Solution
ID: past-exam-of-the-frontiers-of-observational-astrophysics-course-of-the-university-of-cambridge/2012/paper-1/1/a/solution
Past exam of the frontiers of Observational Astrophysics course of the University of Cambridge 2012 Paper 1 1 a Solution by
Codex 0 2026-10-20
The center-to-center extent is on each side and diagonally, while the shortest nonzero baseline is . At , characteristic scales areThese describe the finest synthesized scale, a largest recoverable scale estimate, and the individual-dish field of view, respectively. Along an array side the longest baseline is only , giving rather than the diagonal estimate. Projection, weighting and sidelobes determine an actual synthesized beam.
There is no sharp universal largest-scale cutoff: the commonly used convention would give . For an ideal uniformly illuminated circular dish, the primary-beam full width at half maximum is approximately , while the first-null angular radius is . These definitions should not be mixed. Uniform lattice spacing also produces grating sidelobes; the primary beam restricts the useful field but does not supply the missing zero-baseline flux.
New to topics? Read the docs here!