Hi-5: a potential high-contrast thermal near-infrared imager for the VLTI

D. Defrère, M. Ireland, O. Absil +25

The Araucaria Project: The First-Overtone Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-2532

B. Pilecki, D. Graczyk, W. Gieren +10

The Araucaria Project. OGLE-LMC-CEP-1718: An exotic eclipsing binary system composed of two classical overtone Cepheids in a 413-day orbit

W. Gieren, B. Pilecki, G. Pietrzynski +11

Multiplicity of Galactic Cepheids from long-baseline interferometry. II. The Companion of AX Circini revealed with VLTI/PIONIER

A. Gallenne, A. Mérand, P. Kervella +6

Binary Cepheids from optical interferometry

A. Gallenne, P. Kervella, A. Mérand +3

Shadows and asymmetries in the T Tauri disk HD 143006: Evidence for a misaligned inner disk

M. Benisty, A. Juhasz, S. Facchini +13

Investigating Cepheid $\ell$ Carinae's Cycle-to-cycle Variations via Contemporaneous Velocimetry and Interferometry

R. I. Anderson, A. Mérand, P. Kervella +8

Extended envelopes around Galactic Cepheids IV. T Monocerotis and X Sagittarii from mid-infrared interferometry with VLTI/MIDI

A. Gallenne, A. Merand, P. Kervella +3

The close circumstellar environment of Betelgeuse - III. SPHERE/ZIMPOL visible polarimetry of the inner envelope and photosphere

P. Kervella, E. Lagadec, M. Montargès +7

A geometrical 1% distance to the short-period binary Cepheid V1334 Cygni

A. Gallenne, P. Kervella, N. R. Evans +18

Observational calibration of the projection factor of Cepheids IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids

A. Gallenne, P. Kervella, A. Mérand +4

Molecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments

A. Smette, H. Sana, S. Noll +10

Four years' interferometric observations of Galactic binary Cepheids

A. Gallenne, A. Merand, P. Kervella +4

VEGA/CHARA interferometric observations of Cepheids. I. A resolved structure around the prototype classical Cepheid delta Cep in the visible spectral range

N. Nardetto, A. Mérand, D. Mourard +23

The path towards high-contrast imaging with the VLTI: the Hi-5 project

D. Defrère, O. Absil, J. -P. Berger +26

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

N. Nardetto, E. Poretti, M. Rainer +13

Robust high-contrast companion detection from interferometric observations. The CANDID algorithm and an application to six binary Cepheids

A. Gallenne, A. Mérand, P. Kervella +15

The long-period Galactic Cepheid RS Puppis - III. A geometric distance from HST polarimetric imaging of its light echoes

P. Kervella, H. E. Bond, M. Cracraft +8

Refined parameters and spectroscopic transit of the super-massive planet HD147506b

B. Loeillet, A. Shporer, F. Bouchy +26

An interferometric view on binarity and circumstellar envelopes of Cepheids

A. Gallenne, P. Kervella, A. Mérand +4

Multiplicity of Galactic Cepheids from long-baseline interferometry. IV. New detected companions from MIRC and PIONIER observations

A. Gallenne, P. Kervella, S. Borgniet +10

The dust disk and companion of the nearby AGB star L2 Puppis - SPHERE/ZIMPOL polarimetric imaging at visible wavelengths

P. Kervella, M. Montargès, E. Lagadec +6

Searching for visual companions of close Cepheids. VLT/NACO lucky imaging of Y~Oph, FF~Aql, X~Sgr, W~Sgr and $η$~Aql

A. Gallenne, P. Kervella, A. Mérand +4

Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2 - I. Binarity from proper motion anomaly

P. Kervella, A. Gallenne, N. R. Evans +8

Mean angular diameters, distances and pulsation modes of the classical Cepheids FF Aql and T Vul - CHARA/FLUOR near-infrared interferometric observations

A. Gallenne, P. Kervella, A. Mérand +8

The Araucaria Project. Precise physical parameters of the eclipsing binary IO Aqr

D. Graczyk, P. F. L. Maxted, G. Pietrzynski +11

The Araucaria Project. Binary Classical Cepheids in the LMC

D. Graczyk, B. Pilecki, G. Pietrzyński +5

The SOPHIE search for northern extrasolar planets III. A Jupiter-mass companion around HD 109246

I. Boisse, A. Eggenberger, N. C. Santos +22

Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227

B. Pilecki, D. Graczyk, G. Pietrzyński +14

Multiplicity of Galactic Cepheids from long-baseline interferometry~III. Sub-percent limits on the relative brightness of a close companion of $δ$~Cephei

A. Gallenne, A. Merand, P. Kervella +11

The effect of metallicity on Cepheid Period-Luminosity relations from a Baade-Wesselink analysis of Cepheids in the Milky Way and Magellanic Clouds

W. Gieren, J. Storm, P. Konorski +14

The Araucaria Project. A Distance Determination to the Local Group Spiral M33 from Near-Infrared Photometry of Cepheid Variables

W. Gieren, M. Gorski, G. Pietrzynski +10

Fundamental properties of red-clump stars from long-baseline H-band interferometry

A. Gallenne, G. Pietrzyński, D. Graczyk +7

Dynamical masses of Cepheids from the GAIA parallaxes

A. Gallenne, P. Kervella, A. Merand +2

Multiplicity of Galactic Cepheids from long-baseline interferometry I. CHARA/MIRC detection of the companion of V1334 Cygni

A. Gallenne, J. D. Monnier, A. Mérand +16

The Araucaria Project: High-precision orbital parallax and masses of the eclipsing binary TZ~Fornacis

A. Gallenne, G. Pietrzyński, D. Graczyk +6

A distance to the Large Magellanic Cloud that is precise to one per cent

G. Pietrzynski, D. Graczyk, A. Gallenne +19

Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2 -- II. Resolved common proper motion pairs

P. Kervella, A. Gallenne, N. R. Evans +6

The study uses Gaia DR2 proper motion data to identify wide, spatially resolved common proper motion companions of Galactic Cepheid and RR Lyrae stars, reporting several high‑proba…

The radii and limb darkenings of Alpha Centauri A and B - Interferometric measurements with VLTI/PIONIER

P. Kervella, L. Bigot, A. Gallenne +1

CRIRES high-resolution infrared spectroscopy of the long-period Cepheid l Car

N. Nardetto, E. Poretti, A. Gallenne +17

An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent

G. Pietrzyński, D. Graczyk, W. Gieren +25