SHARK-NIR, toward the installation at the Large Binocular Telescope

Luca Marafatto; Maria Bergomi; Federico Biondi; Elena Carolo; Marco De Pascale; Davide Greggio; Luigi Lessio; Dino Mesa; Kalyan Kumar Radhakrishnan Santhakumari; Gabriele Umbriaco; Daniele Vassallo; Valentina Viotto; Andrea Bianco; Marco Dima; Valentina D'Orazi; Paul Grenz; Jarron M. Leisenring; Lars Mohr; Manny Montoya; Alessio Zanutta; Simone Antoniucci; Carmelo Arcidiacono; Francesca Bacciotti; Carlo Baffa; Andrea Baruffolo; Angela Bongiorno; Alexis Carlotti; Simonetta Chinellato; Laird Close; Simone Di Filippo; Simone Esposito; Giancarlo Farisato; Olivier Guyon; Philip Hinz; Demetrio Magrin; Fernando Pedichini; Enrico Pinna; Elisa Portaluri; Alfio Puglisi; Roberto Ragazzoni; Fabio Rossi; Jacopo Farinato

doi:10.1117/12.2562515

SHARK-NIR, toward the installation at the Large Binocular Telescope

Luca Marafatto, Maria Bergomi, Federico Biondi, Elena Carolo, Marco De Pascale, Davide Greggio, Luigi Lessio, Dino Mesa, Kalyan Kumar Radhakrishnan Santhakumari, Gabriele Umbriaco, Daniele Vassallo, Valentina Viotto, Andrea Bianco, Marco Dima, Valentina D'Orazi, Paul Grenz, Jarron M. Leisenring, Lars Mohr, Manny Montoya, Alessio ZanuttaSimone Antoniucci, Carmelo Arcidiacono, Francesca Bacciotti, Carlo Baffa, Andrea Baruffolo, Angela Bongiorno, Alexis Carlotti, Simonetta Chinellato, Laird Close, Simone Di Filippo, Simone Esposito, Giancarlo Farisato, Olivier Guyon, Philip Hinz, Demetrio Magrin, Fernando Pedichini, Enrico Pinna, Elisa Portaluri, Alfio Puglisi, Roberto Ragazzoni, Fabio Rossi, Jacopo Farinato

Steward Observatory

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

3 Scopus citations

Abstract

SHARK-NIR in an instrument that will provide direct imaging, coronagraphic imaging, dual band imaging and low resolution spectroscopy in Y, J and H bands, and it will be soon installed at the Large Binocular Telescope. Used in combination with SHARK-VIS (operating in V band) and LMIRCam of LBTI (operating from K to M bands), SHARKNIR will exploit coronagraphic simultaneous observations in three different wavelengths. Exoplanets search and characterization, young stellar systems, jets and disks are the main science cases, but the extreme performance of the LBT AO systems, above all in the faint end regime, will allow to open to science difficult to be achieved from other similar instruments, such as AGN and QSO morphological studies. A variety of coronagraphic techniques have been implemented, as the Gaussian Lyot, Shaped Pupil and Four Quadrant masks, with the aim to possibly have a suitable coronagraphic masks for each science case, since the coronagraphic requirement in term of contrast and inner and outer working angle are depending on the target and on the science to be achieved.

Original language	English (US)
Title of host publication	Adaptive Optics Systems VII
Editors	Laura Schreiber, Dirk Schmidt, Elise Vernet
Publisher	SPIE
ISBN (Electronic)	9781510636835
DOIs	https://doi.org/10.1117/12.2562515
State	Published - 2020
Event	Adaptive Optics Systems VII 2020 - Virtual, Online, United States Duration: Dec 14 2020 → Dec 22 2020

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11448
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Adaptive Optics Systems VII 2020
Country/Territory	United States
City	Virtual, Online
Period	12/14/20 → 12/22/20

Keywords

Adaptive secondary
Coronagraphy
Extreme adaptive optics
Large binocular telescope
Planet finding
Pyramid sensor

