Visible AO observations at halpha for accreting young planets

L. M. Close; K. Follette; J. R. Males; K. Morzinski; T. J. Rodigas; P. Hinz; Y. L. Wu; D. Apai; J. Najita; A. Puglisi; S. Esposito; A. Riccardi; V. Bailey; M. Xompero; R. Briguglio; A. Weinberger

doi:10.1017/S1743921313007734

Visible AO observations at halpha for accreting young planets

L. M. Close, K. Follette, J. R. Males, K. Morzinski, T. J. Rodigas, P. Hinz, Y. L. Wu, D. Apai, J. Najita, A. Puglisi, S. Esposito, A. Riccardi, V. Bailey, M. Xompero, R. Briguglio, A. Weinberger

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

Abstract

We utilized the new high-order (250-378 mode) Magellan Adaptive Optics system (MagAO) to obtain very high-resolution science in the visible with MagAO's VisAO CCD camera. In the good-median seeing conditions of Magellan (0.5-0.7″) we find MagAO delivers individual short exposure images as good as 19 mas optical resolution. Due to telescope vibrations, long exposure (60s) r' (0.63μm) images are slightly coarser at FWHM = 23-29 mas (Strehl ~ 28%) with bright (R < 9 mag) guide stars. These are the highest resolution filled-aperture images published to date. Images of the young (~ 1 Myr) Orion Trapezium θ¹ Ori A, B, and C cluster members were obtained with VisAO. In particular, the 32 mas binary θ¹ Ori C 1 C 2 was easily resolved in non-interferometric images for the first time. Relative positions of the bright trapezium binary stars were measured with ~ 0.6-5 mas accuracy. In the second commissioning run we were able to correct 378 modes and achieved good contrasts (Strehl>20% on young transition disks at Hα). We discuss the contrasts achieved at Hα and the possibility of detecting low mass (~ 1-5 Mjup) planets (past 5AU) with our new SAPPHIRES survey with MagAO at Hα.

Original language	English
Title of host publication	Exploring the Formation and Evolution of Planetary Systems
Publisher	Cambridge University Press
Pages	32-33
Number of pages	2
Edition	S299
ISBN (Print)	9781107045200
DOIs	https://doi.org/10.1017/S1743921313007734
Publication status	Published - 2013 Jun
Externally published	Yes

Publication series

Name	Proceedings of the International Astronomical Union
Number	S299
Volume	8
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

Keywords

Adaptive Optics
Extra-solar Planets

ASJC Scopus subject areas

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

Access to Document

10.1017/S1743921313007734

Cite this

Close, L. M., Follette, K., Males, J. R., Morzinski, K., Rodigas, T. J., Hinz, P., Wu, Y. L., Apai, D., Najita, J., Puglisi, A., Esposito, S., Riccardi, A., Bailey, V., Xompero, M., Briguglio, R., & Weinberger, A. (2013). Visible AO observations at halpha for accreting young planets. In Exploring the Formation and Evolution of Planetary Systems (S299 ed., pp. 32-33). (Proceedings of the International Astronomical Union; Vol. 8, No. S299). Cambridge University Press. https://doi.org/10.1017/S1743921313007734

Visible AO observations at halpha for accreting young planets. / Close, L. M.; Follette, K.; Males, J. R. et al.
Exploring the Formation and Evolution of Planetary Systems. S299. ed. Cambridge University Press, 2013. p. 32-33 (Proceedings of the International Astronomical Union; Vol. 8, No. S299).

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

Close, LM, Follette, K, Males, JR, Morzinski, K, Rodigas, TJ, Hinz, P, Wu, YL, Apai, D, Najita, J, Puglisi, A, Esposito, S, Riccardi, A, Bailey, V, Xompero, M, Briguglio, R & Weinberger, A 2013, Visible AO observations at halpha for accreting young planets. in Exploring the Formation and Evolution of Planetary Systems. S299 edn, Proceedings of the International Astronomical Union, no. S299, vol. 8, Cambridge University Press, pp. 32-33. https://doi.org/10.1017/S1743921313007734

