Some recent results from the CHARA Array

T. A. ten Brummelaar; David Huber; K. von Braun; T. Boyajian; N. D. Richardson; G. Schaefer; I. Tallon-Bosc; D. Mourard; H. A. McAlister; N. H. Turner; L. Sturmann; J. Sturmann; J. D. Monnier; M. Ireland

Some recent results from the CHARA Array

T. A. ten Brummelaar^*, David Huber, K. von Braun, T. Boyajian, N. D. Richardson, G. Schaefer, I. Tallon-Bosc, D. Mourard, H. A. McAlister, N. H. Turner, L. Sturmann, J. Sturmann, J. D. Monnier, M. Ireland

^*Corresponding author for this work

Department of Physics and Astronomy

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

Abstract

The CHARA Array is a six 1-m telescope optical and near infrared interferometer located at the Mount Wilson Observatory in southern California and operated by the Center for High Angular Resolution Astronomy of Georgia State University. The CHARA Array has been in regular scientific operation since 2005 and now has over 55 publications in the refereed literature, including two in Science and one in Nature. The Array now supports seven beam combiners ranging from 0.5 microns up to 2.3 microns and combing from 2 to 4 beams at a time. An upgrade to a full 6-beam combiner is now underway, and fringes with all six telescopes were achieved soon after the meeting. We present some of the more recent results from the CHARA Array.

Original language	English
Title of host publication	Resolving the future of astronomy with long-baseline interferometry
Subtitle of host publication	proceedings of a conference held at New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA 28-31 March 2011
Editors	Michelle J. Creech-Eakman, Joyce A. Guzik, Robert E. Stencel
Place of Publication	San Francisco, CA
Publisher	Astronomical Society of the Pacific
Pages	389-393
Number of pages	5
ISBN (Electronic)	9781583818596
ISBN (Print)	9781583818589
Publication status	Published - 2014
Event	Conference on Resolving the Future of Astronomy with Long-Baseline Interferometry - Socorro Duration: 28 Mar 2011 → 31 Mar 2011

Publication series

Name	Astronomical Society of the Pacific conference series
Publisher	Astronomical Society of the Pacific
Volume	487

Conference

Conference	Conference on Resolving the Future of Astronomy with Long-Baseline Interferometry
City	Socorro
Period	28/03/11 → 31/03/11

Access to Document

http://aspbooks.org/custom/publications/paper/487-0389.html

Cite this

ten Brummelaar, T. A., Huber, D., von Braun, K., Boyajian, T., Richardson, N. D., Schaefer, G., Tallon-Bosc, I., Mourard, D., McAlister, H. A., Turner, N. H., Sturmann, L., Sturmann, J., Monnier, J. D., & Ireland, M. (2014). Some recent results from the CHARA Array. In M. J. Creech-Eakman, J. A. Guzik, & R. E. Stencel (Eds.), Resolving the future of astronomy with long-baseline interferometry: proceedings of a conference held at New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA 28-31 March 2011 (pp. 389-393). (Astronomical Society of the Pacific conference series; Vol. 487). Astronomical Society of the Pacific. http://aspbooks.org/custom/publications/paper/487-0389.html

ten Brummelaar, T. A. ; Huber, David ; von Braun, K. ; Boyajian, T. ; Richardson, N. D. ; Schaefer, G. ; Tallon-Bosc, I. ; Mourard, D. ; McAlister, H. A. ; Turner, N. H. ; Sturmann, L. ; Sturmann, J. ; Monnier, J. D. ; Ireland, M. / Some recent results from the CHARA Array. Resolving the future of astronomy with long-baseline interferometry: proceedings of a conference held at New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA 28-31 March 2011. editor / Michelle J. Creech-Eakman ; Joyce A. Guzik ; Robert E. Stencel. San Francisco, CA : Astronomical Society of the Pacific, 2014. pp. 389-393 (Astronomical Society of the Pacific conference series).

@inproceedings{39123a4a57e34aadb988406c6ca10c05,

title = "Some recent results from the CHARA Array",

abstract = "The CHARA Array is a six 1-m telescope optical and near infrared interferometer located at the Mount Wilson Observatory in southern California and operated by the Center for High Angular Resolution Astronomy of Georgia State University. The CHARA Array has been in regular scientific operation since 2005 and now has over 55 publications in the refereed literature, including two in Science and one in Nature. The Array now supports seven beam combiners ranging from 0.5 microns up to 2.3 microns and combing from 2 to 4 beams at a time. An upgrade to a full 6-beam combiner is now underway, and fringes with all six telescopes were achieved soon after the meeting. We present some of the more recent results from the CHARA Array.",

author = "{ten Brummelaar}, {T. A.} and David Huber and {von Braun}, K. and T. Boyajian and Richardson, {N. D.} and G. Schaefer and I. Tallon-Bosc and D. Mourard and McAlister, {H. A.} and Turner, {N. H.} and L. Sturmann and J. Sturmann and Monnier, {J. D.} and M. Ireland",

year = "2014",

language = "English",

isbn = "9781583818589",

series = "Astronomical Society of the Pacific conference series",

publisher = "Astronomical Society of the Pacific",

pages = "389--393",

editor = "Creech-Eakman, {Michelle J.} and Guzik, {Joyce A.} and Stencel, {Robert E.}",

booktitle = "Resolving the future of astronomy with long-baseline interferometry",

note = "Conference on Resolving the Future of Astronomy with Long-Baseline Interferometry ; Conference date: 28-03-2011 Through 31-03-2011",

