Calibration Pipeline for the CTAO Data Processing and Preservation System

Accurate calibration is essential for maximizing the scientific output of the Cherenkov Telescope Array Observatory (CTAO). The Calibration Pipeline, a core component of the Data Processing and Preservation System (DPPS), is part of the low-level offline reconstruction software. It is responsible for generating and maintaining high-precision calibration products. It encompasses the refinement of individual telescope calibrations, atmospheric corrections, and inter-telescope calibration, ensuring that CTAO data achieve the highest possible accuracy. The pipeline integrates multiple data sources, including telescope calibration events, array elements monitoring and service data, as well as atmospheric measurements from FRAM, LIDAR, and external meteorological data. Using advanced data analysis techniques, the pipeline derives calibration coefficients, corrects instrumental biases, and tracks long-term stability. The pipeline’s key components include: - Instrument Calibration: The pipeline analyzes calibration event data from individual telescopes to improve the in-situ calibrations performed during data taking, addressing uncertainties in baseline, gain, timing, and optical system precision and efficiency. - Atmospheric Calibration: A best-fitting atmospheric description model is derived from FRAM, LIDAR, and external meteorological data. This model is then used to select or generate the most appropriate simulations, ensuring accurate event reconstruction. - Inter- and Cross-Telescope Calibration: The pipeline compares air shower events observed by neighboring telescopes in the array, deducing the relative calibration coefficients of the telescopes. To enable seamless data processing, the Calibration Pipeline interfaces with other DPPS components, including the Workload Management System, Simulation, Data Reconstruction, and Data Quality Monitoring pipelines. This contribution presents the current status and development roadmap of the Calibration Pipeline, highlighting key advancements and future improvements. We discuss the challenges involved in implementing a scalable, automated, and high-precision calibration framework, as well as ongoing efforts to optimize its integration within the DPPS software package.

Authors

Institutions

Publication Details

Published
2025-09-23
DOI
https://doi.org/10.22323/1.501.0620
Primary Topic
Astronomical Observations and Instrumentation
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Calibration Pipeline for the CTAO Data Processing and Preservation System

Matteo Balbo, Georgios Gerasimos Voutsinas, T. Montaruli, Tjark Miener et al.
Astronomical Observations and Instrumentation
article

Calibration Pipeline for the CTAO Data Processing and Preservation System

Matteo Balbo, Georgios Gerasimos Voutsinas, T. Montaruli, Tjark Miener, M. Dalchenko
article en

Abstract

Accurate calibration is essential for maximizing the scientific output of the Cherenkov Telescope Array Observatory (CTAO). The Calibration Pipeline, a core component of the Data Processing and Preservation System (DPPS), is part of the low-level offline reconstruction software. It is responsible for generating and maintaining high-precision calibration products. It encompasses the refinement of individual telescope calibrations, atmospheric corrections, and inter-telescope calibration, ensuring that CTAO data achieve the highest possible accuracy. The pipeline integrates multiple data sources, including telescope calibration events, array elements monitoring and service data, as well as atmospheric measurements from FRAM, LIDAR, and external meteorological data. Using advanced data analysis techniques, the pipeline derives calibration coefficients, corrects instrumental biases, and tracks long-term stability. The pipeline’s key components include: - Instrument Calibration: The pipeline analyzes calibration event data from individual telescopes to improve the in-situ calibrations performed during data taking, addressing uncertainties in baseline, gain, timing, and optical system precision and efficiency. - Atmospheric Calibration: A best-fitting atmospheric description model is derived from FRAM, LIDAR, and external meteorological data. This model is then used to select or generate the most appropriate simulations, ensuring accurate event reconstruction. - Inter- and Cross-Telescope Calibration: The pipeline compares air shower events observed by neighboring telescopes in the array, deducing the relative calibration coefficients of the telescopes. To enable seamless data processing, the Calibration Pipeline interfaces with other DPPS components, including the Workload Management System, Simulation, Data Reconstruction, and Data Quality Monitoring pipelines. This contribution presents the current status and development roadmap of the Calibration Pipeline, highlighting key advancements and future improvements. We discuss the challenges involved in implementing a scalable, automated, and high-precision calibration framework, as well as ongoing efforts to optimize its integration within the DPPS software package.

University of Geneva (CH)
Openalex Percentile: Top 72%
Astronomical Observations and Instrumentation
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.