File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Conference Paper: Surveys of Low Surface Brightness Galaxies with 4415 Films

TitleSurveys of Low Surface Brightness Galaxies with 4415 Films
Authors
Editors
Issue Date1994
PublisherSpringer
Citation
Astronomy from wide-field imaging: proceedings of the 161st Symposium of the International Astronomical Union, Potsdam, Germany, 23-27 August 1993, p. 541-544 How to Cite?
AbstractDuring the past few years there have been a number of surveys for low surface brightness galaxies (LSBGs). Searches using both photographic and CCD data have shown that LSBGs are actually very numerous (Impey, Bothun & Malin 1987; Irwin et al. 1990). However, they are seriously biased against in any random sky survey, and even in a cluster area there are inherent size and signal-to-noise problems. The number of objects we can detect are therefore limited in two ways.
Persistent Identifierhttp://hdl.handle.net/10722/211222
ISBN
Series/Report no.International Astronomical Union, Vol. 161

 

DC FieldValueLanguage
dc.contributor.authorPhillipps, S-
dc.contributor.authorParker, QA-
dc.contributor.editorMacGillivray, HT-
dc.date.accessioned2015-07-08T03:23:17Z-
dc.date.available2015-07-08T03:23:17Z-
dc.date.issued1994-
dc.identifier.citationAstronomy from wide-field imaging: proceedings of the 161st Symposium of the International Astronomical Union, Potsdam, Germany, 23-27 August 1993, p. 541-544-
dc.identifier.isbn9780792328797-
dc.identifier.urihttp://hdl.handle.net/10722/211222-
dc.description.abstractDuring the past few years there have been a number of surveys for low surface brightness galaxies (LSBGs). Searches using both photographic and CCD data have shown that LSBGs are actually very numerous (Impey, Bothun & Malin 1987; Irwin et al. 1990). However, they are seriously biased against in any random sky survey, and even in a cluster area there are inherent size and signal-to-noise problems. The number of objects we can detect are therefore limited in two ways.-
dc.languageeng-
dc.publisherSpringer-
dc.relation.ispartofAstronomy from Wide-Field Imaging-
dc.relation.ispartofseriesInternational Astronomical Union, Vol. 161-
dc.titleSurveys of Low Surface Brightness Galaxies with 4415 Films-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.doi10.1007/978-94-011-1146-1_114-
dc.identifier.volume161-
dc.identifier.spage541-
dc.identifier.epage544-
dc.publisher.placeNetherlands-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats