, Skemer, A, Xompero, M

“…We present deep near-infrared (NIR) J, Ks photometry of the old, metal-poor Galactic globular cluster M\,15 obtained with images collected with the LUCI1 and…”
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Discovery of H-alpha Emission from the Close Companion Inside the Gap of Transitional Disk HD142527 by Close, L. M, Follette, K. B, Males, J. R, Puglisi, A, Xompero, M, Apai, D, Najita, J, Weinberger, A. J, Morzinski, K, Rodigas, T. J, Hinz, P, Bailey, V, Briguglio, R

“…We utilized the new high-order 585 actuator Magellan Adaptive Optics system (MagAO) to obtain very high-resolution visible light images of HD142527 with…”
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High Resolution H alpha Images of the Binary Low-mass Proplyd LV 1 with the Magellan AO System by Wu, Y. -L, Close, L. M, Males, J. R, Follette, K, Morzinski, K, Kopon, D, Rodigas, T. J, Hinz, P, Puglisi, A, Esposito, S, Pinna, E, Riccardi, A, Xompero, M, Briguglio, R

“…Wu et al. 2013, ApJ, 774, 45 We utilize the new Magellan adaptive optics system (MagAO) to image the binary proplyd LV 1 in the Orion Trapezium at H alpha…”
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Diffraction-limited Visible Light Images of Orion Trapezium Cluster With the Magellan Adaptive Secondary AO System (MagAO) by Close, L. M, Males, J. R, Morzinski, K, Kopon, D, Follette, K, Rodigas, T. J, Hinz, P, Wu, Y-L, Puglisi, A, Esposito, S, Riccardi, A, Pinna, E, Xompero, M, Briguglio, R, Uomoto, A, Hare, T

“…We utilized the new high-order (250-378 mode) Magellan Adaptive Optics system (MagAO) to obtain very high spatial resolution observations in "visible light"…”
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LBT observations of the HR 8799 planetary system: First detection of HR8799e in H band by 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…”
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High Resolution Images of Orbital Motion in the Orion Trapezium Cluster with the LBT Adaptive Optics System by 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…”
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