Closed-loop atmospheric dispersion compensation

On-sky demonstration of sub-milliarcsecond residual dispersion across H-band

P. Pathak, Olivier Guyon, N. Jovanovic, J. Lozi, F. Martinache, Y. Minowa, T. Kudo, T. Kotani, H. Takami

Research output: Contribution to conferencePaper

Abstract

On ground-based telescopes employing adaptive optics (AO) systems, atmospheric dispersion compensation is essential to deliver high quality imaging, and critical for coronagraphy and precision astrometry. In AO systems delivering high-Strehl, residual dispersion if often a dominant source of error, and is especially challenging to correct on large aperture telescopes. Imperfect compensation by atmospheric dispersion compensator (ADC) can be due to errors in the atmospheric dispersion estimation (usually derived from local temperature and pressure measurements), or calibration errors in the instrument and ADC optics. These limitations can be addressed with a high-precision on-sky measurement of residual dispersion in a closed-loop control scheme. In this work, we present a focal plane based technique, which utilizes the chromatic scaling of speckles to measure residual dispersion (atmospheric and optical) in the final science image. By using an adaptive speckle grid generated using a deformable mirror (DM) with a sufficiently large number of actuators, the residual dispersion is accurately measured and subsequently corrected in a closed-loop control. We demonstrate on-sky residual dispersion of 0.75 mas across H-band, reduced from 8.4 mas before closing the loop. This work will be useful for upcoming extremely large telescopes (ELTs) to achieve sub-milliarcsecond precision on astrometry and residual dispersion.

Original languageEnglish (US)
StatePublished - Jan 1 2017
Event5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017 - Tenerife, Canary Islands, Spain
Duration: Jun 25 2017Jun 30 2017

Other

Other5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017
CountrySpain
CityTenerife, Canary Islands
Period6/25/176/30/17

Fingerprint

Dispersion compensation
sky
Demonstrations
Telescopes
Adaptive optics
astrometry
Speckle
speckle
compensators
telescopes
adaptive optics
Antenna grounds
Pressure measurement
deformable mirrors
Temperature measurement
closing
pressure measurement
Optics
Mirrors
temperature measurement

Keywords

  • Adaptive Optics
  • ADC
  • Atmospheric dispersion
  • Exoplanets

ASJC Scopus subject areas

  • Space and Planetary Science
  • Mechanical Engineering
  • Control and Systems Engineering
  • Instrumentation
  • Astronomy and Astrophysics
  • Electronic, Optical and Magnetic Materials

Cite this

Pathak, P., Guyon, O., Jovanovic, N., Lozi, J., Martinache, F., Minowa, Y., ... Takami, H. (2017). Closed-loop atmospheric dispersion compensation: On-sky demonstration of sub-milliarcsecond residual dispersion across H-band. Paper presented at 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017, Tenerife, Canary Islands, Spain.

Closed-loop atmospheric dispersion compensation : On-sky demonstration of sub-milliarcsecond residual dispersion across H-band. / Pathak, P.; Guyon, Olivier; Jovanovic, N.; Lozi, J.; Martinache, F.; Minowa, Y.; Kudo, T.; Kotani, T.; Takami, H.

