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dc.contributor.authorFitzgerald, K.
dc.contributor.authorBrowne, Lisa-Marie
dc.contributor.authorButler, Ray F.
dc.date.accessioned2019-08-22T08:55:51Z
dc.date.issued2019-05-11
dc.identifier.citationFitzgerald, K., Browne, L. M., & Butler, R. F. (2019). Using the Agile software development lifecycle to develop a standalone application for generating colour magnitude diagrams. Astronomy and Computing, 28, 100283. doi: https://doi.org/10.1016/j.ascom.2019.05.001en_IE
dc.identifier.issn2213-1337
dc.identifier.urihttp://hdl.handle.net/10379/15341
dc.description.abstractVirtual observatories allow the means by which an astronomer is able to discover, access, and process data seamlessly, regardless of its physical location. However, steep learning curves are often required to become proficient in the software employed to access, analyse and visualise this trove of data. It would be desirable, for both research and educational purposes, to have applications which allow users to visualise data at the click of a button. Therefore, we have developed a standalone application (written in Python) for plotting photometric Colour Magnitude Diagrams (CMDs) — one of the most widely used tools for studying and teaching about astronomical populations. The CMD Plot Tool application functions “out of the box” without the need for the user to install code interpreters, additional libraries and modules, or to modify system paths; and it is available on multiple platforms. Interacting via a graphical user interface (GUI), users can quickly and easily generate high quality plots, annotated and labelled as desired, from various data sources. This paper describes how CMD Plot Tool was developed using Object Orientated Programming and a formal software design lifecycle (SDLC). We highlight the need for the astronomical software development culture to identify appropriate programming paradigms and SDLCs. We outline the functionality and uses of CMD Plot Tool, with examples of star cluster photometry. All results plots were created using CMD Plot Tool on data readily available from various online virtual observatories, or acquired from observations and reduced with IRAF/PyRAF.en_IE
dc.description.sponsorshipThis work was supported by Athlone Institute of Technology, Ireland (K.F.) and National University of Ireland - Galway (L.-M.B.)en_IE
dc.formatapplication/pdfen_IE
dc.language.isoenen_IE
dc.publisherElsevieren_IE
dc.relation.ispartofAstronomy And Computingen
dc.subjectAgile software developmenten_IE
dc.subjectObject oriented developmenten_IE
dc.subjectScientific visualisationen_IE
dc.subjectHertzsprung–Russell diagramen_IE
dc.subjectGlobular clustersen_IE
dc.titleUsing the Agile software development lifecycle to develop a standalone application for generating colour magnitude diagramsen_IE
dc.typeArticleen_IE
dc.date.updated2019-08-22T08:44:46Z
dc.identifier.doi10.1016/j.ascom.2019.05.001
dc.local.publishedsourcehttps://doi.org/10.1016/j.ascom.2019.05.001en_IE
dc.description.peer-reviewedpeer-reviewed
dc.description.embargo2021-05-11
dc.internal.rssid17348350
dc.local.contactRay Butler, School Of Physics, Arts/Science Building, Nui Galway. 3788 Email: ray.butler@nuigalway.ie
dc.local.copyrightcheckedYes
dc.local.versionACCEPTED
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