
The E-ELT Design Reference Mission:
S5_3: Giant-planet-mass objects in the Large Magellanic Cloud (PI: F. Comeron)
==============================================================================

Annalisa Calamida <acalamid@eso.org>, 02 June 2009


The data in this directory accompany the DRM report for the DRM
science case. Please see
http://www.eso.org/sci/facilities/eelt/science/drm/S5  
for details.


-- catalog_input.dat: the input catalog with X,Y-coordinates, J, H, Ks
magnitudes, and masses, adopted in the simulations for the case of 100
stars uniformly distributed in a circle of radius 1".

-- catalog100000_input.dat: the input catalog with X,Y-coordinates, J,
H, Ks magnitudes, and masses, adopted in the simulations for the case
of 10,000 stars uniformly distributed in a circle of radius 10".


-- uni/: this directory contains 3 sub-directories, J,H,K. Each of
these contains example input and output data for a specific band and
pixel scale for the simulations performed assuming a uniform
background:

- the input catalog (100 star case, .dat);

- a simulated image (.fits);

- a simulated image of the sky background (.fits);

- a file with the reconstructed Point-Spread Function (PSF) performed
  with DAOPHOTIV (.psf);

- a file with the result of the PSF-fitting photometry performed with
  ALLFRAME (.alf, contains star ID, X,Y, Magnitude, error, background,
  iteration at which the fit converged, CHI of the fit);

- an image after the stars have been subtracted by the PSF-fitting
  photometry performed with ALLFRAME (.j.fits);

- a median image of the set of images of that specific run (.fits);

- the output catalog with the recoverd magnitudes, errors, and CHI
  parameter (.tab)


-- var/: this directory contains 3 sub-directories, J,H,K. Each of
these contains example input and output data for a specific band and
pixel scale for the simulations performed assuming a variable
background. The files have the same nomenclature of the files in
directory uni/


For more details on the data reduction procedures see Section 3.2
of the report.

