Index of /ogle/ogle3/maps/gd

[ICO]NameLast modifiedSizeDescription
[PARENTDIR]Parent Directory  -  
[TXT]README2012-08-20 19:59 5.1K 
[TXT]fields.txt2012-08-20 19:57 1.2K 
[DIR]maps/2012-08-20 20:04 -  
[DIR]old/2012-08-20 20:03 -  
[ ]pap.pdf2011-01-03 13:14 16M 
[DIR]ref_images/2012-08-20 19:43 -  
This directory contains OGLE-III maps of 21 Galactic disk (Car, Cen, Mus)
fields observed during the OGLE-III phase of the OGLE survey. 

REMARK: This a NEW DATASET (Aug 20, 2012), corrected in V and V-I for
        calibration inaccuracy of very red objects (V-I>1.5) due to
        non-standard OGLE-III I-band filter passband, using data from
        OGLE-IV camera, as described in the paper by Szymanski et al.
        (2011), Acta Astron. 61, 83, section 3.2

The directory structure is as follows:

README              - this file
fields.txt          - equatorial and galactic coordinates and number of objects
                      found in the OGLE-III GD fields.
pap.pdf             - PDF version of the paper Szymanski et al.(2010),
                      Acta Astron. 60, 295, describing the maps.
maps/               - subdirectory with compressed map files
                      (168 files)
  car100.1.map.bz2       - data for subfield CAR100.1
  car100.2.map.bz2       - data for subfield CAR100.2
  car100.3.map.bz2       - data for subfield CAR100.3
  car100.4.map.bz2       - data for subfield CAR100.4
  car100.5.map.bz2       - data for subfield CAR100.5
  car100.6.map.bz2       - data for subfield CAR100.6
  car100.7.map.bz2       - data for subfield CAR100.7
  car100.8.map.bz2       - data for subfield CAR100.8
  ...
  mus101.1.map.bz2       - data for subfield MUS101.1
  mus101.2.map.bz2       - data for subfield MUS101.2
  mus101.3.map.bz2       - data for subfield MUS101.3
  mus101.4.map.bz2       - data for subfield MUS101.4
  mus101.5.map.bz2       - data for subfield MUS101.5
  mus101.6.map.bz2       - data for subfield MUS101.6
  mus101.7.map.bz2       - data for subfield MUS101.7
  mus101.8.map.bz2       - data for subfield MUS101.8

ref_images/         - subdirectory with compressed I-band reference images
                      (168 FITS files, 2180x4176 pixels)
  car100.i.1.fts.bz2     - I-band reference image of the subfield CAR100.1 
  car100.i.2.fts.bz2     - I-band reference image of the subfield CAR100.2 
  car100.i.3.fts.bz2     - I-band reference image of the subfield CAR100.3 
  car100.i.4.fts.bz2     - I-band reference image of the subfield CAR100.4 
  car100.i.5.fts.bz2     - I-band reference image of the subfield CAR100.5 
  car100.i.6.fts.bz2     - I-band reference image of the subfield CAR100.6 
  car100.i.7.fts.bz2     - I-band reference image of the subfield CAR100.7 
  car100.i.8.fts.bz2     - I-band reference image of the subfield CAR100.8 
  ...
  mus101.i.1.fts.bz2     - I-band reference image of the subfield MUS101.1 
  mus101.i.2.fts.bz2     - I-band reference image of the subfield MUS101.2 
  mus101.i.3.fts.bz2     - I-band reference image of the subfield MUS101.3 
  mus101.i.4.fts.bz2     - I-band reference image of the subfield MUS101.4 
  mus101.i.5.fts.bz2     - I-band reference image of the subfield MUS101.5 
  mus101.i.6.fts.bz2     - I-band reference image of the subfield MUS101.6 
  mus101.i.7.fts.bz2     - I-band reference image of the subfield MUS101.7 
  mus101.i.8.fts.bz2     - I-band reference image of the subfield MUS101.8 

All *.bz2 files are compressed with the bzip2 utility.

Format of maps in C-language is:

"%6d %11s %11s %7.2f %7.2f %6.3f %6.3f %6.3f %3d %2d %5.3f %4d %2d %5.3f\n"
 
with columns:
                                                 V-band     I-band
DB_no RA(J2000) DEC(J2000) X_ref Y_ref V V-I I  Ng Nb sig  Ng Nb sig

where

DB_no - number in the database,
RA, DEC - equatorial coordinates,
X_ref,Y_ref - pixel coordinates in the I-band reference image,
V, V-I, I - photometry data,
Ng - number of "good" measurements,
Nb - number of "bad" (removed with 5 sigma rejection alghoritm) measurements,
sig - standard deviation of "good" measurements.

Here is a sample of data from the CAR100.1 subfield map:

     1 11:07:04.46 -61:23:31.8  294.26   49.94 16.459  1.779 14.679   3  0 0.002 1682  0 0.010
     2 11:07:04.80 -61:22:34.5  514.49   60.12 14.823  0.715 14.108   3  0 0.004 1874  3 0.008
     3 11:07:08.48 -61:23:07.3  387.98  161.32 15.424  0.948 14.476   3  0 0.002 2678  1 0.006
     4 11:07:09.05 -61:22:35.5  510.34  177.54 15.448  0.902 14.546   3  0 0.001 2680  0 0.010
     5 11:07:09.77 -61:23:00.5  414.15  196.89 15.609  1.235 14.374   3  0 0.005 2668 15 0.008
     6 11:07:10.38 -61:22:38.8  497.40  214.18 15.374  0.970 14.404   3  0 0.002 2683  1 0.006
     7 11:07:11.95 -61:24:33.9   54.68  255.49 99.999  9.999 99.999   0  0 9.999    0  0 9.999
     8 11:07:13.81 -61:22:38.7  497.27  308.60 99.999  9.999 99.999   0  0 9.999    0  0 9.999
     9 11:07:14.71 -61:23:24.8  320.12  332.82 14.317  9.999 99.999   3  0 0.003    0  0 9.999
    10 11:07:15.12 -61:24:12.6  136.06  343.20 15.483  0.949 14.533   3  0 0.000 2481  9 0.008

WARNING!!! "Magic" numbers: 99.999 for magnitude and 9.999 for color and
standard deviation denote "no measurement". -1 in the N_b V-band column
indicates that the V-band counterpart of an object was found in more
than one subfield and the photometry was merged.


!!! Any presentation of the scientific analysis or usage of the data from
the OGLE-III VI maps of the SMC should cite the apropriate OGLE paper(s). !!!