[HTML][HTML] 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 …
First light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope Interferometer
GRAVITY is a new instrument to coherently combine the light of the European Southern
Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 …
Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 …
Optical interferometry
A Quirrenbach - Annual Review of Astronomy and Astrophysics, 2001 - annualreviews.org
▪ Abstract The field of optical and infrared (IR) interferometry has seen rapid technical and
scientific progress over the past few years. A number of instruments capable of precise …
scientific progress over the past few years. A number of instruments capable of precise …
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 …
[HTML][HTML] AMBER, the near-infrared spectro-interferometric three-telescope VLTI instrument
Context. Optical long-baseline interferometry is moving a crucial step forward with the
advent of general-user scientific instruments that equip large aperture and hectometric …
advent of general-user scientific instruments that equip large aperture and hectometric …
Mass-radius relation of low and very low-mass stars revisited with the VLTI
BO Demory, D Ségransan, T Forveille… - Astronomy & …, 2009 - aanda.org
We measured the radii of 7 low and very low-mass stars using long baseline interferometry
with the VLTI interferometer and its VINCI and AMBER near-infrared recombiners. We use …
with the VLTI interferometer and its VINCI and AMBER near-infrared recombiners. We use …
First radius measurements of very low mass stars with the VLTI
D Segransan, P Kervella, T Forveille… - Astronomy & …, 2003 - aanda.org
We present 4 very low mass stars radii measured with the VLTI using the 2.2 μm VINCI test
instrument. The observations were carried out during the commissioning of the 104-meter …
instrument. The observations were carried out during the commissioning of the 104-meter …
[HTML][HTML] Radiative hydrodynamics simulations of red supergiant stars-I. interpretation of interferometric observations
Context. It has been proposed that convection in red supergiant (RSG) stars produces large-
scale granules causing observable surface inhomogeneities. This convection is also …
scale granules causing observable surface inhomogeneities. This convection is also …
[HTML][HTML] 2023 Astrophotonics Roadmap: pathways to realizing multi-functional integrated astrophotonic instruments
N Jovanovic, P Gatkine, N Anugu… - Journal of Physics …, 2023 - iopscience.iop.org
Photonic technologies offer numerous functionalities that can be used to realize
astrophotonic instruments. The most spectacular example to date is the ESO Gravity …
astrophotonic instruments. The most spectacular example to date is the ESO Gravity …
[HTML][HTML] Imaging the spotty surface of Betelgeuse in the H band
X Haubois, G Perrin, S Lacour, T Verhoelst… - Astronomy & …, 2009 - aanda.org
Aims. This paper reports on H-band interferometric observations of Betelgeuse made at the
three-telescope interferometer IOTA. We image Betelgeuse and its asymmetries to …
three-telescope interferometer IOTA. We image Betelgeuse and its asymmetries to …