M
Marco Xompero
Researcher at INAF
Publications - 170
Citations - 4363
Marco Xompero is an academic researcher from INAF. The author has contributed to research in topics: Adaptive optics & Deformable mirror. The author has an hindex of 32, co-authored 147 publications receiving 3988 citations.
Papers
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Journal ArticleDOI
HD?106906?b: A Planetary-mass Companion Outside a Massive Debris Disk
Vanessa P. Bailey,Tiffany Meshkat,Megan Reiter,Katie M. Morzinski,Jared R. Males,Kate Y. L. Su,Philip M. Hinz,Matthew A. Kenworthy,Daniel P. Stark,Eric E. Mamajek,Runa Briguglio,Laird M. Close,Katherine B. Follette,Alfio Puglisi,Timothy J. Rodigas,Timothy J. Rodigas,Alycia J. Weinberger,Marco Xompero +17 more
TL;DR: In this paper, the Magellan Adaptive Optics (MAGAO) + Clio2 system was used to detect a planetary-mass companion, HD?106906 b, at a projected separation of 7''1 (650 AU).
Journal ArticleDOI
FIRST LIGHT LBT AO IMAGES OF HR 8799 bcde AT 1.6 AND 3.3 μm: NEW DISCREPANCIES BETWEEN YOUNG PLANETS AND OLD BROWN DWARFS*
Andrew J. Skemer,Philip M. Hinz,Simone Esposito,Adam Burrows,Jarron Leisenring,Michael F. Skrutskie,Silvano Desidera,Dino Mesa,Carmelo Arcidiacono,Filippo Mannucci,Timothy J. Rodigas,Laird M. Close,Donald W. McCarthy,Craig Kulesa,Guido Agapito,Daniel Apai,Javier Argomedo,Vanessa P. Bailey,K. Boutsia,Runa Briguglio,Guido Brusa,Lorenzo Busoni,Riccardo Claudi,Joshua Eisner,Luca Fini,Katherine B. Follette,Peter M. Garnavich,Raffaele Gratton,J. C. Guerra,John M. Hill,William F. Hoffmann,Terry J. Jones,M. Krejny,Jared R. Males,Elena Masciadri,Michael Meyer,Douglas L. Miller,Katie M. Morzinski,Matthew J. Nelson,Enrico Pinna,Alfio Puglisi,Sascha P. Quanz,Fernando Quiros-Pacheco,Armando Riccardi,P. Stefanini,Vidhya Vaitheeswaran,John C. Wilson,Marco Xompero +47 more
TL;DR: In this paper, the spectral energy distribution of the HR 8799 planets is modeled as a mixture of clouds of varying opacity, similar to the patchy cloud structures on Jupiter and L/T transition brown dwarfs.
Journal ArticleDOI
First Light LBT AO Images of HR 8799 bcde at 1.65 and 3.3 Microns: New Discrepancies between Young Planets and Old Brown Dwarfs
Andrew J. Skemer,Philip M. Hinz,Simone Esposito,Adam Burrows,Jarron Leisenring,Michael F. Skrutskie,Silvano Desidera,Dino Mesa,Carmelo Arcidiacono,Filippo Mannucci,Timothy J. Rodigas,Laird M. Close,Donald W. McCarthy,Craig Kulesa,Guido Agapito,Daniel Apai,Javier Argomedo,Vanessa P. Bailey,K. Boutsia,Runa Briguglio,Guido Brusa,Lorenzo Busoni,Riccardo Claudi,Joshua Eisner,Luca Fini,Katherine B. Follette,Peter M. Garnavich,Raffaele Gratton,Juan Carlos Guerra,John M. Hill,William F. Hoffmann,Terry Jones,Megan Krejny,Jared R. Males,Elena Masciadri,Michael Meyer,Douglas L. Miller,Katie M. Morzinski,Matthew J. Nelson,Enrico Pinna,Alfio Puglisi,Sascha P. Quanz,Fernando Quiros-Pacheco,Armando Riccardi,P. Stefanini,Vidhya Vaitheeswaran,John C. Wilson,Marco Xompero +47 more
TL;DR: In this paper, the authors used the LBT adaptive optics system, PISCES, and LBTI/LMIRCam to image all four of the HR 8799 planets at H-band and 3.3 microns.
Journal ArticleDOI
Discovery of H-alpha Emission from the Close Companion Inside the Gap of Transitional Disk HD142527
Laird M. Close,Katherine B. Follette,J. Males,Alfio Puglisi,Marco Xompero,Daniel Apai,Joan Najita,Alycia J. Weinberger,Katie M. Morzinski,T. J. Rodigas,P. M. Hinz,Vanessa P. Bailey,Runa Briguglio +12 more
TL;DR: In this paper, the Magellan Adaptive Optics System (MAGAO) was used to obtain very high-resolution visible light images of HD142527 with MagAO's VisAO science camera.
Proceedings ArticleDOI
First light AO (FLAO) system for LBT: final integration, acceptance test in Europe, and preliminary on-sky commissioning results
Simone Esposito,Armando Riccardi,Luca Fini,Alfio Puglisi,Enrico Pinna,Marco Xompero,Runa Briguglio,Fernando Quiros-Pacheco,P. Stefanini,Juan Carlos Guerra,Lorenzo Busoni,Andrea Tozzi,F. Pieralli,Guido Agapito,Guido Brusa-Zappellini,Richard A. Demers,Joar Brynnel,Carmelo Arcidiacono,Piero Salinari +18 more
TL;DR: In this article, the authors present the laboratory characterization and performance evaluation of the First Light Adaptive Optics (FLAO) the Natural Guide Star adaptive optics system for the Large Binocular Telescope (LBT), which uses an adaptive secondary mirror with 672 actuators and a pyramid wavefront sensor with adjustable sampled pupil from 30×30 down to 4×4 subapertures.