English

IOP4, the Interactive Optical Photo-Polarimetric Python Pipeline

Instrumentation and Methods for Astrophysics 2024-05-31 v1

Abstract

IOP4 is a pipeline to perform photometry and polarimetry analysis of optical data from Calar Alto (CAHA) and Sierra Nevada (OSN) observatories. IOP4 implements Object Relational Mapping (ORM) to seamlessly integrate all information about the reduction and results in a database which can be used to query and plot results, flag data and inspect the reduction process in an integrated fashion with the whole pipeline. It also ships with an already built-in web interface which can be used out of the box to browse the database and supervise all pipeline processes. It is built to ease debugging and inspection of data. Reduction from five different instruments are already implemented: RoperT90, AndorT90 and DIPOL (at OSN 0.9m telescope), AndorT150 (OSN 1.5m telescope) and CAFOS (CAHA 2.2m telescope). IOP4's modular design allows for easy integration of new observatories and instruments, and its results have already featured in several high-impact refereed publications. In this paper we describe the implementation and characteristics of IOP4.

Cite

@article{arxiv.2405.20111,
  title  = {IOP4, the Interactive Optical Photo-Polarimetric Python Pipeline},
  author = {Juan Escudero Pedrosa and Ivan Agudo and Daniel Morcuende and Jorge Otero-Santos and Giacomo Bonnoli and Vilppu Piirola and César Husillos and Mabel Bernardos and Rubén López-Coto and Alfredo Sota and Víctor Casanova and Francisco Aceituno and Pablo Santos-Sanz},
  journal= {arXiv preprint arXiv:2405.20111},
  year   = {2024}
}

Comments

Submitted April 23, 2024

R2 v1 2026-06-28T16:47:16.715Z