EDS Configurations: Generic Binned
- General Description
- Detailed Description
- Reduction requirements and options
- Gain and offset
- Other features
The generic Binned configurations are designated with a character string beginning with B, e.g. B_250us_2A_0_17_Q.
Files containing Binned data are in science array format. The science data occupy the XTE_SA extension in the form of histograms accumulated from good xenon events (i.e. those which survive background rejection, but sometimes including propane veto events) according to time, in two or more channel bands. The columns containing the histograms are preceded by the Time column which gives the time of the start of each accumulation.
The naming convention of the configuration provides a summary of the
properties of the data. For generic binned data, the format
gives
While the configuration name provides a summary of the properties of the
data, further information is written in the file itself. This more
detailed information is accessible via the ftools fstruct, flcol, fdump and fkeyprint. We recommend that you run these tools on sample files (one, say, per configuration), starting with fstruct, the least verbose. Here are the key pieces of information, and where to find them:
The above information - time resolution, channel boundaries etc - is also available in one place in the data file, namely the DDL string which occupies the TTDES2 keyword. DDL - Data Description Language - is a compact way of describing the properties of the data for downstream software. Although somewhat terse, it is not difficult to read. For example, the value of TTDES2 for the B_250us_2A_0_17_Q configuration is:
Spectra and light curves are extracted from generic binned data using
the ftool saextrct. Binned configurations with just a few
channels will, of course, result in crude spectra. Apart from adjusting screening criteria,
your primary reduction options will always include:
Gain and offset corrections are applied by the EDS to generic Binned data.
In common with other configurations in science array format, generic Binned files have two additional columns called Spillage and ModeSpecific, as well as a coda of keywords summarizing EDS status.
General Description
Detailed Description
B_ttt_ccX_0_hh_b
For example, in the B_250us_2A_0_17_Q configuration, two
histograms with ~250-microsecond resolution are accumulated from
channels 0 to 17, with the "A" channel distribution/binning
scheme. "Q" means that there are 4 bits per bin, i.e. that up to 16
counts can be accumulated per ~250 microseconds without overflowing
the telemetry. For a complete list of available Binned mode
configurations, see the RXTE
PCA Configurations page. For more details about the different
binned mode configurations, please consult the Technical Appendix.
Note that the accumulation time of the histograms is not a key
piece of information for most users, as it only dictates the
arrangement of the data in the file, rather than their scientific
properties. The RXTE ftool saextrct transparently extracts data
without your having to know how many steps each histogram contains or
how often the histograms are accumulated. However, if you intend to
write your own data reduction software, the accumulation time is
crucial. To determine it, use fkeyprint to look at the
DELTAT keyword. For example, in the
B_250us_2A_0_17_Q configuration, the value of DELTAT
is 2 seconds.
D[0~4] & E[X1L^X1R^X2L^X2R^X3L^X3R] & C[0~11,12~17] & T[0.0;0.000244140625;8192]
which, broken down into its parts, means:
Reduction requirements and options
The RXTE Cookbook recipe Reduction and Analysis of PCA
Spectra describes reduction of Standard 2 mode data, but also
provides general guidelines for reducing any generic binned
configuration.
Gain and offset
Other features
The ABC of XTE is written and maintained by the RXTE GOF. Please email xtehelp@athena.gsfc.nasa.gov if you have any questions or comments. This particular page was last modified on Tuesday, 14-Sep-1999 13:45:43 EDT.

