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dc.contributor.authorHudec , R.
dc.contributor.authorHudec , L.
dc.contributor.authorKlíma , M.
dc.date.accessioned2017-02-03T11:17:36Z
dc.date.available2017-02-03T11:17:36Z
dc.date.issued2012
dc.identifier.citationActa Polytechnica. 2012, vol. 52, no. 1.
dc.identifier.issn1210-2709 (print)
dc.identifier.issn1805-2363 (online)
dc.identifier.urihttp://hdl.handle.net/10467/66905
dc.description.abstractThe ultra-low dispersion spectroscopy to be applied in the ESA Gaia space observatory and the ground-based objective-prism plate surveys represent a similar type of astrophysical data. Although the dispersion in plate surveys is usually larger than in the Gaia blue and red photometers (BP/RP), the spectral resolutions differ by a factor of 2–3 only, since the resolution in ground-based spectra is seeing-limited. We argue that some of the algorithms developed for digitized objective-prism plates can also be applied for the Gaia spectra. At the same time, the plate results confirm the feasibility of observing strong emission lines with Gaia RP/BP.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherČeské vysoké učení technické v Prazecs
dc.publisherCzech Technical University in Pragueen
dc.relation.ispartofseriesActa Polytechnica
dc.relation.urihttps://ojs.cvut.cz/ojs/index.php/ap/article/view/1504
dc.rightsCreative Commons Attribution 4.0 International Licenseen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectastronomical spectroscopyen
dc.subjectlow dispersion spectroscopyen
dc.subjectslitless spectroscopyen
dc.subjectGaiaen
dc.titleUltra Low Dispersion Spectroscopy with Gaia and Astronomical Slitless Surveys
dc.typearticleen
dc.date.updated2017-02-03T11:17:36Z
dc.rights.accessopenAccess
dc.type.statusPeer-reviewed
dc.type.versionpublishedVersion


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Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License