In all cases involving short spacings, the relative weight of the single
dish data to interferometer data is critical. Within the restrictions
imposed by the noise level, this relative weight is a free parameter. It is
all the more important that the Fourier transform of the uv plane
density of weights is the dirty beam, a key parameter of the deconvolution.
The general goal is to have a dirty beam as close as possible to a
Gaussian. As the Fourier transform of a Gaussian is a Gaussian, we search
for obtaining a uv plane density of weights as close as possible to a
Gaussian. In general, the short spacing frequencies are small compared to
the largest spatial frequency measured by an interferometer. This implies
we can use the linear approximation of a Gaussian, i.e. a constant, in the
range of frequencies used for the short spacing processing. We thus end up
with the need to match (as far as possible) the Single-Dish and
interferometric densities of weights in the uv plane. In practice, we
compute the density of weights from the single-dish in a uv circle of
radius 1.25d and we match it to the averaged density of weights from the
interferometer in a uv ring between 1.25 and 2.5d. Experience shows
that this gives the right order of magnitude for the relative weight and
that a large range of relative weight around this value gives very similar
final results.
When processing IRAM-30m data to combine to NOEMA data, this criterion
implies a large down-weighting of the IRAM-30m data which may make think
that too much observing time was used at the IRAM-30m data. However, just
using the above criterion to determine the observing time needed at the
IRAM-30m would in general lead to very low signal-to-noise ratio of the
single-dish map. In such a case, it is very difficult to detect problems
which would translate in strong artifacts in the IRAM-30m + NOEMA
combination. We recommend to ask for enough IRAM-30m time to get a
median signal-to-noise ratio of 5 on the single-dish map. This ratio
should be achieved for all velocity channels of interest (which may include
the line wings).
Next: Comparison
Up: Pseudo-visibility technique
Previous: General description
Contents
Index
Gildas manager
2023-06-01