

Index
A
ADC (see "analog-to-digital converter")
AFMs (see "actuated fold mirrors")
AB magnitude
aberration correction
ACOADD (STSDAS)
actuated fold mirrors [1] [2]
Ammonia heat pipe
analog-to-digital converter [1] [2]
AP-17 [1] [2]
apertures
position updates
filter combinations
aperture photometry
Application Processor (see "AP-17")
AREA mode [1] [2]
artifacts
blooming
bright object
diffraction spikes [1] [2]
field flattener ghosts
filter ghosts
horizontal smearing
large angle scattering [1] [2]
residual image
scattering of bright Earth light
CCD, image
astrometry
image scale
B
BSC (Yale Bright Star Catalog)
background
dark count rates
sky
bandpass
effective width
BD+75D325
bias frame
calibration
blooming [1] [2]
breathing
bright objects
avoidance regions
observing strategies
CCD artifacts
Bruzual, Persson, Gunn, Stryker atlas
C
CTE (see "charge transfer efficiency")
CVZ (continuous viewing zone)
calibration
astrometry
bias
bright object artifacts
charge transfer efficiency (CTE) [1] [2]
dark [1] [2]
flat field [1] [2]
flux
linear ramp filters [1] [2]
observations
pipeline process
plan
Cycle 5
Cycle 6
point spread function
polarizers [1] [2]
proposal numbers (see number)
reference files
sky flats
StarView
calibration channel
CALWP2 (see STSDAS)
CCD
34-row defect
back illuminated
blooming [1] [2]
charge transfer efficiency
problem
long-term degradation
charge trapping
clearing
description
DQE
dynamic range
epitaxial thickness
flat field
flat field response
front-side illuminated
full well capacity
gain [1] [2]
gamma
hot pixels
image purge
MTF [1] [2] [3]
vs. WF/PC-1
(see also "pixel response function")
multi-pinned phase [1] [2]
orientation
over-clocked pixels
pixel response function
impact on PSF
polysilicon gate
quantization noise [1] [2]
quantum efficiency
hysteresis [1] [2]
radiation damage
readout
readout time
read noise [1] [2]
recombination length
residual image
bulk residual image
CTE trails
residual image artifact
saturation
Si-SiO2 interface
silicon band-gap
sub-pixel QE variations
thick
undersampling
WFPC2 vs. WF/PC-1
charge transfer efficiency [1] [2] [3]
calibration
long-term degradation
problem
residual image trails
CLOCKS [1] [2] [3] [4]
CMD_EXP
coarse track
cold junction
color transformation
contamination
control
WFPC2 and UV imaging
WFPC2 decontamination and UV response
continous viewing zone
cooldown
cosmic rays [1] [2]
dark current
count rate
dark current
sky
target
Cousins RI
CR-SPLIT [1] [2] [3] [4]
CR-TOLERANCE [1] [2] [3]
D
DQF (see "data quality file")
data quality file
dark current [1] [2]
cosmic-ray induced scintillation
electronic
dark frame
calibration
DARKTIME
data set
contents
Delta Cas
detector MTF (see "CCD MTF")
Deuterium lamp
diffraction spikes
dimensionless efficiency
distortion
optical
DITHER-TYPE
dithering
accuracy
and overhead time
DQE
CCD [1] [2]
dripping and drizzling
dynamic range [1] [2]
E
ETC (see "Exposure Time Calculator")
EARTH-CALIB
efficiency
dimensionless
emission line targets
observation strategies
encircled energy
Epsilon Eridani
EXPEND
EXPFLAG
exposure
overhead time
CCD clearing
CCD readout
dithering
filter change
spacial scans
exposure time
and efficiency
anomalies
CLOCKS=YES
estimation
quantized values
photometric accuracy/errors
reconstructing actual time from shutter blades
Exposure Time Calculator
emission lines
extended sources
stars
stars with background
EXPSTART
EXPTIME
and calibration
F
FGS (see "Fine Guidance Sensor")
faint objects
observing near bright objects
observing strategies
field flattener
short wavelength cutoff
field-of-view
orientation on sky
filter change
filters (see "optical filters")
Fine Guidance Sensor [1] [2] [3]
breathing effects
Fine Lock
and jitter
FK5 (Julian) reference frame
flat field response
flat field
quality
calibration
CCD
sky flats
flux calibration
FULL mode
full well capacity
G
gain
gain switch [1] [2]
ghost images
field flattener
filter ghost
GRW+70D5824 [1] [2] [3]
gyro hold
H
HDF (see Hubble Deep Field)
header keywords
CMD_EXP
DARKTIME
EXPEND
EXPFLAG
EXPSTART
EXPTIME
