K Release Notes—V2.1-0
The main changes are the addition of spatially jittered Fabry-Perot recipes, and recipes for compact
comets.
K.1 New recipes
-
FP_JITTER
- Reduction of a Fabry-Perot observation, comprising eight frames, on and off the
source, and on and off the spectral line both to the blue and to the red. This is repeated
for a series of spatial positions of the source.
-
FP_JITTER_NO_SKY
- Reduction of a Fabry-Perot observation, comprising four frames, all on
the source, and on and off the spectral line both to the blue and to the red. This is repeated
for a series of spatial positions of the source.
-
MOVING_QUADRANT_JITTER
- As QUADRANT_JITTER but registration is adjusted to track
the motion of a comet using ephemeris data. The comet should 45
arcsec diameter for UFTI, or 10
arcsec for IRCAM. Compared with MOVING_JITTER_SELF_FLAT, this recipe avoids
cometary artifacts appearing in the flat field.
-
QUADRANT_JITTER_TELE
- As QUADRANT_JITTER, but registers using the telescope
offsets. This is used for observing compact comets (limiting angular sizes as above), when
the telescope has tracked the nucleus.
K.2 Modified recipes
- ARRAY_TESTS For UFTI, the ADU conversion is obtained from the GAIN header, rather
than being hardwired at 7.0.
- CHOP_SKY_JITTER This now functions correctly for multiple cycles of the recipe.
- FP Documentation improvements especially in the description. Primitive _FP_STEER_
has a new steering parameter, NPAIRS, and parameter NUMBER has changed to its
normal meaning.
- NIGHT_LOG This can start from observation numbers other than 1. A bug has been fixed
where the dimensions appeared as zero for UFTI. It arose because certain headers no
longer existed after 2000 August.
- SKY_FLAT_FP This is no longer limited to eight frames.
- SKY_AND_JITTER A bug has been fixed where some intermediate files were not being
removed for this recipe and its variant.
K.3 Global changes
The main changes from a user perspective were as follows.
- The aperture for _APHOT recipes is now 5 arcseconds.
- A new photometry catalogue
fs2001.dat, supplied in original form by Sandy Leggett, is
used by the _APHOT recipes. The new catalogue contains
magnitudes for the first time, and the
data have been refined to account for recent observations. The 2000 edition is accessed for
photometry if the 2001 catalogue is unavailable.
- Another new UFTI bad-pixel mask. Old masks are available on request.
- A bug that affected some rare mixed-method registrations has been fixed. The
offset had the wrong sign.
- Allow for a special case in the mosaicking registration, when the nearest-neighbour
method is used to align the various images, and an automatic multiple-object registration
was found. It was possible not to find a common object identifier in all the fields when
the target is a low-surface brightness galaxy. While this is still possible, it is far less likely
than before.
- The IRCAM saturation level was refined upwards to 20000, or 33000 if header SPD_GAIN
is "Deepwell". SPD_GAIN is created by the recipe when it is absent, based upon the value
of the detector bias.
- The message concerning an AST SKY Frame creation, which could be confused with a
data frame of blank sky, has been clarified. The same script allows for a missing CROTA2
header in old data when inserting world co-ordinate system headers.
- Various minor improvements and corrections to the documentation, such as correcting
the former prefix for UFTI mosaics in the reference section, and excluding references to
IRCAM in the FP recipes.
Copyright © 2004 Particle Physics and Astronomy Research Council