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SPA Headers

This section describes in alphabetical order the headers associated with SPA scans.

airm -
mean number of airmasses during observation (units=.01)
atten(2) -
atmospheric attenuation tex2html_wrap_inline1217 in 1 airmass (unit=0.001)
azlev -
az pointing correction from levels (units=.0001 deg)
azoff -
az offset from pointing correction thumbwheel (0.0001)
azsb -
subreflector azimuth angle
azs -
azimuth at start of observation
bcen -
galactic latitude of center of map
bw(4) -
bandwidth(mhz) of the four backends
b -
galactic latitude of reference pixel
calcon -
calibration constant ( degress k / volts )
calscan -
scan number of data used for calibration of y values
cfac -
sky dip calibration factor
dalp -
right ascension displacement in arcminutes
db -
galactic latitude displacement from bcen (degrees)
dchdin -
change in channel with index in row
ddec -
declination displacement from deco (units=1arcminute)
deccen -
dec of center of map
dece -
declination at epoch of reference pixel
decoff(2) -
offsets to offsource positions (units=1 min)
dewang -
array commanded dewar angle
dewcur -
array current dewar angle
dewinv -
array dewar invert flag
dewmode -
array dewar tracking mode
dfrdin -
change in frequency with index in row (GHz)
dfside -
frequency spacing between upper and lower sideband
distance -
equatorial coordinate distance on sky from racen,deccen (units=arcmin).
dl -
galactic longitude displacement from lcen (degrees)
dra -
right ascension displacement from rao (units=4sec)
dskydin -
change in sky coordinate with index in row
dveldin -
change in velocity with index in row
dx(32) -
x offset of array pixel from center of map in map coordinate system
dy(32) -
y offset of array pixel from center of map in map coordinate system
ellev -
el pointing correction from levels (units=.0001 deg)
eloff -
el offset from pointing correction thumbwheel (0.0001)
elsb -
subreflector elevation position
els -
elevation at start of observation
epoch -
year to which coordinates are precessed
etab(2) -
fraction of beam including sidelobes which falls in 1/2 degree disk on sky (unit=0.001)
fl -
rest frequency of line (GHz)
focus -
subreflector focus position
fr1 -
sky frequency in center of first reference band (GHz)
fr2 -
sky frequency in center of 2nd reference band (GHz)
fsrate -
fraction of observing time spent on the signal freq unit=0.001
fs -
sky frequency in center of signal band (GHz)
gain(16) -
relative gains of the 16 quarry elements
h2o -
partial pressure of water in .01 mm
harm -
number of harmonic
horn(32) -
quarry id numbers for 32 pixels of scan
ichbe(4) -
index in row where data for each possible spectrometer starts
in1 -
index in row where data starts
iscold -
original scan number of data ( used in sequence funct
isideb -
dsb/ssb calibration flag
kbe -
backend identifier of data in y array (if kbe = 1 to 4 only one backend is in y, if kbe=5 all backends)
khm -
lo above(=2,+lock) or below(=1,-lock) the phase lock
khorn -
reference pixel
klo -
local oscillator above (1=lsb) or below (2=usb) line
krecv -
identifier for receiver
ksr -
signal or reference band assumed for xin1 and dxdin ( 1=signal, 2=first reference, 3=2nd reference )
ktel -
identifier for telescope (1=fcrao, 2=kitt peak, 3=texas, 4=bonn, 5=haystack, 6=nrao, 7=areceibo)
kx -
nature of x coordinate xind1 and dxdind 0=channel, 1=vlsr, 2=vsun, 3=flsr, 4=fsky, 5=ra, 6=dec, 7=az, 8=el, 9=k )
ky -
nature of y coordinate ( 0=t, 1=t*, 2=tb, 3=tau, 4=column density, 5=s, 6=weight, 7=acf )
lcen -
galactic longitude of center of map
lenscan -
length of scan as recorded in directory lenscan = 1000 * nhd + ndt, where nhd and ndt are the number of 1024 byte records in the header and data areas respectively
l -
galactic longitude of reference pixel
mapsys -
map coordinate system and grid sample spacing 1st-digit: (1=az/el, 2=ra/dec, 3=l/b) 2nd-digit: (1=bw, 1=offset bw, 2= 1/2 bw, 3= hex, {4= 1/3 bw, 5= 1/4 bw)
message(6) -
message entered by data reducer
name(6) -
source name as entered by operator ( 12 letters )
nbe -
number of backends or number of seperate feeds in case this is a continuum observation
nchan(4) -
number of channels available for each pixel in the four possible backends or number of data points per feed
ndat -
the number of data values written on tape with this header
nhorn -
number of pixels within the scan
nin -
number of data entries ( 0 to 1024 )
nrept -
number of repetitions in the y array
nxcol -
number of columns in the array receiver
off(4) -
offsets(mhz) in sky frequency of the centers of the four backends
offscan(2) -
off source scan numbers( max of two) or y-data values which are offs if offscan <0.
