Data outside the survey area
There are tsObj files in DR1 which have no or few primary objects
because they lie outside the lambda limits in a number of stripes. As
a consequence, the photometry catalogs for this part of the sky are
not accessible through the Imaging Query Server,
and the Spectro Query
Server will not find spectra from this part of the sky if you
request, or select on, imaging parameters. This affects about 5000
galaxy spectra, and a much smaller number of other spectral
objects.
Here is the list of fields which have no or few
primary objects.
stripe 10:
run fields
1239 11-33
756 41-63
745 534-609
752 636-711
stripe 12:
run fields
2125 13-32
2126 11-29
stripe 34:
run fields
2131 17-34
2137 47-64
stripe 35:
run fields
2328 168-179
2305 168-180
stripe 36:
run fields
2248 263-274
2335 136-148
stripe 37:
run fields
1350 20-23
1402 11-14
Another thing to watch out for is that the mu limits in the
tsChunk*.par files will therefore extend beyond the survey lambda
limits. A consequence is that the mask csv's, which use these
mu limits, will extend beyond the lambda limits as well.
Last modified: Tue Apr 29 11:13:28 CDT 2003
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