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Science Run Archive
ATICA organized the events it extracted in the same way that the flight
software organizes science data - by science runs which are defined
in Ford & Francis (1997). ATICA creates a directory for each science
run, named for the mode and start time of the run, e.g. the run tefwb_111:07:17
was a Timed Exposure Faint With Bias run that started at IRIG time 111:07:17.
Within that directory the event list is arbitrarily divided into files
of about 100,000 events each. ATICA was not able to organize the data by
TRW ID because the flight software and thus the telemetry knew nothing
about that concept. Unfortunately it was necessary to schedule multiple
TRW ID's within one ACIS science run so a single ATICA output directory
will contain data from several TRW ID's.
The FITS binary tables used to store the event lists consist of the
following columns.
-
TIME: A timestamp for the CCD frame, expressed as an IRIG time in seconds,
i.e. the number of seconds since 1997.0.
-
CHIPX/CHIPY: The 1-based position of the event. Note that the flight software
telemeters event positions in a 0-based system.
-
TDETX/TDETY: The position of the event in the ``tiled coordinate system
AXAF-ACIS-2.2'' defined by Jonathan McDowell at the ASC [McDowell1997].
-
CCD_ID: The CCD that detected the event. (See Table 3.1.)
Table 3.1: Conversion table from CCD_ID to ACIS array location.
| CCD_ID |
Chip |
Serial # |
CCD_ID |
Chip |
Serial # |
CCD_ID |
Chip |
Serial # |
| 0 |
I0 |
w203c4r |
4 |
S0 |
w168c4r |
8 |
S4 |
w457c4 |
| 1 |
I1 |
w193c2 |
5 |
S1 |
w140c4r |
9 |
S5 |
w201c3r |
| 2 |
I2 |
w158c4r |
6 |
S2 |
w182c4r |
|
|
|
| 3 |
I3 |
w215c2r |
7 |
S3 |
w134c4r |
|
|
|
-
AMP_ID: The amplifier, numbered 0,1,2,3, associated with the central pixel
of the event.
-
EXPOSURE: The exposure sequence number as telemetered by the flight software.
-
PHAS: For most modes this is a 9 element vector containing the event island
pixel values NOT corrected for bias. The relationship between this 9-vector
and the 3x3 event island is shown in Figure 3.1.
Figure 3.1: Ordering of the elements of the PHAS and BIAS
Vectors
 |
-
BIAS: A vector of the same form as PHAS, containing the BIAS values used
for processing this event.
-
OVRCLK: The overclock value associated with the amp in AMP_ID for this
exposure.3.1



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Please address comments and questions to Dr. John Nousek ( nousek@astro.psu.edu
)