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File Name Conventions
Most ASCA file names have one of two forms. The first is a date and time based
format used for telemetry files and files derived directly from them.
The other is a sequence number based file name, with additional components
describing the conditions under which the data were taken. Most files
have the sequence number based format.
Date-Based File Names
Telemetry, attitude, housekeeping, gain history, and filter files
all follow a date and time based format
(e.g. ft930415_2053_0240.mkf).
Their names have five parts:
- A prefix - `fa' for attitude files and `ft'
for all other files.
- The starting date of the data in the file in `yymmdd' format.
- The starting time (UT) of the data in the file in `hhmm' format.
- The ending time (UT) of the data in the file, also in `hhmm' format.
Note that files may go past midnight, so the ending time may be smaller
than the starting time.
- An extension specifying the file type (see the descriptions of the
individual files).
The example file name given above covers data starting on April 15, 1993
at 8:53 PM UT, and ending at 2:40 AM UT, probably on the following day.
Sequence Number Based Filenames
Most file names have a sequence number based format
(e.g. ad51011020s100102h.unf, ad51011020g210170_0.pi,
ad51011020gis25670_hi.totsky). This format has several parts as follows:
- The string `ad' which stands for "Astro-D".
This is the pre-launch name for ASCA.
- The eight-digit sequence number unique to this observation.
Some of its digits
have special significance.
The first digit of
the sequence number gives the target type as follows:
- '1' - Calibration and Targets of Opportunity.
- '2' - Stars
- '3' - Cataclysmic Variables
- '4' - X-Ray Binaries
- '5' - Supernova Remnants and Galactic Diffuse
Emission
- '6' - Galaxies
- '7' - Active Galactic Nuclei
- '8' - Clusters of Galaxies and Superclusters
- '9' - X-Ray background, Deep Survey, and other
For non-calibration sequences, the second digit gives the AO number,
with `0' used for PV phase data.
Multiple observations for the same proposal will generally
have sequence numbers which differ only in their second-to-last digit.
- Instrument name. This can be one of `s0', `s1',
`g2', or `g3'
for SIS0, SIS1, GIS2, or GIS3, respectively.
Also 'sis' is used to refer to data which combine SIS0 and
SIS1, and 'gis' is used to refer to data which combine
GIS2 and GIS3.
- Index. This is a three digit number mostly used to keep file names
unique. In general a file will have the same index as the file from
which it was derived. For image and source list files, the index
refers to the number of pixels across the image.
- Observing mode. This is a two digit code specifying the instrument mode
as follows:
- 01 for SIS Faint mode data.
- 02 for SIS Bright mode data.
- 12 for SIS Bright2 mode data.
- 03 for SIS FAST mode data.
- 70 for GIS PH mode data.
- 71 for GIS MPC mode data.
- Bit-rate. This is the single character
`h',
`m', or
`l' for high, medium or low bit-rate, respectively. Some of
the data products such as images, spectra, and binned light curves may
combine data of different bit-rates, and therefore do not have a
bit-rate designation.
- Source number. Products such as spectra and light curves are extracted
for individual sources within the field of view of the instruments.
The source number is a single digit separated from the rest of the
file name by an underscore. Source `_0' is used to refer to
the entire field of view with all detected sources excluded.
- Extension. File names will generally have additional characters
separated by an underscore or dot which indicate the file type.
See the descriptions of individual file types for more information.
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