Adaptive Optics Telemetry Standard: Design and specification of a novel data exchange format
arXiv:2312.08300 · doi:10.1051/0004-6361/202348486
Abstract
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 activities that involve large-scale telemetry mining, processing, and curation. This paper introduces the Adaptive Optics Telemetry (AOT) data exchange format as a standard for sharing AO telemetry from visible/infrared ground-based observatories. AOT is based on the Flexible Image Transport System (FITS) and aims to provide unambiguous and consistent data access across various systems and configurations, including natural and single/multiple laser guide-star AO systems. We designed AOT focused on two key use cases: atmospheric turbulence parameter estimation and point-spread function reconstruction (PSF-R). We prototyped and tested the design using existing AO telemetry datasets from multiple systems: single conjugate with natural and laser guide stars, tomographic systems with multi-channel wavefront sensors, single and multi wavefront correctors in systems featuring either a Shack-Hartmann or Pyramid as main wavefront sensors. The AOT file structure has been thoroughly defined, specifying data fields, descriptions, data types, units, and expected dimensions. To support this format, we have developed a Python package that enables data conversion, reading, writing and exploration of AOT files, which has been made publicly available and compatible with a general-purpose Python package manager. We demonstrate the flexibility of the AOT format by packaging data from five different instruments, installed on different telescopes.
References in corpus (13)
- Astropy: A Community Python Package for Astronomy
- First Light LBT AO Images of HR 8799 bcde at 1.65 and 3.3 Microns: New Discrepancies between Young Planets and Old Brown Dwarfs
- A Data Exchange Standard for Optical (Visible/IR) Interferometry
- Reconstruction of the ground-layer adaptive-optics point spread function for MUSE Wide Field Mode observations
- OIFITS 2: the 2nd version of the Data Exchange Standard for Optical (Visible/IR) Interferometry
- New algorithms for adaptive optics point-spread function reconstruction
- Estimation of atmospheric turbulence parameters from Shack-Hartmann wavefront sensor measurements
- PRIME: Psf Reconstruction and Identification for Multiple sources characterization Enhancement. Application to Keck NIRC2 imager
- Learning from FITS: Limitations in use in modern astronomical research
- The ERIS Adaptive Optics System
- Pushing Point spread function reconstruction to the next level. Application to SPHERE/ZIMPOL
- Once FITS, Always FITS? Astronomical Infrastructure in Transition
- Integrated turbulence parameters' estimation from NAOMI adaptive optics telemetry data