Advances in optical/infrared interferometry
F Eisenhauer, JD Monnier… - Annual Review of …, 2023 - annualreviews.org
After decades of fast-paced technical advances, optical/infrared (O/IR) interferometry has
seen a revolution in recent years:▪ The GRAVITY instrument at the Very Large Telescope …
seen a revolution in recent years:▪ The GRAVITY instrument at the Very Large Telescope …
A guide to realistic uncertainties on the fundamental properties of solar-type exoplanet host stars
J Tayar, ZR Claytor, D Huber… - The Astrophysical …, 2022 - iopscience.iop.org
Our understanding of the properties and demographics of exoplanets critically relies on our
ability to determine the fundamental properties of their host stars. The advent of Gaia and …
ability to determine the fundamental properties of their host stars. The advent of Gaia and …
MIRC-X: a highly sensitive six-telescope interferometric imager at the CHARA array
Abstract Michigan InfraRed Combiner-eXeter (MIRC-X) is a new highly sensitive six-
telescope interferometric imager installed at the CHARA Array that provides an angular …
telescope interferometric imager installed at the CHARA Array that provides an angular …
Accurate fundamental parameters for 23 bright solar-type stars
H Bruntt, TR Bedding, PO Quirion… - Monthly Notices of …, 2010 - academic.oup.com
We combine results from interferometry, asteroseismology and spectroscopy to determine
accurate fundamental parameters of 23 bright solar-type stars, from spectral type F5 to K2 …
accurate fundamental parameters of 23 bright solar-type stars, from spectral type F5 to K2 …
Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA array
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 …
combiner at the CHARA Array to measure the angular sizes of five main-sequence stars …
The NN-explore exoplanet stellar speckle imager: Instrument description and preliminary results
A new speckle and wide-field imaging instrument for the WIYN telescope called NN-
EXPLORE Exoplanet Stellar Speckle Imager (NESSI) is described. NESSI offers …
EXPLORE Exoplanet Stellar Speckle Imager (NESSI) is described. NESSI offers …
Interferometric radii of bright Kepler stars with the CHARA Array: θ Cygni and 16 Cygni A and B
We present the results of long-baseline optical interferometry observations using the
Precision Astronomical Visual Observations (PAVO) beam combiner at the Center for High …
Precision Astronomical Visual Observations (PAVO) beam combiner at the Center for High …
VEGA: Visible spEctroGraph and polArimeter for the CHARA array: principle and performance
D Mourard, JM Clausse, A Marcotto, K Perraut… - Astronomy & …, 2009 - aanda.org
Context. Among optical stellar interferometers, the CHARA Array located at Mt Wilson in
California offers the potential of very long baselines (up to 330 m) and the prospect of …
California offers the potential of very long baselines (up to 330 m) and the prospect of …
Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades
The most powerful tests of stellar models come from the brightest stars in the sky, for which
complementary techniques, such as astrometry, asteroseismology, spectroscopy and …
complementary techniques, such as astrometry, asteroseismology, spectroscopy and …
First results from the hertzsprung SONG telescope: asteroseismology of the g5 subgiant star μ herculis
F Grundahl, MF Andersen… - The Astrophysical …, 2017 - iopscience.iop.org
We report the first asteroseismic results obtained with the Hertzsprung Stellar Observations
Network Group Telescope from an extensive high-precision radial-velocity observing …
Network Group Telescope from an extensive high-precision radial-velocity observing …