papers

Publications (61)

astro-ph.EP2021

The SPHERE infrared survey for exoplanets (SHINE)- I Sample definition and target characterization

S. Desidera, G. Chauvin, M. Bonavita +105

Large surveys with new-generation high-contrast imaging instruments are needed to derive the frequency and properties of exoplanet populations with separations from 5 to 300…

astro-ph2008

Wavefront error correction and Earth-like planet detection by Self-Coherent Camera in space

R. Galicher, P. Baudoz, G. Rousset

In the context of exoplanet detection, the performance of coronagraphs is limited by wavefront errors. To efficiently correct for these aberrations with a deformable mirror, it is…

astro-ph.IM2015

The Mid-Infrared Instrument for the James Webb Space Telescope, V: Predicted Performance of the MIRI Coronagraphs

A. Boccaletti, P. -O. Lagage, P. Baudoz +17

The imaging channel on the Mid-Infrared Instrument (MIRI) is equipped with four coronagraphs that provide high contrast imaging capabilities for studying faint point sources and ex…

astro-ph.IM2019

SPHERE: the exoplanet imager for the Very Large Telescope

J. -L. Beuzit, A. Vigan, D. Mouillet +108

Observations of circumstellar environments to look for the direct signal of exoplanets and the scattered light from disks has significant instrumental implications. In the past 15…

astro-ph.EP2018

Post conjunction detection of Pictoris b with VLT/SPHERE

A. -M. Lagrange, A. Boccaletti, M. Langlois +102

With an orbital distance comparable to that of Saturn in the solar system, \bpic b is the closest (semi-major axis \,9\,au) exoplanet that has been imaged to orbit a star.…

astro-ph.IM2017

High-contrast imaging at small separation: impact of the optical configuration of two deformable mirrors on dark holes

M. Beaulieu, L. Abe, P. Martinez +3

The direct detection and characterization of exoplanets will be a major scientific driver over the next decade, involving the development of very large telescopes and requires high…

astro-ph.EP2018

Discovery of a brown dwarf companion to the star HIP 64892

A. Cheetham, M. Bonnefoy, S. Desidera +89

We report the discovery of a bright, brown dwarf companion to the star HIP 64892, imaged with VLT/SPHERE during the SHINE exoplanet survey. The host is a B9.5V member of the Lower-…

astro-ph.IM2012

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.EP2014

Search for cool extrasolar giant planets combining coronagraphy, spectral and angular differential imaging

A. -L. Maire, A. Boccaletti, J. Rameau +8

Spectral differential imaging (SDI) is part of the observing strategy of current and on-going high-contrast imaging instruments on ground-based telescopes. Although it improves the…

astro-ph2008

Diversity among other worlds: characterization of exoplanets by direct detection

J. Schneider, A. Boccaletti, A. Aylward +34

The physical characterization of exoplanets will require to take spectra at several orbital positions. For that purpose, a direct imaging capability is necessary. Direct imaging re…

astro-ph.EP2019

Investigating the presence of two belts in the HD 15115 system

N. Engler, A. Boccaletti, H. M. Schmid +16

We present new observations of the edge-on debris disk around HD 15115 (F star at 48.2 pc) obtained in the near-IR. We search for observational evidence for a second inner planetes…

astro-ph.IM2022

JWST/MIRI coronagraphic performances as measured on-sky

A. Boccaletti, C. Cossou, P. Baudoz +16

Characterization of directly imaged exoplanets is one of the most eagerly anticipated science functions of the James Webb Space Telescope. MIRI, the mid-IR instrument has the capab…

astro-ph2008

Coronagraphic near-IR photometry of AB Dor C

A. Boccaletti, G. Chauvin, P. Baudoz +1

Observations of low-mass companions for which the dynamical masses are well constrained help to improve the calibration of evolutionary models. Such observations thereby provide mo…

astro-ph.IM2014

An aperture masking mode for the MICADO instrument

S. Lacour, P. Baudoz, E. Gendron +8

MICADO is a near-IR camera for the Europea ELT, featuring an extended field (75" diameter) for imaging, and also spectrographic and high contrast imaging capabilities. It has been…

astro-ph.EP2018

Observations of fast-moving features in the debris disk of AU Mic on a three-year timescale: Confirmation and new discoveries

