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Article: Faint UBVRI CCD sequences for wide-field surveys - II. UBVR sequences at Oδ = - 30°

TitleFaint UBVRI CCD sequences for wide-field surveys - II. UBVR sequences at Oδ = - 30°
Authors
KeywordsCatalogues
Techniques: photometric
Issue Date1999
Citation
Monthly Notices of the Royal Astronomical Society, 1999, v. 306, n. 3, p. 592-598 How to Cite?
AbstractWe present results from a continuing campaign to secure deep multi-colour CCD sequences for photometric calibration in UK Schmidt fields with galactic latitudes |b| > 50°. In this paper we present UBVR photometry in 12 fields and BR photometry in a further 14 fields observed within UK Schmidt survey fields centred at δ = - 30°. Photometric errors are at the 0.05 level at 20.2, 21, 20.5 and 20 mag for UBVR sequences respectively. Our observations were carried out with the 0.9-m telescope at the Cerro-Tololo Inter-American Observatory. These data are not intended for use as highly accurate individual photometric standards, but rather for use as sequences, using a large number of stars to calibrate wide-area data such as photographic plates. The data are available electronically at http:// icstar5.ph.ic.ac.uk/~scroom/phot/photom.html.
Persistent Identifierhttp://hdl.handle.net/10722/208820
ISSN
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DC FieldValueLanguage
dc.contributor.authorCroom, Scott M.-
dc.contributor.authorRatcliffe, Andrew-
dc.contributor.authorParker, Quentin A.-
dc.contributor.authorShanks, Tom-
dc.contributor.authorBoyle, Brian J.-
dc.contributor.authorSmith, Robert J E-
dc.date.accessioned2015-03-23T02:01:48Z-
dc.date.available2015-03-23T02:01:48Z-
dc.date.issued1999-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1999, v. 306, n. 3, p. 592-598-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/208820-
dc.description.abstractWe present results from a continuing campaign to secure deep multi-colour CCD sequences for photometric calibration in UK Schmidt fields with galactic latitudes |b| > 50°. In this paper we present UBVR photometry in 12 fields and BR photometry in a further 14 fields observed within UK Schmidt survey fields centred at δ = - 30°. Photometric errors are at the 0.05 level at 20.2, 21, 20.5 and 20 mag for UBVR sequences respectively. Our observations were carried out with the 0.9-m telescope at the Cerro-Tololo Inter-American Observatory. These data are not intended for use as highly accurate individual photometric standards, but rather for use as sequences, using a large number of stars to calibrate wide-area data such as photographic plates. The data are available electronically at http:// icstar5.ph.ic.ac.uk/~scroom/phot/photom.html.-
dc.languageeng-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.subjectCatalogues-
dc.subjectTechniques: photometric-
dc.titleFaint UBVRI CCD sequences for wide-field surveys - II. UBVR sequences at Oδ = - 30°-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.scopuseid_2-s2.0-0039596814-
dc.identifier.volume306-
dc.identifier.issue3-
dc.identifier.spage592-
dc.identifier.epage598-

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