IOP4, the Interactive Optical Photo-Polarimetric Python Pipeline

dc.contributor.authorPedrosa, Juan Escudero
dc.contributor.authorAgudo, Ivan
dc.contributor.authorMorcuende, Daniel
dc.contributor.authorOtero-Santos, Jorge
dc.contributor.authorBonnoli, Giacomo
dc.contributor.authorPiirola, Vilppu
dc.contributor.authorHusillos, Cesar
dc.contributor.authorBernardos, Mabel
dc.contributor.authorLopez-Coto, Ruben
dc.contributor.authorSota, Alfredo
dc.contributor.authorCasanova, Victor
dc.contributor.authorAceituno, Fran J.
dc.contributor.authorSantos-Sanz, Pablo
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organizationfi=fysiikan ja tähtitieteen laitos|en=Department of Physics and Astronomy|
dc.contributor.organizationfi=matemaattis-luonnontieteellinen tiedekunta|en=Faculty of Science|
dc.contributor.organization-code1.2.246.10.2458963.20.36798383026
dc.converis.publication-id457447219
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/457447219
dc.date.accessioned2025-08-27T21:39:29Z
dc.date.available2025-08-27T21:39:29Z
dc.description.abstractIOP4 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 to seamlessly integrate all information about the reduction and results in a database that 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 that 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, DIPOL (at OSN 0.9 m telescope), AndorT150 (OSN 1.5 m telescope), and CAFOS (CAHA 2.2 m 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.
dc.identifier.eissn1538-3881
dc.identifier.jour-issn0004-6256
dc.identifier.olddbid200825
dc.identifier.oldhandle10024/183852
dc.identifier.urihttps://www.utupub.fi/handle/11111/47237
dc.identifier.urlhttps://iopscience.iop.org/article/10.3847/1538-3881/ad5a80
dc.identifier.urnURN:NBN:fi-fe2025082785141
dc.language.isoen
dc.okm.affiliatedauthorPiirola, Vilppu
dc.okm.affiliatedauthorDataimport, Tuorlan observatorio
dc.okm.affiliatedauthorDataimport, Fysiikan ja tähtitieteen laitoksen yhtei
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherIOP Publishing Ltd
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.publisher.placeBRISTOL
dc.relation.articlenumber84
dc.relation.doi10.3847/1538-3881/ad5a80
dc.relation.ispartofjournalThe Astronomical Journal
dc.relation.issue2
dc.relation.volume168
dc.source.identifierhttps://www.utupub.fi/handle/10024/183852
dc.titleIOP4, the Interactive Optical Photo-Polarimetric Python Pipeline
dc.year.issued2024

Tiedostot

Näytetään 1 - 1 / 1
Ladataan...
Name:
Escudero_Pedrosa_2024_AJ_168_84.pdf
Size:
1.62 MB
Format:
Adobe Portable Document Format