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View article: Exomoon search with VLTI/GRAVITY around the substellar companion HD 206893 B
Exomoon search with VLTI/GRAVITY around the substellar companion HD 206893 B Open
Direct astrometric detection of exomoons remains unexplored. This study presents the first application of high-precision astrometry to search for exomoons around substellar companions. We investigate whether the orbital motion of the compa…
View article: Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432 <i>(Corrigendum)</i>
Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432 <i>(Corrigendum)</i> Open
Contains fulltext : 318351.pdf (Publisher’s version ) (Open Access)
View article: Adaptive optics telemetry standard
Adaptive optics telemetry standard Open
Context . The amount of adaptive optics (AO) telemetry generated by visible/near-infrared ground-based observatories is ever greater, leading to a growing need for a standardised data exchange format to support performance analysis, AO res…
View article: Upgrading the GRAVITY fringe tracker for GRAVITY+
Upgrading the GRAVITY fringe tracker for GRAVITY+ Open
Context. The GRAVITY beam-combiner at the Very Large Telescope Interferometer has recently made important contributions to many different fields of astronomy, from observations of the Galactic centre to the study of massive stars, young st…
View article: Upgrading the GRAVITY fringe tracker for GRAVITY+: Tracking the white light fringe in the non-observable Optical Path Length state-space
Upgrading the GRAVITY fringe tracker for GRAVITY+: Tracking the white light fringe in the non-observable Optical Path Length state-space Open
Aims. As part of the ongoing GRAVITY+ upgrade of the Very Large Telescope Interferometer infrastructure, we aim to improve the performance of the GRAVITY Fringe-Tracker, and to enable its use by other instruments. Methods. We modify the gr…
View article: The GRAVITY young stellar object survey XIII. Tracing the time-variable asymmetric disk structure in the inner AU of the Herbig star HD98922
The GRAVITY young stellar object survey XIII. Tracing the time-variable asymmetric disk structure in the inner AU of the Herbig star HD98922 Open
Temporal variability in the photometric and spectroscopic properties of protoplanetary disks is common in YSO. However, evidence pointing toward changes in their morphology over short timescales has only been found for a few sources, mainl…
View article: The GRAVITY young stellar object survey
The GRAVITY young stellar object survey Open
Context . Temporal variability in the photometric and spectroscopic properties of protoplanetary disks is common in young stellar objects. However, evidence pointing toward changes in their morphology over short timescales has only been fo…
View article: Adaptive Optics Telemetry Standard: Design and specification of a novel data exchange format
Adaptive Optics Telemetry Standard: Design and specification of a novel data exchange format Open
The amount of Adaptive Optics (AO) telemetry generated by VIS/NIR ground-based observatories is ever greater, leading to a growing need for a standardised data exchange format to support performance analysis and AO research and development…
View article: Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432
Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432 Open
Context. Rocky planets form by the concentration of solid particles in the inner few au regions of planet-forming disks. Their chemical composition reflects the materials in the disk available in the solid phase at the time the planets wer…
View article: Integrated turbulence parameters' estimation from NAOMI adaptive optics telemetry data
Integrated turbulence parameters' estimation from NAOMI adaptive optics telemetry data Open
Context. Monitoring turbulence parameters is crucial in high-angular resolution astronomy for various purposes, such as optimising adaptive optics systems or fringe trackers. The former systems are present at most modern observatories and …
View article: Proof-of-concept AO telemetry data using the AOT standard format
Proof-of-concept AO telemetry data using the AOT standard format Open
Dataset containing a demonstration of AO telemetry data using the AOT standard format. Contains data from 5 different systems (CIAO, ERIS, GALACSI, NAOMI and PAPYRUS). The data is as follows: 4 CIAO files "CIAO#_*.fits" where # indicates t…
View article: Proof-of-concept AO telemetry data using the AOT standard format
Proof-of-concept AO telemetry data using the AOT standard format Open
Dataset containing a demonstration of AO telemetry data using the AOT standard format. Contains data from 5 different systems (CIAO, ERIS, GALACSI, NAOMI and PAPYRUS). The data is as follows: 4 CIAO files "CIAO#_*.fits" where # indicates t…
View article: Integrated turbulence parameters' estimation from NAOMI adaptive optics telemetry data
Integrated turbulence parameters' estimation from NAOMI adaptive optics telemetry data Open
Monitoring turbulence parameters is crucial in high-angular resolution astronomy for various purposes, such as optimising adaptive optics systems or fringe trackers. The former are present at most modern observatories and will remain signi…
View article: Towards virtual access of adaptive optics telemetry data
Towards virtual access of adaptive optics telemetry data Open
International audience
View article: Towards virtual access of adaptive optics telemetry data
Towards virtual access of adaptive optics telemetry data Open
Large amounts of Adaptive-Optics (AO) control loop data and telemetry are currently inaccessible to end-users. Broadening access to those data has the potential to change the AO landscape on many fronts, addressing several use-cases such a…