A. Boccaletti, E. Sezestre, A. -M. Lagrange +60

The nearby and young M star AU Mic is surrounded by a debris disk in which we previously identified a series of large-scale arch-like structures that have never been seen before in…

astro-ph2005

Fundamental limitations on Earth-like planet detection with Extremely Large Telescopes

C. Cavarroc, A. Boccaletti, P. Baudoz +2

We analyse the fundamental limitations for the detection of extraterrestrial planets with Extremely Large Telescopes. For this task, a coronagraphic device combined to a very high…

astro-ph.EP2018

Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70

M. Keppler, M. Benisty, A. Müller +123

Young circumstellar disks are of prime interest to understand the physical and chemical conditions under which planet formation takes place. Only very few detections of planet cand…

astro-ph.EP2017

The circumstellar disk HD169142: gas, dust and planets acting in concert?

A. Pohl, M. Benisty, P. Pinilla +33

HD169142 is an excellent target to investigate signs of planet-disk interaction due to the previous evidence of gap structures. We performed J-band (~1.2μm) polarized intensit…

astro-ph2008

Super Earth Explorer: A Coronagraphic Off-Axis Space Telescope

J. Schneider, A. Boccaletti, D. Mawet +12

The Super-Earth Explorer is an Off-Axis Space Telescope (SEE-COAST) designed for high contrast imaging. Its scientific objective is to make the physico-chemical characterization of…

astro-ph.EP2010

Searching for sub-stellar companion into the LkCa15 proto-planetary disk

M. Bonavita, G. Chauvin, A. Boccaletti +8

Recent sub-millimetric observations at the Plateau de Bure interferometer evidenced a cavity at ~ 46 AU in radius into the proto-planetary disk around the T Tauri star LkCa15 (V107…

astro-ph.IM2016

Focal plane wavefront sensor achromatization : The multireference self-coherent camera

J. -R. Delorme, R. Galicher, P. Baudoz +3

High contrast imaging and spectroscopy provide unique constraints for exoplanet formation models as well as for planetary atmosphere models. But this can be challenging because of…

astro-ph.EP2014

Is the HD 15115 inner disk really asymmetrical ?

J. Mazoyer, A. Boccaletti, J. -C. Augereau +3

Context. Debris disks are intrinsically connected to the planetary system's formation and evolution. The development of high-contrast imaging techniques in the past 20 years is now…

astro-ph.EP2017

Discovery of a warm, dusty giant planet around HIP65426

G. Chauvin, S. Desidera, A. -M. Lagrange +120

The SHINE program is a large high-contrast near-infrared survey of 600 young, nearby stars. It is aimed at searching for and characterizing new planetary systems using VLT/SPHERE's…

astro-ph2007

Optimization of Apodized Pupil Lyot Coronagraph for ELTs

P. Martinez, A. Boccaletti, M. Kasper +2

We study the optimization of the Apodized Pupil Lyot Coronagraph (APLC) in the context of exoplanet imaging with ground-based telescopes. The APLC combines an apodization in the pu…

astro-ph.EP2025

The SPHERE infrared survey for exoplanets (SHINE). V. Complete observations, data reduction and analysis, detection performances, and final results

A. Chomez, P. Delorme, A. -M. Lagrange +117

During the past decade, state-of-the-art planet-finder instruments like SPHERE@VLT, coupling coronagraphic devices and extreme adaptive optics systems, unveiled, thanks to large su…

astro-ph2007

Expected Performance of a Self-Coherent Camera

R. Galicher, P. Baudoz

Residual wavefront errors in optical elements limit the performance of coronagraphs. To improve their efficiency, different types of devices have been proposed to correct or calibr…

astro-ph.EP2025

JWST/MIRI observations of the young TWA 27 system: hydrocarbon disk chemistry, silicate clouds, evidence for a CPD