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2562515

Cite this

Marafatto, L., Bergomi, M., Biondi, F., Carolo, E., De Pascale, M., Greggio, D., Lessio, L., Mesa, D., Santhakumari, K. K. R., Umbriaco, G., Vassallo, D., Viotto, V., Bianco, A., Dima, M., D'Orazi, V., Grenz, P., Leisenring, J. M., Mohr, L., Montoya, M., ... Farinato, J. (2020). SHARK-NIR, toward the installation at the Large Binocular Telescope. In L. Schreiber, D. Schmidt, & E. Vernet (Eds.), Adaptive Optics Systems VII Article 114481M (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11448). SPIE. https://doi.org/10.1117/12.2562515

SHARK-NIR, toward the installation at the Large Binocular Telescope. / Marafatto, Luca; Bergomi, Maria; Biondi, Federico et al.
Adaptive Optics Systems VII. ed. / Laura Schreiber; Dirk Schmidt; Elise Vernet. SPIE, 2020. 114481M (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11448).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Marafatto, L, Bergomi, M, Biondi, F, Carolo, E, De Pascale, M, Greggio, D, Lessio, L, Mesa, D, Santhakumari, KKR, Umbriaco, G, Vassallo, D, Viotto, V, Bianco, A, Dima, M, D'Orazi, V, Grenz, P, Leisenring, JM, Mohr, L, Montoya, M, Zanutta, A, Antoniucci, S, Arcidiacono, C, Bacciotti, F, Baffa, C, Baruffolo, A, Bongiorno, A, Carlotti, A, Chinellato, S, Close, L, Di Filippo, S, Esposito, S, Farisato, G, Guyon, O, Hinz, P, Magrin, D, Pedichini, F, Pinna, E, Portaluri, E, Puglisi, A, Ragazzoni, R, Rossi, F & Farinato, J 2020, SHARK-NIR, toward the installation at the Large Binocular Telescope. in L Schreiber, D Schmidt & E Vernet (eds), Adaptive Optics Systems VII., 114481M, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11448, SPIE, Adaptive Optics Systems VII 2020, Virtual, Online, United States, 12/14/20. https://doi.org/10.1117/12.2562515

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title = "SHARK-NIR, toward the installation at the Large Binocular Telescope",

abstract = "SHARK-NIR in an instrument that will provide direct imaging, coronagraphic imaging, dual band imaging and low resolution spectroscopy in Y, J and H bands, and it will be soon installed at the Large Binocular Telescope. Used in combination with SHARK-VIS (operating in V band) and LMIRCam of LBTI (operating from K to M bands), SHARKNIR will exploit coronagraphic simultaneous observations in three different wavelengths. Exoplanets search and characterization, young stellar systems, jets and disks are the main science cases, but the extreme performance of the LBT AO systems, above all in the faint end regime, will allow to open to science difficult to be achieved from other similar instruments, such as AGN and QSO morphological studies. A variety of coronagraphic techniques have been implemented, as the Gaussian Lyot, Shaped Pupil and Four Quadrant masks, with the aim to possibly have a suitable coronagraphic masks for each science case, since the coronagraphic requirement in term of contrast and inner and outer working angle are depending on the target and on the science to be achieved.",

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author = "Luca Marafatto and Maria Bergomi and Federico Biondi and Elena Carolo and {De Pascale}, Marco and Davide Greggio and Luigi Lessio and Dino Mesa and Santhakumari, {Kalyan Kumar Radhakrishnan} and Gabriele Umbriaco and Daniele Vassallo and Valentina Viotto and Andrea Bianco and Marco Dima and Valentina D'Orazi and Paul Grenz and Leisenring, {Jarron M.} and Lars Mohr and Manny Montoya and Alessio Zanutta and Simone Antoniucci and Carmelo Arcidiacono and Francesca Bacciotti and Carlo Baffa and Andrea Baruffolo and Angela Bongiorno and Alexis Carlotti and Simonetta Chinellato and Laird Close and {Di Filippo}, Simone and Simone Esposito and Giancarlo Farisato and Olivier Guyon and Philip Hinz and Demetrio Magrin and Fernando Pedichini and Enrico Pinna and Elisa Portaluri and Alfio Puglisi and Roberto Ragazzoni and Fabio Rossi and Jacopo Farinato",

