THE UMASS GALAXY POSTAGE STAMP IMAGE ARCHIVE  (DRAFT FOR REVIEW)
The UMASS galaxy postage stamp image archive contains 2,577,162 gzip compressed six plane fits images stored on 3-750 GB Reiser file system SATA hard disks. Galaxy postage stamp images are stored in the same directories as the scan-sized fits images.

Galaxy postage stamp image files are distributed on the hard disks in order of date of original observation.
Image files on these disks may be accessed by clicking on the links above. As the disks may be in the idle state and the directories are large it may take some time for the disk directory to appear.

The complete path from the top directory of an archive disk and the file name for postage stamp images in the archive is as follows:

/DDDDDDH/sSSS/gDDDDDDHSSSFCCCiIIIIII.fits.gz
/981029s/s028/g981029s0280221i003157.fits.gz  

The fields in the above path/filename are Date, Hemis, Scan, F_type, Coadd, and Id. The first letter of the file name is 'g' to indicate that the file is a galaxy postage stamp. The file name for postage stamps is slightly different from that of image archive files because it was necessary to add the id field to make the file names unique.

A postgres loadable table gal_pstamps is available for searches on the galaxy postage stamp archive. An explanation of the gal_pstamps fields is given in format_gal_pstamps.html.  
All of the postage stamp images have f_type='0', i.e. they have not been modified to to make them more compressible by removing low-order bit noise. All are gzip compressed. The gal_pstamps table entry for the postage stamp used for illustration on this page is:

    date    | hemis | scan | scan_key | cat_scn | qual | coadd |  id  | naxis2 |             f_name             | f_size | f_type | disk |     ra      |     decl     | xsc_prox | ext_key | jskyval | jskysig  | hskyval | hskysig  | kskyval | kskysig  | jseesh | hseesh | kseesh | jmagzp  | hmagzp  | kmagzp
------------+-------+------+----------+---------+------+-------+------+--------+--------------------------------+--------+--------+------+-------------+--------------+----------+---------+---------+----------+---------+----------+---------+----------+--------+--------+--------+---------+---------+---------
 1998-10-29 | s     |   28 |     7931 | y       |    9 |   221 | 3157 |     39 | g981029s0280221i003157.fits.gz |  17717 | 0      | ia_1 | 74.10629272 | -64.96828461 |    0.001 |  297801 | 67.9967 | 0.504965 | 280.043 | 0.788282 | 478.773 | 0.978596 |  1.002 |  0.988 |  1.013 | 20.7808 | 20.3702 | 19.8559

The size of this archive is as follows: The gal_pstamps table can be downloaded from the following links to compressed comma delimited ascii files with null as \N:
A postgres function get_pstamp can be used to create path and file names for galaxy postage stamps. This function is not guaranteed to return a valid path/filename unless its arguments are  from or joined to the gal_pstamps table.

Example:
psql -Atc "SELECT get_pstamp(date,hemis,scan,coadd,id) FROM gal_pstamps WHERE naxis2 > 100 LIMIT 5" wsdb
Result:
/image_archive/ia_3/000926s/s086/g000926s0860267i000410.fits.gz
/image_archive/ia_3/000211s/s035/g000211s0350267i000439.fits.gz
/image_archive/ia_3/000211s/s049/g000211s0490267i000435.fits.gz
/image_archive/ia_3/000322s/s097/g000322s0970267i000449.fits.gz
/image_archive/ia_3/000211s/s040/g000211s0400267i000455.fits.gz


PROPERTIES OF THE POSTAGE STAMP IMAGES
 
Postage stamp images are discussed in sec 1_3 of the explanatory supplment.
An example image from the UMASS archive may be downloaded by clicking on the following file name g981029s0280221i003157.fits.gz .  A utility,  splitfits for creating a single fits image from one of the six images in a galaxy postage stamp has been provided by Martin Weinberg.  A cutout of the j-band image of the above galaxy from the UMASS coadd image archive can be downloaded by clicking on j_original.fits.gz .  A comparison of the j-band background subtracted image with the UMASS coadd image is shown in the figure below:


j band original coadd image. Sky subtracted postage stamp image. Original-GPS image
J Band Original Coadd  Sky subtracted J Postage Stamp Image  Difference of the two images


The value of JSKYVAL in the postage stamp header is 67.99669657.  A comparison of the difference between the original and the sky subtracted fits files is as follows.

  mean value  = 67.9972
  minimum value = 67.9425
  maximum value = 68.0599
 
The tiny variations shown in the difference fits file are present because the coadd images in the UMASS archive have very low order computational noise removed to make them more compressible whereas the galaxy postage stamps do not. 

The second J-band image of a galaxy postage stamp fits file has background and star flux subtracted.  


j band original coadd image. Sky subtracted postage stamp image. Original-GPS image
Sky subtracted J postage stamp  Sky and star subtracted J postage stamp Difference of the two images

The difference image above shows that only the brighter two of the four stars visible in the sky subtracted image have been removed from the sky and star subtracted image. The point source catalog, two_mass_psc, contains four stars within 30 arc-seconds of the galaxy.  The following table lists all twomass_psc sources within 30 arc-seconds of the galaxy.


  pts_key  | ext_key |    ra     |    decl    |  j_m   | dist(sec)| subtracted
-----------+---------+-----------+------------+--------+----------+------------
 136501710 |  297801 | 74.106295 | -64.968407 |  13.66 |        0 |    no
 136501703 |         | 74.101881 | -64.966072 | 16.762 |       11 |    no
 136501716 |         | 74.110959 | -64.971382 | 16.782 |       13 |    no
 136501711 |         | 74.115342 | -64.968941 | 15.314 |       14 |   yes
 136501693 |         | 74.104242 | -64.962784 |  12.53 |       20 |   yes

These detections are illustrated on the image below:

j_band annotated image
 J magnitude of twomass_psc sources



 Requests for copies of image archive hard disks should be directed to Rae Stiening at the University of Massachusetts.  Last updated May 23, 2008