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Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/271491
Description: 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 Astronom ... More
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Reviewed: Reviewed
Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/271584
Description: We present the first multiplicity-dedicated long-baseline optical interferometric survey of the Scorpius-Centaurus-Lupus-Crux association. We used the Sydney University Stellar Interferometer to under ... More
Reviewed: Reviewed
Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/271410
Description: We present interferometric observations of seven main-sequence and three giant stars with spectral types from B2 to F6 using the Precision Astronomical Visible Observations beam combiner at the Center ... More
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Reviewed: Reviewed
Authors: Ireland, M. J
Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/226900
Description: Bispectrum phase, closure phase and their generalization to kernel phase are all independent of pupil-plane phase errors to first order. This property, when used with sparse aperture masking behind ad ... More
Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/171003
Description: 21 page(s)
Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/195560
Description: We present an analysis of the WISE photometric data for 829 stars in the Sco-Cen OB2 association, using the latest high-mass membership probabilities. We detect infrared excesses associated with 135 B ... More
Reviewed: Reviewed
Date: 2011
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/152389
Description: We present four model series of the CODEX dynamical opacity-sampling models of Mira variables with solar abundances, designed to have parameters similar to o Cet, R Leo and R Cas. We demonstrate that ... More
Reviewed: Reviewed
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137689
Description: We have measured solar-like oscillations in red giants using time-series photometry from the first 34 days of science operations of the Kepler Mission. The light curves, obtained with 30 minute sampli ... More
Reviewed: Reviewed
Authors: Chaplin, W. J | Appourchaux, T | Brown, T. M | Aguirre, V. S | Stevens, I. R | Suárez, J. C | Suran, M. D | Trampedach, R | Turck-Chièze, S | Uytterhoeven, K | Ventura, R | Wilson, P. A | Christensen-Dalsgaard, J | Gilliland, R. L | Kjeldsen, H | Borucki, W. J | Koch, D | Jenkins, J. M | Ballot, J | Basu, S | Bazot, M | Elsworth, Y | Bedding, T. R | Benomar, O | Bonanno, A | Brandão, I. M | Bruntt, H | Campante, T. L | Creevey, O. L | Mauro, M. P. Di | Doğan, G | Dreizler, S | García, R. A | Eggenberger, P | Esch, L | Fletcher, S. T | Frandsen, S | Gai, N | Gaulme, P | Handberg, R | Hekker, S | Howe, R | Huber, D | Houdek, G | Korzennik, S. G | Lebrun, J. C | Leccia, S | Martic, M | Mathur, S | Mosser, B | New, R | Quirion, P.-O | Régulo, C | Roxburgh, I. W | Karoff, C | Salabert, D | Schou, J | Sousa, S. G | Stello, D | Verner, G. A | Arentoft, T | Barban, C | Belkacem, K | Benatti, S | Biazzo, K | Metcalfe, T. S | Boumier, P | Bradley, P. A | Broomhall, A.-M | Buzasi, D. L | Claudi, R. U | Cunha, M. S | D'Antona, F | Deheuvels, S | Derekas, A | Hernández, A. García | Molenda-Żakowicz, J | Giampapa, M. S | Goupil, M. J | Gruberbauer, M | Guzik, J. A | Hale, S. J | Ireland, M. J | Kiss, L. L | Kitiashvili, I. N | Kolenberg, K | Korhonen, H | Monteiro, M. J. P. F. G | Kosovichev, A. G | Kupka, F | Lebreton, Y | Leroy, B | Ludwig, H.-G | Mathis, S | Michel, E | Miglio, A | Montalbán, J | Moya, A | Thompson, M. J | Noels, A | Noyes, R. W | Pallé, P. L | Piau, L | Preston, H. L | Cortés, T. Roca | Roth, M | Sato, K. H | Schmitt, J | Serenelli, A. M
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137906
Description: We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-nois ... More
Reviewed: Reviewed
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137633
Description: The mid-infrared properties of pre-planetary disks are sensitive to the temperature and flaring profiles of disks for the regions where planet formation is expected to occur. In order to constrain the ... More
Reviewed: Reviewed
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137405
Description: Observations of the southern Cepheid ℓ Car to yield the mean angular diameter and angular pulsation amplitude have been made with the Sydney University Stellar Interferometer at a wavelength of 696 nm ... More
Reviewed: Reviewed
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137626
Description: We present results from a spectro-interferometric study of the Miras o Cet, R Leo, and W Hya obtained with the Keck Aperture Masking Experiment from 1998 September to 2002 July. The spectrally dispers ... More
Reviewed: Reviewed
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137408
Description: We have used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of the F9 V star β Virginis (β Vir). After correcting for limb darkening and combining with the revised ... More
Reviewed: Reviewed
Date: 2008
Language: eng
Resource Type: conference paper
Identifier: http://hdl.handle.net/1959.14/137255
Description: Observations of the southern Cepheids ℓ Car and β Dor to yield the mean angular diameters and angular pulsation amplitudes have been made with the Sydney University Stellar Interferometer (SUSI)at a w ... More
Reviewed: Reviewed