Search Results - "Ligi, Roxanne"
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Mass, Radius, and Composition of the Transiting Planet 55 Cnc e: Using Interferometry and Correlations
Published in The Astrophysical journal (20-06-2018)“…The characterization of exoplanets relies on that of their host star. However, stellar evolution models cannot always be used to derive the mass and radius of…”
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Journal Article -
2
Disentangling stellar activity from exoplanetary signals with interferometry
Published in EPJ Web of conferences (01-01-2015)“…Stellar activity can express as many forms at stellar surfaces: dark spots, convective cells, bright plages. Particularly, dark spots and bright plages add…”
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Journal Article Conference Proceeding -
3
Statistical tests with multi-wavelength Kernel-phase analysis for the detection and characterization of planetary companions
Published 09-08-2022“…Kernel phase is a method to interpret stellar point source images by considering their formation as the analytical result of an interferometric process. Using…”
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4
3-beam self-calibrated Kernel nulling photonic interferometer
Published 10-06-2022“…The use of interferometric nulling for the direct characterization of extrasolar planets is an exciting prospect, but one that faces many practical challenges…”
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5
High-contrast detection of exoplanets with a kernel-nuller at the VLTI
Published 27-04-2023“…A&A 676, A43 (2023) Context: The conventional approach to direct imaging has been the use of a single aperture coronagraph with wavefront correction via…”
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Mass, radius, and composition of the transiting planet 55 Cnc e : using interferometry and correlations
Published 13-12-2018“…The Astrophysical Journal, Volume 860, Issue 2, article id. 122, 12 pp. (2018) The characterization of exoplanets relies on that of their host star. However,…”
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Journal Article -
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Mass, radius, and composition of the transiting planet 55 Cnc e : using interferometry and correlations --- A quick update
Published 21-09-2018“…2018, Research Notes of the American Astronomical Society, vol. 2, number 3, 172 In a recent paper (Crida et al. 2018, accepted on April 19), we presented a…”
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Directly Determined Properties of HD 97658 from Interferometric Observations
Published 25-08-2021“…We conducted interferometric observations with the CHARA Array of transiting super-Earth host HD 97658 and measured its limb-darkened angular diameter to be…”
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CHARA/SPICA: a 6-telescope visible instrument for the CHARA Array
Published 17-10-2022“…SPIE Optical and Infrared Interferometry and Imaging VIII, p. 1218308 (2022) With a possible angular resolution down to 0.1-0.2 millisecond of arc using the…”
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From the stellar properties of HD219134 to the internal compositions of its transiting exoplanets
Published 30-10-2019“…A&A 631, A92 (2019) The harvest of exoplanet discoveries has opened the area of exoplanet characterisation. But this cannot be achieved without a careful…”
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K2 Targets Observed with SPHERE/VLT: An M4-7 Dwarf Companion Resolved around EPIC 206011496
Published 30-10-2018“…The quest to discover exoplanets is one of the most important missions in astrophysics, and is widely performed using the transit method, which allows for the…”
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Planet transit and stellar granulation detection with interferometry
Published 28-04-2014“…A&A 567, A115 (2014) Aims. We used realistic three-dimensional (3D) radiative hydrodynamical (RHD) simulations from the Stagger-grid and synthetic images…”
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Radii, masses, and ages of 18 bright stars using interferometry and new estimations of exoplanetary parameters
Published 14-02-2016“…A&A 586, A94 (2016) Accurate stellar parameters are needed in numerous domains of astrophysics. The position of stars on the H-R diagram is an important…”
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Journal Article -
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The operation of VEGA/CHARA : from the scientific idea to the final products
Published 23-02-2014“…Journal of Astronomical Instrumentation, 2013, 2, 1340003 We describe the data flow in the operation of the VEGA/CHARA instrument. After a brief summary of the…”
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Journal Article -
15
Science cases for a visible interferometer
Published 07-03-2017“…High spatial resolution is the key for the understanding various astrophysical phenomena. But even with the future E-ELT, single dish instruments are limited…”
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Journal Article