Cosmic Microwave Background at low frequencies
| dc.creator | Subrahmanyan, R. | |
| dc.date | 2000-03-15 | |
| dc.date.accessioned | 2026-07-07T01:52:45Z | |
| dc.date.available | 2026-07-07T01:52:45Z | |
| dc.description | The next generation low-frequency radio telescopes may probe cosmological models by means of observations of the cosmic microwave background (CMB). I discuss the prospects for observations of CMB imprints - recombination lines from the epoch of recombination, μdistortions and angular temperature anisotropies - at low frequencies. A future low-frequency radio telescope, like the proposed SKA, may be capable of attempting some difficult CMB measurements because of the large collecting area and large element numbers; however, this will require a telescope design that will allow specialized calibration strategies and will give emphasis to the control of spurious responses. | |
| dc.description | 8 pages, includes 1 figure, to appear in The Universe at Low Radio Frequencies, IAU Symp. 199, Pune, India, Dec. 1999 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0003227 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0003227 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/730 | |
| dc.subject | Astrophysics | |
| dc.title | Cosmic Microwave Background at low frequencies | |
| dc.type | text |