2017. Paper presented at 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017, Tenerife, Canary Islands, Spain.

Research output: Contribution to conferencePaper

Pathak, P, Guyon, O, Jovanovic, N, Lozi, J, Martinache, F, Minowa, Y, Kudo, T, Kotani, T & Takami, H 2017, 'Closed-loop atmospheric dispersion compensation: On-sky demonstration of sub-milliarcsecond residual dispersion across H-band' Paper presented at 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017, Tenerife, Canary Islands, Spain, 6/25/17 - 6/30/17, .
Pathak P, Guyon O, Jovanovic N, Lozi J, Martinache F, Minowa Y et al. Closed-loop atmospheric dispersion compensation: On-sky demonstration of sub-milliarcsecond residual dispersion across H-band. 2017. Paper presented at 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017, Tenerife, Canary Islands, Spain.
Pathak, P. ; Guyon, Olivier ; Jovanovic, N. ; Lozi, J. ; Martinache, F. ; Minowa, Y. ; Kudo, T. ; Kotani, T. ; Takami, H. / Closed-loop atmospheric dispersion compensation : On-sky demonstration of sub-milliarcsecond residual dispersion across H-band. Paper presented at 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017, Tenerife, Canary Islands, Spain.
@conference{1a5015c3e2d84930aa2921f4db3e5916,
title = "Closed-loop atmospheric dispersion compensation: On-sky demonstration of sub-milliarcsecond residual dispersion across H-band",
abstract = "On ground-based telescopes employing adaptive optics (AO) systems, atmospheric dispersion compensation is essential to deliver high quality imaging, and critical for coronagraphy and precision astrometry. In AO systems delivering high-Strehl, residual dispersion if often a dominant source of error, and is especially challenging to correct on large aperture telescopes. Imperfect compensation by atmospheric dispersion compensator (ADC) can be due to errors in the atmospheric dispersion estimation (usually derived from local temperature and pressure measurements), or calibration errors in the instrument and ADC optics. These limitations can be addressed with a high-precision on-sky measurement of residual dispersion in a closed-loop control scheme. In this work, we present a focal plane based technique, which utilizes the chromatic scaling of speckles to measure residual dispersion (atmospheric and optical) in the final science image. By using an adaptive speckle grid generated using a deformable mirror (DM) with a sufficiently large number of actuators, the residual dispersion is accurately measured and subsequently corrected in a closed-loop control. We demonstrate on-sky residual dispersion of 0.75 mas across H-band, reduced from 8.4 mas before closing the loop. This work will be useful for upcoming extremely large telescopes (ELTs) to achieve sub-milliarcsecond precision on astrometry and residual dispersion.",
keywords = "Adaptive Optics, ADC, Atmospheric dispersion, Exoplanets",
author = "P. Pathak and Olivier Guyon and N. Jovanovic and J. Lozi and F. Martinache and Y. Minowa and T. Kudo and T. Kotani and H. Takami",
year = "2017",
month = "1",
day = "1",
language = "English (US)",
note = "5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017 ; Conference date: 25-06-2017 Through 30-06-2017",

}

TY - CONF

T1 - Closed-loop atmospheric dispersion compensation

T2 - On-sky demonstration of sub-milliarcsecond residual dispersion across H-band

AU - Pathak, P.

AU - Guyon, Olivier

AU - Jovanovic, N.

AU - Lozi, J.

AU - Martinache, F.

AU - Minowa, Y.

AU - Kudo, T.

AU - Kotani, T.

AU - Takami, H.

PY - 2017/1/1

Y1 - 2017/1/1

N2 - On ground-based telescopes employing adaptive optics (AO) systems, atmospheric dispersion compensation is essential to deliver high quality imaging, and critical for coronagraphy and precision astrometry. In AO systems delivering high-Strehl, residual dispersion if often a dominant source of error, and is especially challenging to correct on large aperture telescopes. Imperfect compensation by atmospheric dispersion compensator (ADC) can be due to errors in the atmospheric dispersion estimation (usually derived from local temperature and pressure measurements), or calibration errors in the instrument and ADC optics. These limitations can be addressed with a high-precision on-sky measurement of residual dispersion in a closed-loop control scheme. In this work, we present a focal plane based technique, which utilizes the chromatic scaling of speckles to measure residual dispersion (atmospheric and optical) in the final science image. By using an adaptive speckle grid generated using a deformable mirror (DM) with a sufficiently large number of actuators, the residual dispersion is accurately measured and subsequently corrected in a closed-loop control. We demonstrate on-sky residual dispersion of 0.75 mas across H-band, reduced from 8.4 mas before closing the loop. This work will be useful for upcoming extremely large telescopes (ELTs) to achieve sub-milliarcsecond precision on astrometry and residual dispersion.

AB - On ground-based telescopes employing adaptive optics (AO) systems, atmospheric dispersion compensation is essential to deliver high quality imaging, and critical for coronagraphy and precision astrometry. In AO systems delivering high-Strehl, residual dispersion if often a dominant source of error, and is especially challenging to correct on large aperture telescopes. Imperfect compensation by atmospheric dispersion compensator (ADC) can be due to errors in the atmospheric dispersion estimation (usually derived from local temperature and pressure measurements), or calibration errors in the instrument and ADC optics. These limitations can be addressed with a high-precision on-sky measurement of residual dispersion in a closed-loop control scheme. In this work, we present a focal plane based technique, which utilizes the chromatic scaling of speckles to measure residual dispersion (atmospheric and optical) in the final science image. By using an adaptive speckle grid generated using a deformable mirror (DM) with a sufficiently large number of actuators, the residual dispersion is accurately measured and subsequently corrected in a closed-loop control. We demonstrate on-sky residual dispersion of 0.75 mas across H-band, reduced from 8.4 mas before closing the loop. This work will be useful for upcoming extremely large telescopes (ELTs) to achieve sub-milliarcsecond precision on astrometry and residual dispersion.

KW - Adaptive Optics

KW - ADC

KW - Atmospheric dispersion

KW - Exoplanets

UR - http://www.scopus.com/inward/record.url?scp=85049251295&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85049251295&partnerID=8YFLogxK

M3 - Paper

ER -