P. Patapis, M. Morales-Calderón, A. M. Arabhavi +39

The Mid-Infrared Instrument (MIRI) on the James Webb Space Telescope (JWST) enables the characterisation of young self-luminous gas giants at previously inaccessible wavelengths, r…

astro-ph.IM2018

SPHERE / ZIMPOL high resolution polarimetric imager. I. System overview, PSF parameters, coronagraphy, and polarimetry

H. M. Schmid, A. Bazzon, R. Roelfsema +59

We describe the Zurich Imaging Polarimeter (ZIMPOL), the visual focal plane subsystem of the SPHERE "VLT planet finder", which pushes the limits of current AO systems to shorter wa…

astro-ph.EP2014

Search for cool giant exoplanets around young and nearby stars - VLT/NaCo near-infrared phase-coronagraphic and differential imaging

A. -L. Maire, A. Boccaletti, J. Rameau +8

[Abridged] Context. Spectral differential imaging (SDI) is part of the observing strategy of current and future high-contrast imaging instruments. It aims to reduce the stellar spe…

astro-ph.EP2019

A search for accreting young companions embedded in circumstellar disks: High-contrast H imaging with VLT/SPHERE

G. Cugno, S. P. Quanz, S. Hunziker +37

Aims: We want to detect and quantify observables related to accretion processes occurring locally in circumstellar disks, which could be attributed to young forming planets. We foc…

astro-ph2002

High Dynamic Range and the Search for Planets

A. T. Tokunaga, C. Ftaclas, J. R. Kuhn +1

General arguments for optimized coronagraphy in the search for planets are presented. First, off-axis telescopes provide the best telescopic platforms for use with coronagraphy, an…

astro-ph.EP2021

First light of the VLT planet finder SPHERE. III. New spectrophotometry and astrometry of the HR8799 exoplanetary system

A. Zurlo, A. Vigan, R. Galicher +70

The planetary system discovered around the young A-type HR8799 provides a unique laboratory to: a) test planet formation theories, b) probe the diversity of system architectures at…

astro-ph.IM2011

Multi-stage four-quadrant phase mask: achromatic coronagraph for space-based and ground-based telescopes

R. Galicher, P. Baudoz, J. Baudrand

Less than 3% of the known exoplanets were directly imaged for two main reasons. They are angularly very close to their parent star, which is several magnitudes brighter. Direct ima…

astro-ph.IM2022

Upgrading the high contrast imaging facility SPHERE: science drivers and instrument choices

A. Boccaletti, G. Chauvin, F. Wildi +71

SPHERE+ is a proposed upgrade of the SPHERE instrument at the VLT, which is intended to boost the current performances of detection and characterization for exoplanets and disks. S…

astro-ph.EP2021

The SPHERE infrared survey for exoplanets (SHINE) -- II. Observations, Data reduction and analysis Detection performances and early-results

M. Langlois, R. Gratton, A. -M. Lagrange +118

Over the past decades, direct imaging has confirmed the existence of substellar companions (exoplanets or brown dwarfs) on wide orbits (>10 au) from their host stars. To understand…

astro-ph.EP2019

Blobs, spiral arms, and a possible planet around HD 169142

R. Gratton, R. Ligi, E. Sissa +24

Young planets are expected to cause perturbations in protostellar disks that may be used to infer their presence. Clear detection of still-forming planets embedded within gas-rich…

astro-ph.EP2016

Discovery of concentric broken rings at sub-arcsec separations in the HD 141569A gas-rich, debris disk with VLT/SPHERE

C. Perrot, A. Boccaletti, E. Pantin +45

Transition disks correspond to a short stage between the young protoplanetary phase and older debris phase. Along this evolutionary sequence, the gas component disappears leaving r…

astro-ph.IM2019

Exoplanet direct imaging in ground-based conditions on THD2 bench

A. Potier, P. Baudoz, R. Galicher +2

The next generation of ground-based instruments aims to break through the knowledge we have on exoplanets by imaging circumstellar environments always closer to the stars. However,…

astro-ph.IM2013

L'-band AGPM vector vortex coronagraph's first light on VLT/NACO: Discovery of a late-type companion at two beamwidths from an F0V star

