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Published on: February 12, 2014
On-sky multiwavelength phasing of segmented telescopes with the Zernike phase contrast sensor
Arthur Vigan1, Kjetil Dohlen, Silvio Mazzanti
1Laboratoire d’Astrophysique de Marseille, UMR 6110, CNRS, Université de Provence, 38 rue Frédéric Joliot-Curie, 13388 Marseille Cedex 13, France. arthur@astro.ex.ac.uk
A new multiwavelength scheme successfully phases extremely large telescope mirrors with large errors. This technique extends the capture range of phasing sensors, crucial for maintaining high wavefront quality in future observatories.
Area of Science:
- Optical astronomy
- Telescope engineering
- Adaptive optics
Background:
- Extremely large telescopes (ELTs) utilize segmented primary mirrors with hundreds of segments.
- Precise cophasing of these segments is critical for achieving high wavefront quality and optimal observational performance.
Purpose of the Study:
- To develop and demonstrate a multiwavelength scheme for enhancing the capture range of phasing sensors.
- To enable phasing of telescope segments with large initial dephasing errors (micrometers).
Main Methods:
- Implementation of a multiwavelength scheme for the Zernike phase contrast sensor.
- On-sky demonstration at the Very Large Telescope (VLT).
- Testing the sensor's ability to correct piston errors up to ±4.0 μm.
Main Results:
- The multiwavelength scheme successfully extended the phasing capture range from ±λ/2 to several micrometers.
- Demonstrated successful phasing of mirror segments with piston errors up to ±4.0 μm.
- Validated the effectiveness of the Zernike phase contrast sensor with the new scheme.
Conclusions:
- The developed multiwavelength scheme is effective for phasing large segmented mirrors in ELTs.
- This approach is essential for maintaining high phasing accuracy during observations.
- A robust phasing strategy for future ELTs has been established.
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