IOP4, the Interactive Optical Photo-Polarimetric Python Pipeline
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866929366325264384 |
|---|---|
| author | Pedrosa, Juan Escudero Agudo, Ivan Morcuende, Daniel Otero-Santos, Jorge Bonnoli, Giacomo Piirola, Vilppu Husillos, César Bernardos, Mabel López-Coto, Rubén Sota, Alfredo Casanova, Víctor Aceituno, Francisco Santos-Sanz, Pablo |
| author_facet | Pedrosa, Juan Escudero Agudo, Ivan Morcuende, Daniel Otero-Santos, Jorge Bonnoli, Giacomo Piirola, Vilppu Husillos, César Bernardos, Mabel López-Coto, Rubén Sota, Alfredo Casanova, Víctor Aceituno, Francisco Santos-Sanz, Pablo |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_20111 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | IOP4, the Interactive Optical Photo-Polarimetric Python Pipeline Pedrosa, Juan Escudero Agudo, Ivan Morcuende, Daniel Otero-Santos, Jorge Bonnoli, Giacomo Piirola, Vilppu Husillos, César Bernardos, Mabel López-Coto, Rubén Sota, Alfredo Casanova, Víctor Aceituno, Francisco Santos-Sanz, Pablo Instrumentation and Methods for Astrophysics 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. |
| title | IOP4, the Interactive Optical Photo-Polarimetric Python Pipeline |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2405.20111 |