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: http://xmm.vilspa.esa.es/sas/8.0.0/doc/cifbuild/node13.html Дата изменения: Wed Jul 2 03:28:32 2008 Дата индексирования: Fri Sep 5 20:45:02 2008 Кодировка: Поисковые слова: rainbow | 
 
 
 
 
 
 
 
Here we address the issue of how to determine what calibration files make up the current calibration file for a given observation time.
Each calibration file has a validity start date and a validity end date. These are indicated by the FITS keywords VALDATE and EVALDATE. A missing EVALDATE is taken to mean no end of validity.
Given the naming convention above, a calibration file can be labeled
with a quadruplet of the form 
 ,
where
,
where 
 , and
, and
 is optional.
 is optional.
New issues of a calibration file can enter the archive with any
 , any
, any  , and increasing issue numbers.
, and increasing issue numbers.
In the simplest case (no end of validity date), a new version of the
calibration file -- call it 
 , will have
, will have 
 and
 and
 (figure 1).
 (figure 1).
A more complex situation is illustrated in figure 2. Here new versions are introduced to improve on past calibrations.
In figure 3 we show an example where a CCF
constituent has an end of validity date. In this case at the time 
the situation is the same as shown in figure 2,
whereas at the time  the constituent
xmm_ExampleTwo_005.ccf is no longer applicable.
 the constituent
xmm_ExampleTwo_005.ccf is no longer applicable.
Within this scheme, at any time  the applicable issue of the
calibration file  is obtained by selecting among all files
 the one
with the higher issue number.
 is obtained by selecting among all files
 the one
with the higher issue number.
Should it become necessary, a new  can be introduced in the
archive, as illustrated in figure 4.
 can be introduced in the
archive, as illustrated in figure 4.
With this scheme the number of constituents in the current calibration file is not fixed, and can be determined only when the time is specified.
XMM-Newton SOC/SSC -- 2008-07-01