HST Keyword Dictionary
Space Telescope Science Institute
3700 San Martin Drive
Baltimore, MD 21212
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Keyword Definitions for the
- High Speed Photometer
- Unique Data Log Header
This is version 11.4, dated 16-NOV-1987
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- ASA_FILE
- area scan analog is present
Datatype: LOGICAL*1
Units:
-
Source :
- ASD_FILE
- area scan digital is present
Datatype: LOGICAL*1
Units:
-
Source :
- ASK_FILE
- analog sky science is present
Datatype: LOGICAL*1
Units:
-
Source :
- AST_FILE
- analog star science is present
Datatype: LOGICAL*1
Units:
-
Source :
- DSK_FILE
- digital sky science is present
Datatype: LOGICAL*1
Units:
-
Source :
- DST_FILE
- digital star science is present
Datatype: LOGICAL*1
Units:
-
Source :
- THRESH
- PAD threshold setting for the object detector
Datatype: INTEGER*4
Units:
-
detector:
Source :
- VDATAFMT
- Format of current observation
Datatype: CHARACTER*04
Units:
-
1: byte,
2: word,
3: longword,
4: analog
7: all
Source :
- VFAPVECX
- x cmp apt vct f/ tav
Datatype: INTEGER*4
Units:
-
the home position of the image. The vector is set by the user
with a default of 0. It can be used to point from a small observing
aperture to the center of the finding aperture image. (norton.51)
Source :
- VFAPVECY
- y cmp apt vct f/ tav
Datatype: INTEGER*4
Units:
-
the home position of the image. The vector is set by the user
with a default of 0. It can be used to point from a small observing
aperture to the center of the finding aperture image. (norton.51)
Source :
- VFCENVEX
- x cmp trg ct vct tav
Datatype: INTEGER*4
Units:
-
points from the coarse target to the centroid of the target's
individual measurements. (norton.52)
Source :
- VFCENVEY
- y cmp trg ct vct tav
Datatype: INTEGER*4
Units:
-
points from the coarse target to the centroid of the target's
individual measurements. (norton.52)
Source :
- VFCTVECX
- x cmp crs trg vt tav
Datatype: INTEGER*4
Units:
-
The vector points from the center of the finding aperture image
to the row and column representing the candidate. (norton.51)
Source :
- VFCTVECY
- y cmp crs trg vt tav
Datatype: INTEGER*4
Units:
-
The vector points from the center of the finding aperture image
to the row and column representing the candidate. (norton.51)
Source :
- VFFTVECX
- x cmp fn trg vct tav
Datatype: INTEGER*4
Units:
-
This is the fine target vector, representing the sum of VFCENVE and
VFCTVEC. (norton.52)
Source :
- VFFTVECY
- y cmp fn trg vct tav
Datatype: INTEGER*4
Units:
-
This is the fine target vector, representing the sum of VFCENVE and
VFCTVEC. (norton.52)
Source :
- VFOBJCNT
- count of trg obj
Datatype: INTEGER*4
Units:
-
Gives the total number (in the range between VFLOFLIM and VFHIFLIM)
of Target Acquisition and Verification objects found. Only the
brightest 20 are saved, although this count could exceed that
number. (norton.50)
Source :
- VFOCUSD
- focus command value for object detector
Datatype: INTEGER*4
Units:
-
Source :
- VFPFACTX
- tav vct cnv fctr - x
Datatype: INTEGER*4
Units:
-
These constants define the conversion between the TAV image
scale and the scale of the image projected by the Space Telescope
on the face of the detector. (norton.47)
Source :
- VFPFACTY
- tav vct vnv fctr - y
Datatype: INTEGER*4
Units:
-
These constants define the conversion between the TAV image
scale and the scale of the image projected by the Space Telescope
on the face of the detector. (norton.47)
Source :
- VFSLWVEX
- x cmp slew vct tav
Datatype: INTEGER*4
Units:
-
This is the vector issued as a slew request. It represents the vector
sum of VFFTVEC and VFAPVEC, and points from the desired observing
aperture to the centroid of the target's inidivual measurements.
(norton.52)
Source :
- VFSLWVEY
- y cmp slew vct tav
Datatype: INTEGER*4
Units:
-
This is the vector issued as a slew request. It represents the vector
sum of VFFTVEC and VFAPVEC, and points from the desired observing
aperture to the centroid of the target's inidivual measurements.