D. Mawet, O. Absil, C. Delacroix +20

Context. High contrast imaging has thoroughly combed through the limited search space accessible with first-generation ground-based adaptive optics instruments and the Hubble Space…

astro-ph.IM2021

The vector-apodizing phase plate coronagraph: design, current performance, and future development

D. S. Doelman, F. Snik, E. H. Por +50

Over the last decade, the vector-apodizing phase plate (vAPP) coronagraph has been developed from concept to on-sky application in many high-contrast imaging systems on 8-m class t…

astro-ph.IM2024

The MICADO first light imager for the ELT: overview and current Status

E. Sturm, R. Davies, J. Alves +151

MICADO is a first light instrument for the Extremely Large Telescope (ELT), set to start operating later this decade. It will provide diffraction limited imaging, astrometry, high…

astro-ph.IM2013

Estimation and correction of wavefront aberrations using the self-coherent camera: laboratory results

J. Mazoyer, P. Baudoz, R. Galicher +2

Direct imaging of exoplanets requires very high contrast levels, which are obtained using coronagraphs. But residual quasi-static aberrations create speckles in the focal plane dow…

astro-ph.EP2024

Water depletion and 15NH3 in the atmosphere of the coldest brown dwarf observed with JWST/MIRI

H. Kühnle, P. Patapis, P. Mollière +21

With a temperature of K WISE0855 is the coldest brown dwarf observed so far. Using the James Webb Space Telescope (JWST) we obtained observations that allow us to charac…

astro-ph2008

Theory and laboratory tests of the multi-stage phase mask coronagraph

P. Baudoz, R. Galicher, J. Baudrand +1

A large number of coronagraphs have been proposed to overcome the ratio that exists between the star and its planet. The planet finder of the Extremely Large Telescope, which is ca…

astro-ph.EP2026

The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization

V. Squicciarini, S. Desidera, G. Chauvin +109

Unbiased surveys of large stellar samples are the prime means through which the prevalence of exoplanets can be derived, and crucial constraints to planet formation models can be s…

astro-ph.IM2018

Review of high-contrast imaging systems for current and future ground- and space-based telescopes I. Coronagraph design methods and optical performance metrics

G. Ruane, A. Riggs, J. Mazoyer +29

The Optimal Optical Coronagraph (OOC) Workshop at the Lorentz Center in September 2017 in Leiden, the Netherlands gathered a diverse group of 25 researchers working on exoplanet in…

astro-ph.EP2020

SPHERE+: Imaging young Jupiters down to the snowline

A. Boccaletti, G. Chauvin, D. Mouillet +130

SPHERE (Beuzit et al,. 2019) has now been in operation at the VLT for more than 5 years, demonstrating a high level of performance. SPHERE has produced outstanding results using a…

astro-ph.EP2025

The planetary-mass-limit VLT/SINFONI library: Spectral extraction and atmospheric characterization via forward modeling

P. Palma-Bifani, M. Bonnefoy, G. Chauvin +9

We aim to deepen our understanding of the M-L transition on planetary-mass companions and isolated brown dwarfs, and search for evidence of possible differences between these two p…

astro-ph.EP2019

Spatially resolved spectroscopy of the debris disk HD 32297: Further evidence of small dust grains

T. Bhowmik, A. Boccaletti, P. Thébault +14

Spectro-photometry of debris disks in total intensity and polarimetry can provide new insight into the properties of the dust grains therein (size distribution and optical properti…

astro-ph.IM2020

High contrast at small separation -- II. Impact on the dark hole of a realistic optical set-up with two deformable mirrors

