Imagine you are in charge of a project on-line archive and you want to integrate it in the VO framework.
Depending of the nature of your data (images, spectra, cubes, timeseries, catalogs) and on the completeness you want to reach the choice of protocols to implement will be different.
The talk will make a review of the various possibilities according to various examples.
In the context of Open Science, data provenance has become a key piece of information to be provided with astronomical data. It is particularly essential to ensure trust in the data, thus promoting its reuse. As such, provenance is explicitly mentioned in the FAIR principles, which aim to make research data Findable, Accessible, Interoperable and Reusable. In practice, provenance should come...
We would like to present an overview of the Common Archive Observation Model (CAOM), a general purpose data structure for use as the core data model of an astronomical data centre, designed by the Canadian Astronomy Data Centre (CADC). This common model is being used at the ESAC Science Data Centre (ESDC) in the contexts of the European Hubble and James Webb Space Telescopes Science Archives....
Yafits (Yet Another FITS viewer) is a standalone web application that enables remote visualisation of 3D data cubes hosted in FITS format on the server-side. The client can display images and spectra in order to quick-look the scientific content of the observations. The prime use is for radio-astronomy data, ie the ones from ALMA, IRAM/NOEMA or SKA but any kind of 2D or 3D FITS could be...
We present the MASER (Measurement, Analysis, and Simulation of Emissions in the Radio range) toolbox, which enables science ready access to low frequency radio astronomy data. MASER focuses on time-domain and dynamic spectra data products and associated tools. Being at the interface between astronomy, heliophysics and planetary sciences, we make use of interoperable standards from each world...
The Centro de Estudios de Física del Cosmos de Aragón (CEFCA) is carrying out from the Observatorio Astrofísico de Javalambre (OAJ, Teruel, Spain) two large area multiband photometric sky surveys, J-PLUS and J-PAS, covering the entire optical spectrum using narrow and broad band filters. J-PAS and J-PLUS include coadded and individual frame images, dual and single catalogue data which include...
Progress in publishing the e-MERLIN archive, and the role of this work as a precursor to SKA Regional Centre development will be described.
In the context of Open Science, data provenance has become a key piece of information to be provided with astronomical data. It is particularly essential to ensure trust in the data, thus promoting its reuse. As such, provenance is explicitly mentioned in the FAIR principles, which aim to make research data Findable, Accessible, Interoperable and Reusable. In practice, provenance should come...
Coronal holes (CH) are seen as dark features on EUV images of the Sun. They are the source of the fast solar wind, and as such are closely monitored. The CH feature recognition module named SPoCA-CH was developped at the Royal Observatory of Belgium. Since 2010, one version of this software is running at LMSAL and provides near-real time detection of coronal holes. We would like to provide the...
