activity
19992021
most citedInterferometric data reduction with AMBER/VLTI.Principle,estimators and illustration

291 citations · 871 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2021★ 50 cited

A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds

J. G. Winters, R. Cloutier, A. A. Medina +79

LTT 1445 is a hierarchical triple M-dwarf star system located at a distance of 6.86 parsecs. The primary star LTT 1445A (0.257 M_Sun) is known to host the transiting planet LTT 144…

astro-ph.SR2009★ 71 cited

Candidate free-floating super-Jupiters in the young sigma Orionis open cluster

G. Bihain, R. Rebolo, M. R. Zapatero Osorio +13

Free-floating substellar candidates with estimated theoretical masses of as low as ~5 Jupiter masses have been found in the ~3 Myr old sigma Orionis open cluster. As the overlap wi…

astro-ph.SR2009★ 193 cited

Mass-radius relation of low and very low-mass stars revisited with the VLTI

B. -O. Demory, D. Segransan, T. Forveille +7

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 the…

astro-ph2008★ 17 cited

Optical configuration and analysis of the AMBER/VLTI instrument

S. Robbe-Dubois, S. Lagarde, R. G. Petrov +23

This paper describes the design goals and engineering efforts that led to the realization of AMBER (Astronomical Multi BEam combineR) and to the achievement of its present performa…

astro-ph2007★ 26 cited

Initial mass function effects on the colour evolution of disk galaxies

P. Westera, M. Samland, S. J. Kautsch +2

In this work, we want to find out if the IMF can be determined from colour images, integrated colours, or mass-to-light ratios, especially at high redshift, where galaxies cannot b…

astro-ph2006★ 108 cited

Near-Infrared interferometry of Eta Carinae with high spatial and spectral resolution using the VLTI and the AMBER instrument

G. Weigelt

We present the first NIR spectro-interferometry of the LBV Eta Carinae. The K band observations were performed with the AMBER instrument of the ESO Very Large Telescope Interferome…