High contrast imaging at the LBT: The LEECH exoplanet imaging survey

Andrew J. Skemer; Philip Hinz; Simone Esposito; Michael F. Skrutskie; Denis Defrère; Vanessa Bailey; Jarron Leisenring; Daniel Apai; Beth Biller; Mickaël Bonnefoy; Wolfgang Brandner; Esther Buenzli; Laird Close; Justin Crepp; Robert J. De Rosa; Silvano Desidera; Josh Eisner; Jonathan Fortney; Thomas Henning; Karl Heinz Hofmann; Taisiya Kopytova; Anne Lise Maire; Jared R. Males; Rafael Millan-Gabet; Katie Morzinski; Apurva Oza; Jenny Patience; Abhijith Rajan; George Rieke; Dieter Schertl; Joshua Schlieder; Kate Su; Amali Vaz; Kimberly Ward-Duong; Gerd Weigelt; Charles E. Woodward; Neil Zimmerman

doi:10.1117/12.2057277

High contrast imaging at the LBT: The LEECH exoplanet imaging survey

Andrew J. Skemer, Philip Hinz, Simone Esposito, Michael F. Skrutskie, Denis Defrère, Vanessa Bailey, Jarron Leisenring, Daniel Apai, Beth Biller, Mickaël Bonnefoy, Wolfgang Brandner, Esther Buenzli, Laird Close, Justin Crepp, Robert J. De Rosa, Silvano Desidera, Josh Eisner, Jonathan Fortney, Thomas Henning, Karl Heinz HofmannTaisiya Kopytova, Anne Lise Maire, Jared R. Males, Rafael Millan-Gabet, Katie Morzinski, Apurva Oza, Jenny Patience, Abhijith Rajan, George Rieke, Dieter Schertl, Joshua Schlieder, Kate Su, Amali Vaz, Kimberly Ward-Duong, Gerd Weigelt, Charles E. Woodward, Neil Zimmerman

Minnesota Institute for Astrophysics

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

27 Scopus citations

Abstract

In Spring 2013, the LEECH (LBTI Exozodi Exoplanet Common Hunt) survey began its ∼130-night campaign from the Large Binocular Telescope (LBT) atop Mt Graham, Arizona. This survey benefits from the many technological achievements of the LBT, including two 8.4-meter mirrors on a single fixed mount, dual adaptive secondary mirrors for high Strehl performance, and a cold beam combiner to dramatically reduce the telescope's overall background emissivity. LEECH neatly complements other high-contrast planet imaging efforts by observing stars at L' (3.8 μm), as opposed to the shorter wavelength near-infrared bands (1-2.4 μm) of other surveys. This portion of the spectrum offers deep mass sensitivity, especially around nearby adolescent (∼0.1-1 Gyr) stars. LEECH's contrast is competitive with other extreme adaptive optics systems, while providing an alternative survey strategy. Additionally, LEECH is characterizing known exoplanetary systems with observations from 3-5μm in preparation for JWST.

Original language	English (US)
Title of host publication	Adaptive Optics Systems IV
Editors	Jean-Pierre Veran, Enrico Marchetti, Laird M. Close
Publisher	SPIE
ISBN (Electronic)	9780819496164
DOIs	https://doi.org/10.1117/12.2057277
State	Published - 2014
Event	Adaptive Optics Systems IV - Montreal, Canada Duration: Jun 22 2014 → Jun 27 2014

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9148
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Adaptive Optics Systems IV
Country/Territory	Canada
City	Montreal
Period	6/22/14 → 6/27/14

Bibliographical note

Publisher Copyright:
© 2014 SPIE.

Keywords

adaptive optics

Publisher link

10.1117/12.2057277

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Skemer, A. J., Hinz, P., Esposito, S., Skrutskie, M. F., Defrère, D., Bailey, V., Leisenring, J., Apai, D., Biller, B., Bonnefoy, M., Brandner, W., Buenzli, E., Close, L., Crepp, J., De Rosa, R. J., Desidera, S., Eisner, J., Fortney, J., Henning, T., ... Zimmerman, N. (2014). High contrast imaging at the LBT: The LEECH exoplanet imaging survey. In J-P. Veran, E. Marchetti, & L. M. Close (Eds.), Adaptive Optics Systems IV [91480L] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9148). SPIE. https://doi.org/10.1117/12.2057277

High contrast imaging at the LBT: The LEECH exoplanet imaging survey. / Skemer, Andrew J.; Hinz, Philip; Esposito, Simone et al.
Adaptive Optics Systems IV. ed. / Jean-Pierre Veran; Enrico Marchetti; Laird M. Close. SPIE, 2014. 91480L (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9148).

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

Skemer, AJ, Hinz, P, Esposito, S, Skrutskie, MF, Defrère, D, Bailey, V, Leisenring, J, Apai, D, Biller, B, Bonnefoy, M, Brandner, W, Buenzli, E, Close, L, Crepp, J, De Rosa, RJ, Desidera, S, Eisner, J, Fortney, J, Henning, T, Hofmann, KH, Kopytova, T, Maire, AL, Males, JR, Millan-Gabet, R, Morzinski, K, Oza, A, Patience, J, Rajan, A, Rieke, G, Schertl, D, Schlieder, J, Su, K, Vaz, A, Ward-Duong, K, Weigelt, G, Woodward, CE & Zimmerman, N 2014, High contrast imaging at the LBT: The LEECH exoplanet imaging survey. in J-P Veran, E Marchetti & LM Close (eds), Adaptive Optics Systems IV., 91480L, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9148, SPIE, Adaptive Optics Systems IV, Montreal, Canada, 6/22/14. https://doi.org/10.1117/12.2057277

