Cosmological number density in depth from V/Vm distribution
| dc.creator | Banhatti, Dilip G. | |
| dc.date | 2009-03-13 | |
| dc.date.accessioned | 2026-07-07T12:52:26Z | |
| dc.date.available | 2026-07-07T12:52:26Z | |
| dc.description | Using distribution p(V/Vm) of V/Vm rather than just mean <V/Vm> in V/Vm-test leads directly to cosmological number density n(z). Calculation of n(z) from p(V/Vm) is illustrated using best sample (of 76 quasars) available in 1981, when method was developed. This is only illustrative, sample being too small for any meaningful results. Keywords: V/Vm . luminosity volume . cosmological number density . V/Vm distribution | |
| dc.description | 3 pages, 3 tables, briefer version for Proceedings of 27th Meeting of Astronomical Society of India, Indian Institute of Astrophysics, Bangaluru, 18-20th February, 2009 | |
| dc.identifier | https://arxiv.org/abs/0903.2442 | |
| dc.identifier | http://arxiv.org/abs/0903.2442 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/223296 | |
| dc.subject | Cosmology and Nongalactic Astrophysics | |
| dc.subject | Instrumentation and Methods for Astrophysics | |
| dc.title | Cosmological number density in depth from V/Vm distribution | |
| dc.type | text |