M. Beaulieu, P. Martinez, L. Abe +3

Future large space- or ground-based telescopes will offer the resolution and sensitivity to probe the habitable zone of a large sample of nearby stars for exo-Earth imaging. To thi…

astro-ph.EP2024

Atmospheric properties of AF Lep b with forward modeling

P. Palma-Bifani, G. Chauvin, D. Borja +11

Aims. We aim to expand the atmospheric exploration of AF Lep b by modeling all available observations obtained with SPHERE at VLT (between 0.95-1.65, at 2.105, and 2.253 m, and…

astro-ph.EP2019

RefPlanets: Search for reflected light from extra-solar planets with SPHERE/ZIMPOL

S. Hunziker, H. M. Schmid, D. Mouillet +55

RefPlanets is a guaranteed time observation (GTO) programme that uses the Zurich IMaging POLarimeter (ZIMPOL) of SPHERE/VLT for a blind search for exoplanets in wavelengths from 60…

astro-ph.IM2026

Vector Apodizing Phase Plates for the ELT: From prototype to final optics for METIS and MICADO

J. A. van den Born, R. Landman, D. S. Doelman +12

The first generation of instruments for the upcoming Extremely Large Telescope (ELT) will allow for the direct imaging of exoplanets that were previously below the sensitivity or r…

astro-ph.EP2015

First light of the VLT planet finder SPHERE. I. Detection and characterization of the sub-stellar companion GJ 758 B

A. Vigan, M. Bonnefoy, C. Ginski +72

GJ758 B is a brown dwarf companion to a nearby (15.76 pc) solar-type, metal-rich (M/H = +0.2 dex) main-sequence star (G9V) that was discovered with Subaru/HiCIAO in 2009. From prev…

astro-ph.EP2023

Peering into the Young Planetary System AB Pic. Atmosphere, Orbit, Obliquity & Second Planetary Candidate

P. Palma-Bifani, G. Chauvin, M. Bonnefoy +24

We aim to revisit the system AB Pic which has a known companion at the exoplanet/ brown-dwarf boundary. We based this study on a rich set of observations to investigate the compani…

astro-ph.EP2020

The SPHERE infrared survey for exoplanets (SHINE). III. The demographics of young giant exoplanets below 300 au with SPHERE

A. Vigan, C. Fontanive, M. Meyer +108

The SHINE project is a 500-star survey performed with SPHERE on the VLT for the purpose of directly detecting new substellar companions and understanding their formation and early…

astro-ph.IM2016

MICADO: first light imager for the E-ELT

R. Davies, J. Schubert, M. Hartl +80

MICADO will equip the E-ELT with a first light capability for diffraction limited imaging at near-infrared wavelengths. The instrument's observing modes focus on various flavours o…

astro-ph2002

Hokupa'a-Gemini Discovery of Two Ultracool Companions to the Young Star HD 130948

D. Potter, E. L. Martín, M. C. Cushing +4

We report the discovery of two faint ultracool companions to the nearby (d~17.9 pc) young G2V star HD 130948 (HR 5534, HIP 72567) using the Hokupa'a adaptive optics instrument moun…

astro-ph.EP2019

The Potential of Exozodiacal Disks Observations with the WFIRST Coronagraph Instrument

B. Mennesson, V. Bailey, J. Kasdin +60

The Wide Field Infrared Survey Telescope (WFIRST) Coronagraph Instrument (CGI) will be the first high-performance stellar coronagraph using active wavefront control for deep starli…

astro-ph.SR2009

VLT/NACO coronagraphic observations of fine structures in the disk of beta Pictoris

A. Boccaletti, J. -C. Augereau, P. Baudoz +2

We present ground-based observations of the disk around the A-type star Pictoris to perform a close inspection of the inner disk morphology. Images were collected with NACO, t…

astro-ph.IM2016

Laboratory validation of the dual-zone phase mask coronagraph in broadband light at the high-contrast imaging THD-testbed

J. R. Delorme, M. N'Diaye, R. Galicher +6

Specific high contrast imaging instruments are mandatory to characterize circumstellar disks and exoplanets around nearby stars. Coronagraphs are commonly used in these facilities…