output
19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2012 · astro-ph.IMShow all

17 papers · 2 filters

astro-ph.IM2012★ 10 cited

GRAVITY: beam stabilization and light injection subsystems

O. Pfuhl, M. Haug, F. Eisenhauer +9

We present design results of the 2nd generation VLTI instrument GRAVITY beam stabilization and light injection subsystems. Designed to deliver micro-arcsecond astrometry, GRAVITY r…

astro-ph.IM2012★ 143 cited

SOPHIE+: First results of an octagonal-section fiber for high-precision radial velocity measurements

F. Bouchy, R. F. Diaz, G. Hébrard +5

High-precision spectrographs play a key role in exoplanet searches and Doppler asteroseismology using the radial velocity technique. The 1 m/s level of precision requires very high…

astro-ph.IM2012★ 1 cited

An experimental testbed for NEAT to demonstrate micro-pixel accuracy

A. Crouzier, F. Malbet, O. Preis +10

NEAT is an astrometric mission proposed to ESA with the objectives of detecting Earth-like exoplanets in the habitable zone of nearby solar-type stars. In NEAT, one fundamental asp…

astro-ph.IM2012★ 154 cited

SOAP. A tool for the fast computation of photometry and radial velocity induced by stellar spots

I. Boisse, X. Bonfils, N. C. Santos

We define and put at the disposal of the community SOAP, Spot Oscillation And Planet, a software tool that simulates the effect of stellar spots and plages on radial velocimetry an…

astro-ph.IM2012★ 10 cited

NEAT: a space born astrometric mission for the detection and characterization of nearby habitable planetary systems

Fabien Malbet, Renaud Goullioud, Pierre-Olivier Lagage +4

The NEAT (Nearby Earth Astrometric Telescope) mission is a proposal submitted to ESA for its 2010 call for M-size mission within the Cosmic Vision 2015-2025 plan. The main scientif…

astro-ph.IM2012★ 146 cited

Review of small-angle coronagraphic techniques in the wake of ground-based second-generation adaptive optics systems

Dimitri Mawet, Laurent Pueyo, Peter Lawson +26

Small-angle coronagraphy is technically and scientifically appealing because it enables the use of smaller telescopes, allows covering wider wavelength ranges, and potentially incr…

astro-ph.IM2012★ 7 cited

Advances in the Development of Mid-Infrared Integrated Devices for Interferometric Arrays

L. Labadie, Guillermo Martin, Airan Rodenas +7

This article reports the advances on the development of mid-infrared integrated optics for stellar interferometry. The devices are fabricated by laser writing techniques on chalcog…

astro-ph.IM2012★ 38 cited

Observing planet-disk interaction in debris disks

Steve Ertel, Sebastian Wolf, Jens Rodmann

Context. Structures in debris disks induced by planetdisk interaction are promising to provide valuable constraints on the existence and properties of embedded planets. Aims. We in…

astro-ph.IM2012★ 24 cited

Imaging the heart of astrophysical objects with optical long-baseline interferometry

J. -P. Berger, F. Malbet, F. Baron +21

The number of publications of aperture-synthesis images based on optical long-baseline interferometry measurements has recently increased due to easier access to visible and infrar…

astro-ph.IM2012★ 24 cited

On the sensitivity of closure phases to faint companions in optical long baseline interferometry

Jean-Baptiste Le Bouquin, Olivier Absil

We explore the sensitivity and completeness of long baseline interferometric observations for detecting unknown, faint companions around bright unresolved stars. We derive a linear…

astro-ph.IM2012★ 28 cited

Circumstellar disks and planets. Science cases for next-generation optical/infrared long-baseline interferometers

Sebastian Wolf, Fabien Malbet, Richard Alexander +10

We present a review of the interplay between the evolution of circumstellar disks and the formation of planets, both from the perspective of theoretical models and dedicated observ…

astro-ph.IM2012★ 46 cited

FIRST, a fibered aperture masking instrument. I. First on-sky test results

E. Huby, G. Perrin, F. Marchis +12

In this paper we present the first on-sky results with the fibered aperture masking instrument FIRST. Its principle relies on the combination of spatial filtering and aperture mask…

astro-ph.IM2012★ 40 cited

Speckle Temporal Stability in eXtreme Adaptive Optics Coronagraphic Images

P. Martinez, C. Loose, E. Aller Carpentier +1

The major noise source limiting high-contrast imaging is due to the presence of quasi-static speckles. Speckle noise originates from wavefront errors caused by various independent…

astro-ph.IM2012★ 15 cited

Atmospheric characterization of cold exoplanets using a 1.5-m coronagraphic space telescope

A. -L. Maire, R. Galicher, A. Boccaletti +5

Context. High-contrast imaging is currently the only available technique for the study of the thermodynamical and compositional properties of exoplanets in long-period orbits. The…

astro-ph.IM2012★ 26 cited

SPICES: Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems

Anthony Boccaletti, Jean Schneider, Wes Traub +28

SPICES (Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems) is a five-year M-class mission proposed to ESA Cosmic Vision. Its purpose is to image and charact…

astro-ph.IM2012★ 4 cited

Kinetic inductance detectors for millimeter and submillimeter astronomy / Détecteurs à inductance cinétique pour l'astronomie millimétrique et sub-millimétrique

Nicolas Boudou, Alain Benoit, Olivier Bourrion +5

We present recent developments in Kinetic Inductance Detectors (KID) for large arrays of detectors. The main application is ground-based millimeter wave astronomy. We focus in part…

astro-ph.IM2012★ 5 cited

Active optics Shack-Hartmann sensor: using spot sizes to measure the seeing at the focal plane of a telescope

P. Martinez, J. Kolb, M. Sarazin +1

Real-time seeing estimation at the focus of a telescope is nowadays strongly emphasized as this knowledge virtually drives the dimensioning of adaptive optics systems and instrumen…