Abstract
Integral field spectrographs are an important technology for exoplanet imaging, due to their ability to take spectra in a high-contrast environment, and improve planet detection sensitivity through spectral differential imaging. ALES is the first integral field spectrograph capable of imaging exoplanets from 3-5 μm, and will extend our ability to characterize self-luminous exoplanets into a wavelength range where they peak in brightness. ALES is installed inside LBTI/LMIRcam on the Large Binocular Telescope, taking advantage of existing AO systems, camera optics, and a HAWAII-2RG detector. The new optics that comprise ALES are a Keplerian magnifier, a silicon lenslet array with diffraction suppressing pinholes, a direct vision prism, and calibration optics. All of these components are installed in filter wheels making ALES a completely modular design. ALES saw first light at the LBT in June 2015.
Original language | English (US) |
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Title of host publication | Techniques and Instrumentation for Detection of Exoplanets VII |
Editors | Stuart Shaklan |
Publisher | SPIE |
ISBN (Electronic) | 9781628417715 |
DOIs | |
State | Published - 2015 |
Event | Techniques and Instrumentation for Detection of Exoplanets VII - San Diego, United States Duration: Aug 10 2015 → Aug 13 2015 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
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Volume | 9605 |
ISSN (Print) | 0277-786X |
ISSN (Electronic) | 1996-756X |
Conference
Conference | Techniques and Instrumentation for Detection of Exoplanets VII |
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Country/Territory | United States |
City | San Diego |
Period | 8/10/15 → 8/13/15 |
Bibliographical note
Publisher Copyright:© 2015 SPIE.
Keywords
- Adaptive optics
- exoplanet imaging
- exoplanet instrumentation
- integral field spectroscopy