The results from this routine are labelled position lists (one for each input list) which may be used to complete image registration using the REGISTER routine. The estimated offsets are reported, but REGISTER should be used to get accurate values.
If NDFNAMES is FALSE then the actual names of the position
lists should be given. These may not use wildcards but may be
specified using indirection (other CCDPACK position list
processing routines will write the names of their results file
into files suitable for use in this manner) the indirection
character is "
".
If the logging system has been initialised using CCDSETUP then the value specified there will be used. Otherwise, the default is "CCDPACK.LOG". [CCDPACK.LOG]
If a global value for this parameter has been set using CCDSETUP then that value will be used. [TRUE]
OUTLIST > *.findIf no image names are given (NDFNAMES is FALSE) then if you want to change the extension of the files (from ".find" to ".off" in this case) use:
OUTLIST > *|find|off|Or alternatively you can use an explicit list of names. These may use indirection elements as well as names separated by commas.
If the associating position lists with NDFs option has been chosen, an position list will still be written for each input NDF, but for NDFs which were not matched the output list will be empty (will consist only of comment lines).
Incomplete matching would ideally indicate that one, or more, of the input lists are from positions not coincident with the others, in which case it is perfectly legimate to proceed. However, it is equally possible that they have too few positions and have consequently been rejected. [TRUE]
This parameter should therefore be set TRUE if the frames are quite well aligned in their Current coordinate systems (especially in the case that there are many objects and a small overlap), and FALSE if they are not.
This parameter is ignored if USEWCS is FALSE. [FALSE]
If USESET is false, all Set header information is ignored. If NDFNAMES is false, USESET will be ignored. If the input images have no Set headers, or if they have no CCD_SET frame in their WCS components, the setting of USESET will make no difference.
If a global value for this parameter has been set using CCDSETUP then that value will be used. [FALSE]
This parameter is ignored if NDFNAMES is false. [TRUE]
CCDPACK format - the first three columns are interpreted as the following.
EXTERNAL format - positions are specified using just an X and a Y entry and no other entries.
In all cases, the coordinates in position lists are pixel coordinates.
Comments may be included in a file using the characters "#" and "!". Columns may be separated by the use of commas or spaces.
Which algorithm you should use depends on the number of points your position lists contain and the expected size of the overlaps between the datasets. Obviously it is much easier to detect two lists with most of their positions in common. With small overlaps a serious concern is the likelihood of finding a `false' match. False matches must be more likely the larger the datasets and the smaller the overlap.
The first algorithm (referred to as SLOW) is more careful and is capable of selecting out positions when small overlaps in the data are present (although a level of false detections will always be present) but the process is inherently slow (scaling as n**3log2(n)). The second algorithm (referred to as FAST) is an n*n process so is much quicker, but requires much better overlapping.
Because the FAST process takes so little CPU time it is better to try this first (without the SLOW process as a backup), only use the SLOW algorithm when you have small datasets and do not expect large areas (numbers of positions) of overlap.
A third algorithm, referred to as SNGL, is used automatically if one or both of the lists in a pair contains only a single object. In this case object matching is trivial and, of course, may easily be in error. SNGL can only be used if the MINMATCH parameter has been set to 1, which should be done with care. The SNGL algorithm may be useful if there really is only one object, correctly identified, in all the frames. If this is not the case, it should only be used when USEWCS is true and MAXDISP is set to a low value, indicating that the alignment of the images in their Current coordinate systems is already fairly accurate.
The global registration process works by forming a graph with each position list at a node and with connecting edges of weight the number of matched position-pairs. The edge weights may be modified by a completeness factor which attempts to assess the quality of the match (this is based on the ratio of the expected number of matches in the overlap region to the actual number, random matches shouldn't return good statistics when compared with genuine ones). This still leaves a possibility of false matches disrupting any attempt to register the datasets so a single "spanning tree" is chosen (this is a graph which just visits each node the minimum number of times required to get complete connectivity, no loops allowed) which has the highest possible number of matched positions (rejecting edges with few matched positions/low completenesses where possible). This gives a most likely solution to the offsets between the position lists, rather than the "best" solution which could well include false matches; compare this solution with a median as opposed to a mean. The final registration is then used to identify all the objects which are the same in all datasets (using a relaxation method), resulting in labelled position lists which are output for use by REGISTER.
Retaining parameter values has the advantage of allowing you to define the default behaviour of the application but does mean that additional care needs to be taken when re-using the application after a break of sometime. The intrinsic default behaviour of the application may be restored by using the RESET keyword on the command line.
Certain parameters (LOGTO, LOGFILE, NDFNAMES and USESET) have global values. These global values will always take precedence, except when an assignment is made on the command line. Global values may be set and reset using the CCDSETUP and CCDCLEAR commands.
CCDPACK