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UFTI manual
Anomalous patterns/structures in UFTI images
Below we show examples of some unusual image structures that have been
seen in UFTI frames. In some cases, the fix seems to be to take a
sequence of short dark exposers (use the "flush array" sequence in the
ORAC-OT template library). These rare structures often result from
leaving the array exposed to background signal (i.e. leaving the
shutter open with a filter in place) or from observing very bright
sources. Fringes may appear if bright stars are present just outside
the target field-of-view.
Click on the icon at left for a larger gif image.
| Example Image |
Description |
Fix |
|
Rectangular bias structure |
Flush array with 3 or 4 short dark exposures |
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Patch of "warm" pixels (few tens of counts) |
Flush array with 3 or 4 short dark exposures |
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Latent image of bright star from a previous jitter position. |
Flush array with 3 or 4 short dark exposures |
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1Fringes (scattered light from nearby bright star?) |
-- |
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2Fringes again (scattered light from nearby star?) |
-- |
|
3Ghost images of bright star with Narrow-band filter |
Median average (rather than average) frames in mosaic |
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4Horizontal "banding" from electronic pickup |
-- |
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5Vignetting "strips" in data |
Median average (rather than average) frames in mosaic |
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6Severe/random horizontal "stripes" (in
darks and sky exposures) |
Reboot UFTI crate (or power cycle array controller) |
Notes:
1The difference of two spatially-offset (by a few arcseconds)
frames; hence fringe seen in positive and (offset) negative.
2Mosaic from a 5-point jitter with fringe at same loaction in
each frame.
3Mosaic from a 5-point jitter with ghosts (one per image,
shifted relative to bright star in each image) appearing in the resulting mosaic after
registration and averaging.
4Horizontal "banding" from electronic pickup (10-20 rows wide; amplitude ~10 counts),
carried through into the dark-subtracted and (self)-flat-fielded object frame.
5Mosaic from a nine-point jitter. The 1-0S(1) filter vignettes the bottom few rows
of each image, so when the nine frames are registered and averaged horizontal strips of noise appear
in the mosaic. Vary N-S jitter offsets and MEDIAN average the data (this can be done with ORAC).
6Sudden change, from clean images to this after only 2-3 exposures;
power-cycling the electronics fixed this (at least temporarily).
There is also available a short document (postscript
file) written by Sandy Leggett when she investigated the
appearance of "fringes" in IRCAM data (from 1997). The fringes seem to be
caused by reflections or scattered light from IR-bright stars that are
situated just outside the array field-of-view.
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