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title = "Visible AO observations at halpha for accreting young planets",

abstract = "We utilized the new high-order (250-378 mode) Magellan Adaptive Optics system (MagAO) to obtain very high-resolution science in the visible with MagAO's VisAO CCD camera. In the good-median seeing conditions of Magellan (0.5-0.7″) we find MagAO delivers individual short exposure images as good as 19 mas optical resolution. Due to telescope vibrations, long exposure (60s) r' (0.63μm) images are slightly coarser at FWHM = 23-29 mas (Strehl ~ 28%) with bright (R < 9 mag) guide stars. These are the highest resolution filled-aperture images published to date. Images of the young (~ 1 Myr) Orion Trapezium θ1 Ori A, B, and C cluster members were obtained with VisAO. In particular, the 32 mas binary θ1 Ori C 1 C 2 was easily resolved in non-interferometric images for the first time. Relative positions of the bright trapezium binary stars were measured with ~ 0.6-5 mas accuracy. In the second commissioning run we were able to correct 378 modes and achieved good contrasts (Strehl>20% on young transition disks at Hα). We discuss the contrasts achieved at Hα and the possibility of detecting low mass (~ 1-5 Mjup) planets (past 5AU) with our new SAPPHIRES survey with MagAO at Hα.",

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author = "Close, {L. M.} and K. Follette and Males, {J. R.} and K. Morzinski and Rodigas, {T. J.} and P. Hinz and Wu, {Y. L.} and D. Apai and J. Najita and A. Puglisi and S. Esposito and A. Riccardi and V. Bailey and M. Xompero and R. Briguglio and A. Weinberger",

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doi = "10.1017/S1743921313007734",

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AU - Close, L. M.

AU - Follette, K.

AU - Males, J. R.

AU - Morzinski, K.

AU - Rodigas, T. J.

AU - Hinz, P.

AU - Wu, Y. L.

AU - Apai, D.

AU - Najita, J.

AU - Puglisi, A.

AU - Esposito, S.

AU - Riccardi, A.

AU - Bailey, V.

AU - Xompero, M.

AU - Briguglio, R.

AU - Weinberger, A.

PY - 2013/6

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N2 - We utilized the new high-order (250-378 mode) Magellan Adaptive Optics system (MagAO) to obtain very high-resolution science in the visible with MagAO's VisAO CCD camera. In the good-median seeing conditions of Magellan (0.5-0.7″) we find MagAO delivers individual short exposure images as good as 19 mas optical resolution. Due to telescope vibrations, long exposure (60s) r' (0.63μm) images are slightly coarser at FWHM = 23-29 mas (Strehl ~ 28%) with bright (R < 9 mag) guide stars. These are the highest resolution filled-aperture images published to date. Images of the young (~ 1 Myr) Orion Trapezium θ1 Ori A, B, and C cluster members were obtained with VisAO. In particular, the 32 mas binary θ1 Ori C 1 C 2 was easily resolved in non-interferometric images for the first time. Relative positions of the bright trapezium binary stars were measured with ~ 0.6-5 mas accuracy. In the second commissioning run we were able to correct 378 modes and achieved good contrasts (Strehl>20% on young transition disks at Hα). We discuss the contrasts achieved at Hα and the possibility of detecting low mass (~ 1-5 Mjup) planets (past 5AU) with our new SAPPHIRES survey with MagAO at Hα.

AB - We utilized the new high-order (250-378 mode) Magellan Adaptive Optics system (MagAO) to obtain very high-resolution science in the visible with MagAO's VisAO CCD camera. In the good-median seeing conditions of Magellan (0.5-0.7″) we find MagAO delivers individual short exposure images as good as 19 mas optical resolution. Due to telescope vibrations, long exposure (60s) r' (0.63μm) images are slightly coarser at FWHM = 23-29 mas (Strehl ~ 28%) with bright (R < 9 mag) guide stars. These are the highest resolution filled-aperture images published to date. Images of the young (~ 1 Myr) Orion Trapezium θ1 Ori A, B, and C cluster members were obtained with VisAO. In particular, the 32 mas binary θ1 Ori C 1 C 2 was easily resolved in non-interferometric images for the first time. Relative positions of the bright trapezium binary stars were measured with ~ 0.6-5 mas accuracy. In the second commissioning run we were able to correct 378 modes and achieved good contrasts (Strehl>20% on young transition disks at Hα). We discuss the contrasts achieved at Hα and the possibility of detecting low mass (~ 1-5 Mjup) planets (past 5AU) with our new SAPPHIRES survey with MagAO at Hα.

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BT - Exploring the Formation and Evolution of Planetary Systems

PB - Cambridge University Press

ER -

Visible AO observations at halpha for accreting young planets

Abstract

Publication series

Keywords

ASJC Scopus subject areas

UN SDGs

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