- An OGIP-compliant Ancillary Response File, as defined in [4].
This contains a table labelled ARF, that in turn
contains:
- A column labelled ENERG_LO,
containing the lower bounds for each energy bin (keV).
- A column labelled ENERG_HI,
containing the upper bounds for each energy bin (keV).
- A column labelled SPECRESP,
listing the area for each energy bin described
by the ENERG_LO and ENERG_HI columns.
and the following attributes:
- TELESCOP
- INSTRUME
- FILTER
- ARFVERSN
- HDUCLASS
- HDUCLAS1
- HDUCLAS2
- HDUCLAS3
- HDUVERS1
- A intermediate and temporary dataset containing the
input detector map in pixel list form.
used as input to attcalc
to compute the detector-sky coordinate conversion.
This contains a table labelled EVENTS, which
in turn contains:
- A column labelled VALUE of type real-64
- A column labelled X of type int-32
- A column labelled Y of type int-32
- A column labelled DETX of type int-16
- A column labelled DETY of type int-16
- A column labelled TIME of type real-64
and the following attributes:
- TELESCOP
- INSTRUME
- DATAMODE
- A version of the input detector map, in pixel
list form, filtered using the DSS information
stored in the spectrum dataset. This is written
out as a permanent dataset with a name
corresponding to filteredset
if withfilteredset is set to true.
This contains a table labelled EVENTS, which
in turn contains:
- A column labelled VALUE of type real-64
- A column labelled X of type int-32
- A column labelled Y of type int-32
- A column labelled DETX of type int-16
- A column labelled DETY of type int-16
- A column labelled TIME of type real-64
and the following attributes:
- TELESCOP
- INSTRUME
- DATAMODE
