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.
- ia_1
Dates before February 17, 1998
- ia_2
Dates from February 17, 1998 through December 14, 1999
- ia_3
Dates from December 15, 1999 to end of the survey on February
15, 2001
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:
- All images in the postage
stamp archive:
69.2 GB
- All images with cat_scn='y'
58.1 GB
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.
- Each fits file consists of 6 images, two for each color in
the
order JHKJHK. This structure is described in the fits file header.
- The two images for each band are in order, background
subtracted and background and star subtracted images.
- The images are square but variable in size depending on the
brightness of the galaxy.
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 |
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.
 |
 |
 |
| 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 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