* Export LSST_LIBRARY_PATH.
* Rewrite shebang lines on files in bin.src.

LSST does not persist an icMatchFull equivalent, so we need to construct this
on the fly based on the source and match records.

If MosaicTask runs with doSolveWcs=False, it does not write a new Wcs. It
should still be possible to apply the flux correction in this case.

This is required by the LSST implementation of PerTractCcdDataIdContainer.

If MosaicTask runs with doSolveFlux=False, it does not write a new flux
correction. It should still be possible to apply the new Wcs in this case.

This is necessary following the merger of DM-4683.

The new (post-DM-4692) ProcessCcdTask uses the src catalog to perform
astrometry and photometry (as opposed to icSrc). It also no longer saves
icMatch, or attaches positional information to icSrcs.

Here, we switch to using src in meas_mosaic.

This is in response to DM-4036, DM-5879 and DM-6095.

Includes:

Migration to std::shared_ptr, including:
- boost::shared_ptr -> std::shared_ptr
- boost::weak_ptr -> std::weak_ptr
- boost::static_pointer_cast -> std::static_pointer_cast
- boost::dynamic_pointer_cast -> std::dynamic_pointer_cast
- boost::const_pointer_cast -> std::const_pointer_cast
- boost::reinterpret_pointer_cast -> std::reinterpret_pointer_cast
- boost::enamble_shared_from_this -> std::enable_shared_from_this
- boost pointer related includes -> standard library memory
Replace boost::math.
Replace boost::ref.

This is useful for debugging.

Also adds the appropriate fluxSigma key and field from which
meas_mosaic extracts it.  This error has been propogated
according to the colorterm correction.

- Add labels and column headers.
- Tweak diagnostic plots to include handling of CCD subsets, and labels and column headers.

If the detector has nQuarter%4 != 0 (i.e. it is rotated w.r.t the focal
plane coordinate system), the (x, y) pixel values of the centroid slot for
the source catalogs need to be rotated such that pixel (0, 0) corresponds
to the LLC (i.e. the coordinate system expected by meas_mosaic).

For the oddly rotated CCDs, the width and height values must be
swapped when setting the bounding box for the spacial cell search.
They also need to be swapped when drawing the CCD outlines on the
diagnostic focal plane plots.

The HSC team is currently using a fork of the main LSST stack.  Many
developements have occurred on this fork for the purpose of HSC SSP
data release production runs.  What is currently the "HSC stack" will
eventually become obsolete, once all new development that happened
there is ported over to the LSST stack and validated.  For this
validation, it is useful to be able to directly LSST vs. HSC stack
runs when using the exact same inputs.  This is implemented here by
including accommodations required to parse HSC stack produced outputs,
namely a mapper between the different source schemas.  See the
readSrc() function in SourceReader class in MosaicTask.py along with
the config/hsc/Mosaic.py file in obs_subaru for an example of how to
apply this mapper.  The mapper itself is in config/hsc/srcSchemaMap.py
in obs_subaru.

Note that these inputs will already be in the coordinate system that
meas_mosaic expects (i.e. all CCDs have LLC pixel (0, 0) w.r.t the
focal plane coordinate system), so no accommodations need to be made
in that respect.

Certain objects are not good candidates for inclusion in the mosaic
fit.  Here we add optional selection criteria as config parameters
to exclude objects based on values in the schema.  The following lists
the config parameters.  If they are set to any valid key name, the
behavior indicated is followed:

extendednessForStarSelection: only include point-like sources
saturatedForStarSelection: do not include saturated sources (unless
                           includeSaturated is True)
psfStarForStarSelection: only include objects used in the PSF determination
                         *unless* extendednessForStarSelection, in which case
                         include all point-like sources
calibStarForStarSelection: only include objects detected as calibration sources
parentForStarSelection: do not include objects with parents
nChildForStarSelection: do not include objects with children

To exclude any given criterion, set its corresponding config value to an
invalid value (e.g. None).

The matrix solvers will be operating on non-invertible matrices
when input is sparse (e.g. operating on a limited number of inputs).
Use full pivoting when using Eigen for a more robust solution.

N.B. This may not be the optimal solution.  Will revisit if it is
deemed necessary.

HSC is using Eigen, so while we are comparing between stacks, keep
this consistent by disabling MKL on LSST stack for now.

These include the various diagnostic plotting and data output
functions, functions accommodating HSC stack run analysis, and
those used to rotate catalog pixel coordinate to accommodate the
coordinate system expected by meas_mosaic (i.e. the LLC of any
CCD as placed in the focal plane is pixel 0, 0).

Updates the application of the results to a catalog.  Since meas_mosaic's
solution is based on a coordinate system where a given detector's origin
(pixel 0, 0) is associated with its LLC w.r.t. to the focal plane.  LSST
always associates the detector origin with the electronics, thus if the
detector was rotated when inserted into the focal plane (nQuarter%4 != 0),
the centroids must be rotated to the meas_mosaic coordinate system before
applying the corrections.

Note that if working with catalogs produced by the HSC stack (hscRun is
not None), the pixels are already in the correct coordinate system, so
no rotations are necessary.