}

ten Brummelaar, TA, Huber, D, von Braun, K, Boyajian, T, Richardson, ND, Schaefer, G, Tallon-Bosc, I, Mourard, D, McAlister, HA, Turner, NH, Sturmann, L, Sturmann, J, Monnier, JD & Ireland, M 2014, Some recent results from the CHARA Array. in MJ Creech-Eakman, JA Guzik & RE Stencel (eds), Resolving the future of astronomy with long-baseline interferometry: proceedings of a conference held at New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA 28-31 March 2011. Astronomical Society of the Pacific conference series, vol. 487, Astronomical Society of the Pacific, San Francisco, CA, pp. 389-393, Conference on Resolving the Future of Astronomy with Long-Baseline Interferometry, Socorro, 28/03/11. <http://aspbooks.org/custom/publications/paper/487-0389.html>

Some recent results from the CHARA Array. / ten Brummelaar, T. A.; Huber, David; von Braun, K.; Boyajian, T.; Richardson, N. D.; Schaefer, G.; Tallon-Bosc, I.; Mourard, D.; McAlister, H. A.; Turner, N. H.; Sturmann, L.; Sturmann, J.; Monnier, J. D.; Ireland, M.

Resolving the future of astronomy with long-baseline interferometry: proceedings of a conference held at New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA 28-31 March 2011. ed. / Michelle J. Creech-Eakman; Joyce A. Guzik; Robert E. Stencel. San Francisco, CA : Astronomical Society of the Pacific, 2014. p. 389-393 (Astronomical Society of the Pacific conference series; Vol. 487).

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

TY - GEN

T1 - Some recent results from the CHARA Array

AU - ten Brummelaar, T. A.

AU - Huber, David

AU - von Braun, K.

AU - Boyajian, T.

AU - Richardson, N. D.

AU - Schaefer, G.

AU - Tallon-Bosc, I.

AU - Mourard, D.

AU - McAlister, H. A.

AU - Turner, N. H.

AU - Sturmann, L.

AU - Sturmann, J.

AU - Monnier, J. D.

AU - Ireland, M.

PY - 2014

Y1 - 2014

N2 - The CHARA Array is a six 1-m telescope optical and near infrared interferometer located at the Mount Wilson Observatory in southern California and operated by the Center for High Angular Resolution Astronomy of Georgia State University. The CHARA Array has been in regular scientific operation since 2005 and now has over 55 publications in the refereed literature, including two in Science and one in Nature. The Array now supports seven beam combiners ranging from 0.5 microns up to 2.3 microns and combing from 2 to 4 beams at a time. An upgrade to a full 6-beam combiner is now underway, and fringes with all six telescopes were achieved soon after the meeting. We present some of the more recent results from the CHARA Array.

AB - The CHARA Array is a six 1-m telescope optical and near infrared interferometer located at the Mount Wilson Observatory in southern California and operated by the Center for High Angular Resolution Astronomy of Georgia State University. The CHARA Array has been in regular scientific operation since 2005 and now has over 55 publications in the refereed literature, including two in Science and one in Nature. The Array now supports seven beam combiners ranging from 0.5 microns up to 2.3 microns and combing from 2 to 4 beams at a time. An upgrade to a full 6-beam combiner is now underway, and fringes with all six telescopes were achieved soon after the meeting. We present some of the more recent results from the CHARA Array.

M3 - Conference proceeding contribution

SN - 9781583818589

T3 - Astronomical Society of the Pacific conference series

SP - 389

EP - 393

BT - Resolving the future of astronomy with long-baseline interferometry

A2 - Creech-Eakman, Michelle J.

A2 - Guzik, Joyce A.

A2 - Stencel, Robert E.

PB - Astronomical Society of the Pacific

CY - San Francisco, CA

T2 - Conference on Resolving the Future of Astronomy with Long-Baseline Interferometry

Y2 - 28 March 2011 through 31 March 2011

ER -

ten Brummelaar TA, Huber D, von Braun K, Boyajian T, Richardson ND, Schaefer G et al. Some recent results from the CHARA Array. In Creech-Eakman MJ, Guzik JA, Stencel RE, editors, Resolving the future of astronomy with long-baseline interferometry: proceedings of a conference held at New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA 28-31 March 2011. San Francisco, CA: Astronomical Society of the Pacific. 2014. p. 389-393. (Astronomical Society of the Pacific conference series).