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Conference Paper: Objective Prism Galaxy Redshifts in Fields around the South Galactic Pole
| Title | Objective Prism Galaxy Redshifts in Fields around the South Galactic Pole |
|---|---|
| Authors | |
| Editors | Editor(s):Capaccioli, M |
| Issue Date | 1984 |
| Publisher | D. Reidel Publishing Co. |
| Citation | Astronomy with Schmidt-type Telescopes: Proceedings of the 78th. Colloquium of the International Astronomical Union, Asiago, Italy, 30 August-2 September 1983, p. 405-405 How to Cite? |
| Abstract | Measurements made with the COSMOS machine on deep objective-prism photographs taken with the UK 1.2 m Schmidt Telescope are being used to obtain approximate redshifts (accurate to ≡0.01 in z) for large numbers of galaxies in fields near the South Galactic Pole. The data are suitable for investigations of the distribution of galaxies, such as the detection of large-scale density enhancements or voids. |
| Persistent Identifier | http://hdl.handle.net/10722/211237 |
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Parker, QA | - |
| dc.contributor.author | MacGillivray, HT | - |
| dc.contributor.author | Dodd, RJ | - |
| dc.contributor.author | Cooke, JA | - |
| dc.contributor.author | Beard, SM | - |
| dc.contributor.author | Kelly, BD | - |
| dc.contributor.author | Emerson, D | - |
| dc.contributor.editor | Capaccioli, M | - |
| dc.date.accessioned | 2015-07-08T03:23:30Z | - |
| dc.date.available | 2015-07-08T03:23:30Z | - |
| dc.date.issued | 1984 | - |
| dc.identifier.citation | Astronomy with Schmidt-type Telescopes: Proceedings of the 78th. Colloquium of the International Astronomical Union, Asiago, Italy, 30 August-2 September 1983, p. 405-405 | - |
| dc.identifier.uri | http://hdl.handle.net/10722/211237 | - |
| dc.description.abstract | Measurements made with the COSMOS machine on deep objective-prism photographs taken with the UK 1.2 m Schmidt Telescope are being used to obtain approximate redshifts (accurate to ≡0.01 in z) for large numbers of galaxies in fields near the South Galactic Pole. The data are suitable for investigations of the distribution of galaxies, such as the detection of large-scale density enhancements or voids. | - |
| dc.language | eng | - |
| dc.publisher | D. Reidel Publishing Co. | - |
| dc.relation.ispartof | Astronomy with Schmidt-type Telescopes | - |
| dc.title | Objective Prism Galaxy Redshifts in Fields around the South Galactic Pole | - |
| dc.type | Conference_Paper | - |
| dc.identifier.email | Parker, QA: quentinp@hku.hk | - |
| dc.identifier.authority | Parker, QA=rp02017 | - |
| dc.identifier.volume | 110 | - |
| dc.identifier.spage | 405 | - |
| dc.identifier.epage | 405 | - |
| dc.publisher.place | Dordrecht, Holland; Boston | - |
