JSkyMap is a visibility simulation and map reconstruction software package for interferometers operating in transit mode. It can be used to compute simulated visibilities starting from sky maps for dish or cylinder arrays, operating in transit mode. It has been developed to perform map reconstruction from cleaned/calibrated visibilities. It provides full sky map making in spherical geometry using the m-mode decomposition, or in rectangular geometry. The package has been written in C++, with parallel, multi-thread capability, over a single node, with mutiple CPU’s or cores. Most operations are performed on a single frequency, meaning that data from different frequencies can be handled in parallel on different nodes.
The code itself is rather compact and simple, built around few classes, but relies on the SOPHYA class library for many services, including various numerical algorithms as well as I/O , in native SOPHYA format, FITS and HDF5. The SOPHYA support class library can be downloaded from this sophya-git.
Package documentation generated using doxygen is available from JSKyMapDoxy
A list of the main classes in the JSkyMap package in given below:
- BeamTP : Single feed beam response or antenna lobe in angular domain
- BeamVis : beam response for a pair of feeds or antenna ( in angular domain)
- BeamLM : beam response in the (l,m) spherical harmonics plane
- SphCoordTrans : Spherical coordinate transformation
- JSphSkyMap : the top level class providing the visibility computation and map making in spherical geometry, through m-mode decomposition
- InterferoArraySetup : Interferometer geometrical description
- PseudoInverse : template class which provides specific matrix operations such as the pseudo-inverse computation
- QuickMapMaker : Class implementing a simple and very fast map making for transit visibilities, through combinations of observed visibilities from all baselines, at fixed RA
- BFMTV_RectangularMap : Brute Force map making in rectangular geometry
- BFMTV_SphericalMap : Brute Force map making in spherical geometry
The package contains a number of main executable programs which can be used to compute simulated visibilities, or map from visibilities. An incomplete list of the most useful programs is given below:
- p4src2vis : Compute visibilities, as Time Ordered Data from a source list, an interferometer setup. Computation is performed in angular domain. check p4src2vis page for more info.
- src2tfm: Computes a set of (ra-frequency) visibilities maps from a list of sources and interferometer setup (computation in angular domain)
- map2vis : Computes visibilities from an input sky map using m-mode decomposition. Check map2vis page for more info.
- vis2map : Computes a spherical map from a set of visibilities through m-mode decomposition. Check vis2map page for more info.
- vis2qmap : Computes a map from set of visibilities using QuickMap or BFMTV (Brute Force Map making)
- filt2map : Computes a filtered spherical map from an input map, or from spherical harmonics coefficients, after applying a filter, mostly low-pass in (l,m) space. check filt2map page for more info.