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Conference Paper: Surveys of Low Surface Brightness Galaxies with 4415 Films
Title | Surveys of Low Surface Brightness Galaxies with 4415 Films |
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Authors | |
Editors | Editor(s):MacGillivray, HT |
Issue Date | 1994 |
Publisher | Springer |
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? |
Abstract | During 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 Identifier | http://hdl.handle.net/10722/211222 |
ISBN | |
Series/Report no. | International Astronomical Union, Vol. 161 |
DC Field | Value | Language |
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dc.contributor.author | Phillipps, S | - |
dc.contributor.author | Parker, QA | - |
dc.contributor.editor | MacGillivray, HT | - |
dc.date.accessioned | 2015-07-08T03:23:17Z | - |
dc.date.available | 2015-07-08T03:23:17Z | - |
dc.date.issued | 1994 | - |
dc.identifier.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 | - |
dc.identifier.isbn | 9780792328797 | - |
dc.identifier.uri | http://hdl.handle.net/10722/211222 | - |
dc.description.abstract | During 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.language | eng | - |
dc.publisher | Springer | - |
dc.relation.ispartof | Astronomy from Wide-Field Imaging | - |
dc.relation.ispartofseries | International Astronomical Union, Vol. 161 | - |
dc.title | Surveys of Low Surface Brightness Galaxies with 4415 Films | - |
dc.type | Conference_Paper | - |
dc.identifier.email | Parker, QA: quentinp@hku.hk | - |
dc.identifier.authority | Parker, QA=rp02017 | - |
dc.identifier.doi | 10.1007/978-94-011-1146-1_114 | - |
dc.identifier.volume | 161 | - |
dc.identifier.spage | 541 | - |
dc.identifier.epage | 544 | - |
dc.publisher.place | Netherlands | - |