Multicolour observations, inhomogeneity and evolution
dc.contributor.author | Hellaby, Charles | |
dc.date.accessioned | 2021-10-08T11:00:59Z | |
dc.date.available | 2021-10-08T11:00:59Z | |
dc.date.issued | 2001 | |
dc.description.abstract | We propose a method of testing source evolution theories that is independent of the effects of inhomogeneity, and thus complementary to other studies of evolution. It is suitable for large scale sky surveys, and the new generation of large telescopes. In an earlier paper it was shown that basic cosmological observations -luminosity versus redshift, area distance versus redshift and number counts versus redshift -cannot separate the effects of cosmic inhomogeneity, cosmic evolution and source evolution. We here investigate multicolour observations, and show that by comparing luminosity versus redshift in two or more colours, contraints can be placed on source evolution even if unknown source evolution is present, providing an important test of evolution theories that is complementary to present methods. However, number counts in different colours versus redshift are not useful in separating the effects of source evolution and inhomogeneity. | |
dc.identifier.apacitation | Hellaby, C. (2001). Multicolour observations, inhomogeneity and evolution. <i>Astronomy and Astrophysics</i>, 372(2), 357 - 363. http://hdl.handle.net/11427/35060 | en_ZA |
dc.identifier.chicagocitation | Hellaby, Charles "Multicolour observations, inhomogeneity and evolution." <i>Astronomy and Astrophysics</i> 372, 2. (2001): 357 - 363. http://hdl.handle.net/11427/35060 | en_ZA |
dc.identifier.citation | Hellaby, C. 2001. Multicolour observations, inhomogeneity and evolution. <i>Astronomy and Astrophysics.</i> 372(2):357 - 363. http://hdl.handle.net/11427/35060 | en_ZA |
dc.identifier.issn | 0004-6361 | |
dc.identifier.issn | 1432-0746 | |
dc.identifier.ris | TY - Journal Article AU - Hellaby, Charles AB - We propose a method of testing source evolution theories that is independent of the effects of inhomogeneity, and thus complementary to other studies of evolution. It is suitable for large scale sky surveys, and the new generation of large telescopes. In an earlier paper it was shown that basic cosmological observations -luminosity versus redshift, area distance versus redshift and number counts versus redshift -cannot separate the effects of cosmic inhomogeneity, cosmic evolution and source evolution. We here investigate multicolour observations, and show that by comparing luminosity versus redshift in two or more colours, contraints can be placed on source evolution even if unknown source evolution is present, providing an important test of evolution theories that is complementary to present methods. However, number counts in different colours versus redshift are not useful in separating the effects of source evolution and inhomogeneity. DA - 2001 DB - OpenUCT DP - University of Cape Town IS - 2 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2001 SM - 0004-6361 SM - 1432-0746 T1 - Multicolour observations, inhomogeneity and evolution TI - Multicolour observations, inhomogeneity and evolution UR - http://hdl.handle.net/11427/35060 ER - | en_ZA |
dc.identifier.uri | http://hdl.handle.net/11427/35060 | |
dc.identifier.vancouvercitation | Hellaby C. Multicolour observations, inhomogeneity and evolution. Astronomy and Astrophysics. 2001;372(2):357 - 363. http://hdl.handle.net/11427/35060. | en_ZA |
dc.language.iso | eng | |
dc.publisher.department | Department of Mathematics and Applied Mathematics | |
dc.publisher.faculty | Faculty of Science | |
dc.source | Astronomy and Astrophysics | |
dc.source.journalissue | 2 | |
dc.source.journalvolume | 372 | |
dc.source.pagination | 357 - 363 | |
dc.source.uri | https://dx.doi.org/10.1051/0004-6361:20010172 | |
dc.subject.other | Astrophysics | |
dc.subject.other | General Relativity and Quantum Cosmology | |
dc.title | Multicolour observations, inhomogeneity and evolution | |
dc.type | Journal Article | |
uct.type.publication | Research | |
uct.type.resource | Journal Article |
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