and darktime
and photometry
PHOTZPT
PHOTFLAM
SHUTTER
UEXPODUR
heat pipe
history
instrument development
hot junction
hot pixels [1] [2]
Hubble Deep Field [1] [2]
I
image purge
CCD
incandescent lamps
instrument
optical filters
configuration [1] [2]
description
objectives
INT ACQ
Investigation Definition Team
J
Johnson UBVRI
K
K-spots (Kelsall spots)
internal monitor
L
LRF (see "linear ramp filters")
lamps
Deuterium
incandescent
large angle scattering [1] [2]
linear ramp filters
calculator tool
calibration observations
observing with
using POS TARGs
loss of guide star lock
LOW-SKY [1] [2]
Lumogen [1] [2] [3]
M
MPP (multi-pinned phase)
operating principle
M67
magnitude
AB
Johnson-Cousins [1] [2]
Oke system
STMAG
Stromgren
determining
mean wavelength [1] [2]
measles
WF/PC-1
methane quad filter
METRIC (STSDAS)
mode
AREA [1] [2]
FULL
SUM=2x2
multi-pinned phase (MPP)
operating principle
N
NGC 2100
NGC 2419
NGC 2682 (M67)
NGC 4472
NGC 5139 (Omega Cen) [1] [2] [3]
noise
background
dark current
CCD read noise [1] [2]
quantization [1] [2] [3]
NSSC-1
O
OTA (see "Optical Telescope Assembly")
observing strategies
bright targets
CCD position and orientation on sky
choosing exposure times
cosmic rays
dithering
emission lines in galaxy nuclei
faint objects
faint targets near bright objects
linear ramp filters
pointing accuracy
polarization
Omega Cen [1] [2] [3]
on-line calculator (see also "Exposure Time Calculator")
optics
actuated fold mirrors [1] [2] [3]
Cassegrain relay
diffraction spikes
distortion
field flattener [1] [2]
image scale
pick-off mirror [1] [2] [3] [4]
impact on polarization
pyramid mirror [1] [2] [3]
relay
spherical abberation
wavefront quality
optical alignment
optical filters
aperture combinations
broad band
features
linear ramp
mean wavelength
methane quad
narrow band
OII redshifted quad
polarizer quad
red leaks
simple
transmission curves
UV quad ([OII])
Wood's
Optical Telescope Assembly [1] [2]
breathing
effect on PSF subtraction
diffraction spikes
focus adjustments
ORIENT
avoiding bloom track
how to compute
over-clocked pixels
overexposure
CCD artifacts
overhead time
P
PSF (see "point spread function")
PCS MODE
PHOTFLAM
photometry
accuracy when CLOCKS=YES
breathing
encircled energy
focus adjustments
orbital variations
sub-pixel response
system throughput
zeropoint
PHOTZPT
pick-off mirror [1] [2] [3] [4]
pipeline calibration [1] [2]
pivot wavelength
pixel response function (see also "CCD MTF")
impact on PSF
plate scale
PODPS
point spread function
astigmatism
in PC1 [1] [2]
in WFC
breathing
calibration [1] [2]
encircled energy
fitting
jitter
loss of lock
model PSF
subtraction
variation with field position
variations with time
pointing
accuracy
jitter
repeatability
polarizers
calibration [1] [2]
filter
observation strategies
POS TARG
and LRF filters
vs. spatial scans
pyramid mirror [1] [2] [3]
Q
QEH (see "quantum efficiency hysteresis")
quantization
noise
A-to-D errors [1] [2]
quantum efficiency [1] [2]
hysteresis [1] [2] [3]
R
RBI (residual bulk image)
radiation damage
READ
read noise [1] [2]
red leaks
UV filters [1] [2]
reference files
bias
dark
calibration
reference frame
FK4
FK5
relay optics
residual image
CTE trails
residual bulk image
resolution
S
SLTV ("thermal vacuum test")
SMOV ("Servicing Mission Observatory Verification")
SOFA (see "selectable optical filter assembly")
SAO catalog
scale
pixel scale
scattering
large angle
Selectable Optical Filter Assembly [1] [2]
serial clocks
Servicing Mission Observatory Verification
SHUTTER (header keyword)
shutter
shutter blade encoder disks
Si-SiO2 interface
signal-to-noise ratio (see also "SNR estimation")
sky background
sky flats
smearing
CCD artifacts
SNR estimation
aperture photometry
examples
aperture photometry
emission lines
extended sources
point source with galaxy
point sources
PSF fitting
SNR tables
extended sources
galaxies
point sources
plots
spacecraft computer ("NSSC-1")
spatial scans
spectral index
spherical aberration
correction [1] [2]
effects
standard stars (see name of individual star)