Simulating a dual beam combiner at SUSI for narrow-angle astrometry

Autor: Yitping Kok, J. Gordon Robertson, Michael J. Ireland, Vicente Maestro, Peter G. Tuthill

Publikováno v: Experimental Astronomy. 36:195-221

The Sydney University Stellar Interferometer (SUSI) has two beam combiners, i.e. the Precision Astronomical Visible Observations (PAVO) and the Microarcsecond University of Sydney Companion Astrometry (MUSCA). The primary beam combiner, PAVO, can be

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc2e8cf4971131630afdf51189c96384
https://doi.org/10.1007/s10686-013-9331-8

Stellar diameters and temperatures - VI. High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfs

Autor: Stephen R. Kane, Gail H. Schaefer, Gregory A. Feiden, Gerard T. van Belle, Jeremy Jones, Pierre Demarque, Stephen T. Ridgway, Daniel Huber, Laszlo Sturmann, Chris Farrington, David R. Ciardi, Nils H. Turner, Sarbani Basu, Tabetha S. Boyajian, P. J. Goldfinger, T. ten Brummelaar, C. Brooke Lamell, Kaspar von Braun, Mercedes Lopez-Morales, Andrew W. Mann, Vicente Maestro, Debra A. Fischer, John M. Brewer, Harold A. McAlister, Federico Spada, Timothy R. White, Michael J. Ireland

We present direct radii measurements of the well-known transiting exoplanet host stars HD 189733 and HD 209458 using the CHARA Array interferometer. We find the limb-darkened angular diameters to be theta_LD = 0.3848 +/- 0.0055 and 0.2254 +/- 0.0072

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::120c348acc06ecd6015d2932d8a62e76

The physical parameters of the retired a star HD 185351

Autor: Thomas Barclay, Daniel Huber, Vicente Maestro, Kaspar von Braun, Timothy R. White, Dennis Stello, Tabetha S. Boyajian, John Asher Johnson, John M. Brewer

Publikováno v: Johnson, J A, Huber, D, Boyajian, T, Brewer, J M, White, T R, Von Braun, K, Maestro, V, Stello, D & Barclay, T 2014, ' The physical parameters of the retired a star HD 185351 ', Astrophysical Journal, vol. 794, no. 1, 15 . https://doi.org/10.1088/0004-637X/794/1/15

We report here an analysis of the physical stellar parameters of the giant star HD185351 using Kepler short-cadence photometry, optical and near infrared interferometry from CHARA, and high-resolution spectroscopy. Asteroseismic oscillations detected

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https://pure.au.dk/portal/da/publications/the-physical-parameters-of-the-retired-a-star-hd-185351(157929e8-0913-4e78-97d2-94bd8c02b51c).html

Interferometric radii of bright Kepler stars with the CHARA Array: θ Cygni and 16 Cygni A and B

Autor: Harold A. McAlister, Nils H. Turner, Judit Sturmann, Daniel Huber, Benjamin J. S. Pope, Timothy R. White, Timothy R. Bedding, Gail Schaefer, P. J. Goldfinger, John D. Monnier, T. ten Brummelaar, Rachael M. Roettenbacher, Tabetha S. Boyajian, Vicente Maestro, Laszlo Sturmann, Michael J. Ireland, Peter G. Tuthill, Chris Farrington, Dennis Stello, Fabien Baron, Xiao Che

Publikováno v: White, T R, Huber, D, Maestro, V, Bedding, T R, Ireland, M J, Baron, F, Boyajian, T S, Che, X, Monnier, J D, Pope, B J S, Roettenbacher, R M, Stello, D, Tuthill, P G, Farrington, C D, Goldfinger, P J, McAlister, H A, Schaefer, G H, Sturmann, J, Sturmann, L, ten Brummelaar, T A & Turner, N H 2013, ' Interferometric radii of bright Kepler stars with the CHARA Array: θ Cygni and 16 Cygni A and B ', Royal Astronomical Society. Monthly Notices, vol. 433, no. 2, pp. 1262-1270 . https://doi.org/10.1093/mnras/stt802

We present the results of long-baseline optical interferometry observations using the Precision Astronomical Visual Observations (PAVO) beam combiner at the Center for High Angular Resolution Astronomy (CHARA) Array to measure the angular sizes of th

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https://pure.au.dk/portal/da/publications/interferometric-radii-of-bright-kepler-stars-with-the-chara-array--cygni-and-16-cygni-a-and-b(5dbc11f5-1f3f-4b6f-8ad1-10b1591f1a7d).html

Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA Array

Autor: J. Christensen-Dalsgaard, Martin C. Stumpe, Chris Farrington, Andrea Miglio, Michael Ireland, Neal J. Turner, Joanna Molenda-Żakowicz, H. A. McAlister, Luca Casagrande, H. Kjeldsen, P. J. Goldfinger, K. Uytterhoeven, H. Bruntt, Antonio Frasca, Vicente Maestro, V. Silva Aguirre, T. ten Brummelaar, Michael Thompson, T. S. Metcalfe, Daniel Huber, R. A. Garcia, T. R. Bedding, S. G. Sousa, Thomas Barclay, Timothy R. White, I. M. Brandão, M. S. Cunha, R. L. Gilliland, Christopher J. Burke, J. Sturmann, Marc H. Pinsonneault, S. Hekker, William J. Chaplin, Steven D. Kawaler, L. Sturmann, L. Piau, Mário J. P. F. G. Monteiro, Gail Schaefer, J. De Ridder, D. Stello

Publikováno v: The Astrophysical Journal
Astrophysical Journal, 760(1). IOP Publishing Ltd.
Huber, D, Ireland, M J, Bedding, T R, Maestro, V, White, T R, Stello, D, Brandão, I M, Sousa, S G, Cunha, M S, Monteiro, M J P F G, Piau, L, Bruntt, H, Aguirre, V S, Chaplin, W J, Christensen-Dalsgaard, J, Kjeldsen, H, Casagrande, L, Molenda-Zakowicz, J, Barclay, T, Burke, C J, Stumpe, M C, Miglio, A, De Ridder, J, Farrington, C D, Goldfinger, P J, McAlister, H A, Schaefer, G H, Sturmann, J, Sturmann, L, Ten Brummelaar, T A, Turner, N, Frasca, A, García, R A, Gilliland, R L, Hekker, S, Kawaler, S D, Metcalfe, T S, Pinsonneault, M H, Thompson, M J & Uytterhoeven, K 2012, ' Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA Array ', Astrophysical Journal, vol. 760, no. 1 . https://doi.org/10.1088/0004-637X/760/1/32

We present results of a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array to measure the angular sizes of five main-sequence stars, one subgiant and four red giant stars for which solar-like oscillations have been

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5c9af01e9b4d0158d176649c0138be6