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AU - Bergomi, Maria

AU - Biondi, Federico

AU - Carolo, Elena

AU - De Pascale, Marco

AU - Greggio, Davide

AU - Lessio, Luigi

AU - Mesa, Dino

AU - Santhakumari, Kalyan Kumar Radhakrishnan

AU - Umbriaco, Gabriele

AU - Vassallo, Daniele

AU - Viotto, Valentina

AU - Bianco, Andrea

AU - Dima, Marco

AU - D'Orazi, Valentina

AU - Grenz, Paul

AU - Leisenring, Jarron M.

AU - Mohr, Lars

AU - Montoya, Manny

AU - Zanutta, Alessio

AU - Antoniucci, Simone

AU - Arcidiacono, Carmelo

AU - Bacciotti, Francesca

AU - Baffa, Carlo

AU - Baruffolo, Andrea

AU - Bongiorno, Angela

AU - Carlotti, Alexis

AU - Chinellato, Simonetta

AU - Close, Laird

AU - Di Filippo, Simone

AU - Esposito, Simone

AU - Farisato, Giancarlo

AU - Guyon, Olivier

AU - Hinz, Philip

AU - Magrin, Demetrio

AU - Pedichini, Fernando

AU - Pinna, Enrico

AU - Portaluri, Elisa

AU - Puglisi, Alfio

AU - Ragazzoni, Roberto

AU - Rossi, Fabio

AU - Farinato, Jacopo

PY - 2020

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N2 - SHARK-NIR in an instrument that will provide direct imaging, coronagraphic imaging, dual band imaging and low resolution spectroscopy in Y, J and H bands, and it will be soon installed at the Large Binocular Telescope. Used in combination with SHARK-VIS (operating in V band) and LMIRCam of LBTI (operating from K to M bands), SHARKNIR will exploit coronagraphic simultaneous observations in three different wavelengths. Exoplanets search and characterization, young stellar systems, jets and disks are the main science cases, but the extreme performance of the LBT AO systems, above all in the faint end regime, will allow to open to science difficult to be achieved from other similar instruments, such as AGN and QSO morphological studies. A variety of coronagraphic techniques have been implemented, as the Gaussian Lyot, Shaped Pupil and Four Quadrant masks, with the aim to possibly have a suitable coronagraphic masks for each science case, since the coronagraphic requirement in term of contrast and inner and outer working angle are depending on the target and on the science to be achieved.

AB - SHARK-NIR in an instrument that will provide direct imaging, coronagraphic imaging, dual band imaging and low resolution spectroscopy in Y, J and H bands, and it will be soon installed at the Large Binocular Telescope. Used in combination with SHARK-VIS (operating in V band) and LMIRCam of LBTI (operating from K to M bands), SHARKNIR will exploit coronagraphic simultaneous observations in three different wavelengths. Exoplanets search and characterization, young stellar systems, jets and disks are the main science cases, but the extreme performance of the LBT AO systems, above all in the faint end regime, will allow to open to science difficult to be achieved from other similar instruments, such as AGN and QSO morphological studies. A variety of coronagraphic techniques have been implemented, as the Gaussian Lyot, Shaped Pupil and Four Quadrant masks, with the aim to possibly have a suitable coronagraphic masks for each science case, since the coronagraphic requirement in term of contrast and inner and outer working angle are depending on the target and on the science to be achieved.

KW - Adaptive secondary

KW - Coronagraphy

KW - Extreme adaptive optics

KW - Large binocular telescope

KW - Planet finding

KW - Pyramid sensor

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ER -

SHARK-NIR, toward the installation at the Large Binocular Telescope

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

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