(norton.52)
Source :
- VGAIND
- gain setting of detector 1
Datatype: INTEGER*4
Units:
-
Gain setting of the object or sky depending on data source. (cgpsdh)
Source :
- VGAINDS
- gain setting of detector "sky"
Datatype: INTEGER*4
Units:
-
See VGAINDn.
Source :
- VHIVOLT1
- high voltage setting for detector 1
Datatype: INTEGER*4
Units:
-
Source :
- VHIVOLT2
- high voltage setting for detector 2
Datatype: INTEGER*4
Units:
-
Source :
- VHIVOLT3
- high voltage setting for detector 3
Datatype: INTEGER*4
Units:
-
Source :
- VHIVOLT4
- high voltage setting for detector 4
Datatype: INTEGER*4
Units:
-
Source :
- VHIVOLT5
- high voltage setting for detector 5
Datatype: INTEGER*4
Units:
-
Source :
- VHIVOLTS
- high voltage setting for detector "sky"
Datatype: INTEGER*4
Units:
-
Source :
- VHORIZ
- commanded horizontal deflection of obj detector
Datatype: INTEGER*4
Units:
-
Source :
- VHORSTPT
- no. of horiz steps/spatial point in area scans
Datatype: INTEGER*4
Units:
-
Deflection steps correspond to about 4.42 microns on the face
of the image dissector tube. If the incrementing process
(starting with the initial deflection) causes the deflection
value to exceed the 12-bit capacity (4096), the counter wraps
and starts over at zero. (Norton.33)
Source :
- VHPOINTS
- no. of horiz points (columns) in area scans
Datatype: INTEGER*4
Units:
-
Source :
- VNOINTPT
- no. of integrations/pt in area scans
Datatype: INTEGER*4
Units:
-
Number of integrations to be done at each of the points in an
area scan. the default value for this parameter after initialization
is 1. (norton.33)
Source :
- VOLTAGE
- commanded high voltage setting of obj detector
Datatype: INTEGER*4
Units:
-
Source :
- VPADTHR1
- PAD threshold setting for detector 1
Datatype: INTEGER*4
Units:
-
Source :
- VPADTHR2
- PAD threshold setting for detector 2
Datatype: INTEGER*4
Units:
-
Source :
- VPADTHR3
- PAD threshold setting for detector 3
Datatype: INTEGER*4
Units:
-
Source :
- VPADTHR4
- PAD threshold setting for detector 4
Datatype: INTEGER*4
Units:
-
Source :
- VPADTHR5
- PAD threshold setting for detector 5
Datatype: INTEGER*4
Units:
-
Source :
- VPADTHRS
- PAD threshold setting for detector "sky"
Datatype: INTEGER*4
Units:
-
Source :
- VREQDET
- requested detector for the object observation
Datatype: CHARACTER*08
Units:
-
1: IDT1 (Image Dissector Tube 1)
2: IDT2 (Image Dissector Tube 2)
3: IDT3 (Image Dissector Tube 3)
4: IDT4 (Image Dissector Tube 4)
5: PMT (Photomultiplier)
Source :
- VSKYDET
- currently selected sky detector
Datatype: CHARACTER*08
Units:
-
1: IDT1 (Image Dissector Tube 1)
2: IDT2 (Image Dissector Tube 2)
3: IDT3 (Image Dissector Tube 3)
4: IDT4 (Image Dissector Tube 4)
5: PMT (Photomultiplier)
Source :
- VVERSTPT
- no. of vert. steps/spatial pt. in area scans
Datatype: INTEGER*4
Units:
-
Deflection steps correspond to about 4.42 microns on the face
of the image dissector tube. If the incrementing process
(starting with the initial deflection) causes the deflection
value to exceed the 12-bit capacity (4096), the counter wraps
and starts over at zero. (Norton.33)
Source :
- VVERT
- commanded vertical deflection of obj detector
Datatype: INTEGER*4
Units:
-
Equivalent to VVERTn for when the object detector=n. (cgpulk)
Source :
- VVERTn
- Vertical deflection for detector 1
Datatype: INTEGER*4
Units:
-
Sets the 12bit DAC which determines the initial vertical image
dissector tube deflection current. (norton.35)
Source :
- VVPOINTS
- no. of vertical points (rows) in area scans
Datatype: INTEGER*4
Units:
-
Source :
HST Keyword Dictionary: 3/15/94: (rose@stsci.edu)