@prefix this: . @prefix sub: . @prefix np: . @prefix dct: . @prefix pav: . @prefix rdf: . @prefix owl: . @prefix rdfg: . @prefix dce: . @prefix xsd: . @prefix rdfs: . @prefix prov: . @prefix npx: . sub:Head { this: a np:Nanopublication; np:hasAssertion sub:assertion; np:hasProvenance sub:provenance; np:hasPublicationInfo sub:pubinfo . } sub:assertion { a . a ; "D3.1: Workflow Evolution, Sharing and Collaboration Initial Requirements" . a ; "Taverna 2.4" . a ; "HYPERLEDA. I. Identification and designation of galaxies" . a ; "D4.1: Workflow Integrity and Authenticity Maintenance Initial Requirements" . a ; "D2.1 Workflow Lifecycle Management Initial Requirements" . a ; "Virtual Observatory activities in the AMIGA group" . a ; "D1.2: Wf4Ever Sandbox v1" . a ; "Python" . a ; "Topcat" . a ; "Capabilities of the HYPERLEDA database" . a ; "from. to. forSb galaxy" . a ; "logr25" . a ; "tool session" . a ; "Oxford University" . a ; "Lawrence" . a ; "property error value" . a ; "Amiga data revision" . a ; "mathematics" . a ; "United Kingdom" . a ; "astronomy" . a ; "Verley" . a ; "AMIGAsample" . a ; "Poznan" . a ; "Poland" . a ; "Oxford" . a ; "appendix B research object structure" . a ; "Madrid" . a ; "NamesLEDA.txt" . a ; "Leiden" . a ; "Hereafter" . a ; "Edinburgh" . a ; "axis ratio" . a ; "dust extinction coefficient" . a ; "deployment of a Research Object" . a ; "cig SDSS sample" . a ; "Colorado" . a ; "physics" . a ; "lumi nous galaxy" . a ; "Karachentseva" . a ; "HyperLEDA database" . a ; "Netherlands" . a ; "Calzetti" . a ; "statistics" . a ; "galaxy" . a ; "database" . a ; "research" . a ; "data" . a ; "sample" . a ; "red shift" . a ; "text file" . a ; "AMIGA" . a ; "FP ICT" . a ; "workflow" . a ; "value" . a ; "correction" . a ; "opticalAGN" . a ; "ratio" . a ; "information and communication technologies" . a ; "value" . a ; "optical luminosity in B-band" . a ; "luminosity" . a ; "e mail address" . a ; "CIG" . a ; "output" . a ; "Enrique Ruiz Minor" . a ; "Red Cross" . a ; "interactions galaxy" . a ; "University of Manchester" . a ; "Naciones" . a ; "evolution galaxy" . a ; "property" . a ; "mag" . a ; "research object management" . a ; "university" . a ; "inAMIGA" . a ; "Granada" . a ; "Alaska" . a ; "Manchester" . a ; "property value" . a ; "group database" . a ; "Vulkan Shmidta" . a ; "León" . a ; "colors" . a ; "SDSS" . a ; "workflow building" . a ; "sample" . a ; "type" . a ; "coordinate" . a ; "propagation" . a ; "Montenegro" . a ; "appendices" . a ; "database" . a ; "property" . a ; "value error" . a ; "calculation" . a ; "galaxy inclination" . a ; "galaxies", "galaxy" . a ; "galaxy" . a ; "sample" . a ; "sc galaxy" . a ; "type galaxies inAMIGA" . a ; "Boadilla del Monte" . a ; "propagation of property" . a ; "assigned galaxy type" . a ; "British Telecom" . a ; "evolution galaxy" . a ; "error of the coordinate" . a ; "AKwas" . a ; "Ai AK" . a ; "AGN" . a ; "IAA" . a ; "Pozna" . a ; "Mpc" . a ; "Sect." . a ; "Spain" . a ; "Golden Exemplar" . a ; "service-account-enrichment" . a , , ; pav:importedBy ; "http://sandbox.rohub.org/rodl/ROs/Pack585/"; "2014-01-27T17:30:51.771+01:00"; "https://www.google.com/accounts/o8/id?id=AItOawnZHKwZJglv16YBiUjsWEnx39mHA0RB250"; ; "2908816"^^xsd:integer; "https://api.rohub.org/api/ros/12f54724-cd7f-4410-b788-3c062fc644f7/crate/download/"; ; "2014-01-24 15:04:31.757000+00:00"; "2025-03-05 01:16:58.921026+00:00"; "2014-01-24 15:04:31.757000+00:00"; """The scientific experiment represented by this research object pertains to the multi-wavelength study for a sample of the most isolated galaxies in the local universe. This study characterizes each galaxy of this sample through both the measurement of basic astrophysical properties:  - The equatorial coordinates in J2000 epoch - The velocities in km/s (v) - The dust extinction coefficient (ag) - The axis ratio of the isophote 25 mag/arcsec2 (logr25) - The apparent total B magnitude (BT) - The morphological type (t) and the calculation of the more complex properties: - The distance in Mega parsecs (D) - The corrected apparent B magnitude (btc) - The optical luminosity in B-band (LB) Specifically, this research object is focused on the calculation of the intrinsic luminosity in the Johnson B-band, in order to achieve it the measurement or calculation of all those astrophysical properties is needed. All the data involved in the characterization of the sample are stored in a local relational MySQL database. To maintain up to date this database and to register all the updates properly is part of this scientific experiment."""; "application/ld+json"; ; "https://w3id.org/ro-id/12f54724-cd7f-4410-b788-3c062fc644f7"; ; "Propagation of properties extracted from the HyperLEDA catalog in the calculation of luminosities of galaxies"; rdfs:comment "Design Sketch and Experiment hypothesis will improve readability. Consider adding these elements.", "Please, take into account Hubble constant value in the determination of distances", "The Hubble constant value has been considered in the script calculateDistance.py"; "Jose Enrique Ruiz. \"Propagation of properties extracted from the HyperLEDA catalog in the calculation of luminosities of galaxies.\" ROHub. 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