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title = "High contrast imaging at the LBT: The LEECH exoplanet imaging survey",

abstract = "In Spring 2013, the LEECH (LBTI Exozodi Exoplanet Common Hunt) survey began its ∼130-night campaign from the Large Binocular Telescope (LBT) atop Mt Graham, Arizona. This survey benefits from the many technological achievements of the LBT, including two 8.4-meter mirrors on a single fixed mount, dual adaptive secondary mirrors for high Strehl performance, and a cold beam combiner to dramatically reduce the telescope's overall background emissivity. LEECH neatly complements other high-contrast planet imaging efforts by observing stars at L' (3.8 μm), as opposed to the shorter wavelength near-infrared bands (1-2.4 μm) of other surveys. This portion of the spectrum offers deep mass sensitivity, especially around nearby adolescent (∼0.1-1 Gyr) stars. LEECH's contrast is competitive with other extreme adaptive optics systems, while providing an alternative survey strategy. Additionally, LEECH is characterizing known exoplanetary systems with observations from 3-5μm in preparation for JWST.",

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author = "Skemer, {Andrew J.} and Philip Hinz and Simone Esposito and Skrutskie, {Michael F.} and Denis Defr{\`e}re and Vanessa Bailey and Jarron Leisenring and Daniel Apai and Beth Biller and Micka{\"e}l Bonnefoy and Wolfgang Brandner and Esther Buenzli and Laird Close and Justin Crepp and {De Rosa}, {Robert J.} and Silvano Desidera and Josh Eisner and Jonathan Fortney and Thomas Henning and Hofmann, {Karl Heinz} and Taisiya Kopytova and Maire, {Anne Lise} and Males, {Jared R.} and Rafael Millan-Gabet and Katie Morzinski and Apurva Oza and Jenny Patience and Abhijith Rajan and George Rieke and Dieter Schertl and Joshua Schlieder and Kate Su and Amali Vaz and Kimberly Ward-Duong and Gerd Weigelt and Woodward, {Charles E.} and Neil Zimmerman",

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AU - Skrutskie, Michael F.

AU - Defrère, Denis

AU - Bailey, Vanessa

AU - Leisenring, Jarron

AU - Apai, Daniel

AU - Biller, Beth

AU - Bonnefoy, Mickaël

AU - Brandner, Wolfgang

AU - Buenzli, Esther

AU - Close, Laird

AU - Crepp, Justin

AU - De Rosa, Robert J.

AU - Desidera, Silvano

AU - Eisner, Josh

AU - Fortney, Jonathan

AU - Henning, Thomas

AU - Hofmann, Karl Heinz

AU - Kopytova, Taisiya

AU - Maire, Anne Lise

AU - Males, Jared R.

AU - Millan-Gabet, Rafael

AU - Morzinski, Katie

AU - Oza, Apurva

AU - Patience, Jenny

AU - Rajan, Abhijith

AU - Rieke, George

AU - Schertl, Dieter

AU - Schlieder, Joshua

AU - Su, Kate

AU - Vaz, Amali

AU - Ward-Duong, Kimberly

AU - Weigelt, Gerd

AU - Woodward, Charles E.

AU - Zimmerman, Neil

PY - 2014

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N2 - In Spring 2013, the LEECH (LBTI Exozodi Exoplanet Common Hunt) survey began its ∼130-night campaign from the Large Binocular Telescope (LBT) atop Mt Graham, Arizona. This survey benefits from the many technological achievements of the LBT, including two 8.4-meter mirrors on a single fixed mount, dual adaptive secondary mirrors for high Strehl performance, and a cold beam combiner to dramatically reduce the telescope's overall background emissivity. LEECH neatly complements other high-contrast planet imaging efforts by observing stars at L' (3.8 μm), as opposed to the shorter wavelength near-infrared bands (1-2.4 μm) of other surveys. This portion of the spectrum offers deep mass sensitivity, especially around nearby adolescent (∼0.1-1 Gyr) stars. LEECH's contrast is competitive with other extreme adaptive optics systems, while providing an alternative survey strategy. Additionally, LEECH is characterizing known exoplanetary systems with observations from 3-5μm in preparation for JWST.

AB - In Spring 2013, the LEECH (LBTI Exozodi Exoplanet Common Hunt) survey began its ∼130-night campaign from the Large Binocular Telescope (LBT) atop Mt Graham, Arizona. This survey benefits from the many technological achievements of the LBT, including two 8.4-meter mirrors on a single fixed mount, dual adaptive secondary mirrors for high Strehl performance, and a cold beam combiner to dramatically reduce the telescope's overall background emissivity. LEECH neatly complements other high-contrast planet imaging efforts by observing stars at L' (3.8 μm), as opposed to the shorter wavelength near-infrared bands (1-2.4 μm) of other surveys. This portion of the spectrum offers deep mass sensitivity, especially around nearby adolescent (∼0.1-1 Gyr) stars. LEECH's contrast is competitive with other extreme adaptive optics systems, while providing an alternative survey strategy. Additionally, LEECH is characterizing known exoplanetary systems with observations from 3-5μm in preparation for JWST.

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BT - Adaptive Optics Systems IV

A2 - Veran, Jean-Pierre

A2 - Marchetti, Enrico

A2 - Close, Laird M.

PB - SPIE

Y2 - 22 June 2014 through 27 June 2014

ER -

High contrast imaging at the LBT: The LEECH exoplanet imaging survey

Abstract

Publication series

Other

Bibliographical note

Keywords

Publisher link

Find It

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