oper -
telescope operator (two initials)
otype -
five digit code for type of observation 1st-digit: 0=correllator, 1=continuum, 2=filter bank, 3=filter + correllator 5=continuum series 2nd-digit: 0=observation, 1=calibration, 2=test 3rd-digit: 0=on, 1=off, 2=on-off=ps, 3=on-(off1+off2)/2=dps, 4=beam switch, 5=map, 6=five point, 7=skydip, 8=calibrate 4th-digit: 0=no load switch, 1=load switch 5th-digit: 0=no polarization switching, 1=pol sw
parang -
parallactic angle
point -
monitor of telescope drive and pointing errors
pol(4) -
feed polarization of data in the four backends (units=2e-04 radians, -1=left, -2=right circular)
polcmd(2) -
polarizer positions during polswitched observations
psrate -
position switch period (=on source time, units=0.01se
qcalcon(16) -
calibration constant for 16 quarry elements
qpol(16) -
position angle of the polarization of the 16 quarry elements in coordinate system used to track dewar angle (units=2e-04 radians, -1=left, -2=right circular)
qtint(32) -
integration time for 32 array pixels
qtsys(16,4) -
system temperatures for array pixels for
qxmax(32) -
line parameter xmax for 32 array pixels
qxmean(32) -
line parameter xmean for 32 array pixels
qxmerr(32) -
line parameter xmerr for 32 array pixels
qxsig(32) -
line parameter xsig for 32 array pixels
qxwerr(32) -
line parameter xwerr for 32 array pixels
qxwidth(32) -
line parameter xwidth for 32 array pixels
qyint(32) -
line parameter yint for 32 array pixels
qymax(32) -
line parameter ymax for 32 array pixels
qysig(32) -
rms error of array pixel
qyterr(32) -
line parameter yterr for 32 array pixels
racen -
ra of center of the map
rae -
right ascension at epoch of reference pixel
raoff(2) -
offsets to offsource positions (units=4sec of time)
resin -
x coordinate resolution in terms of indice
rgain(8) -
relative receiver gains referenced to best one
rotang -
map rotation angle
rx -
free location for mapping coordinates
scale(8) -
additional scale factors not included above (units= 0.001 )
scan -
scan number ( 500 to 30000)
smark(2) -
standard marker within the scan which contains spa rev
spill(2) -
fraction of beam directed skyward(units=0.001)
stype -
five digit code for type of spectral line observation 1st-digit: ( 0=total power, 1=frequency switching, 2=double frequency switching ) 2nd-digit: ( 0=series, 1=parallel )
tatm -
assumed atmospheric temperature used in sky dip
tcal(8) -
cal temperatures( units=0.05k )
temp(1) -
outside air temperature at beginning of scan ( unit=0.1k for all these temperatures )
temp(2,3) -
dewpoints inside and outside dome
temp(4) -
average temperature on radome
temp(5) -
average temperature on antenna surface
temp(6) -
maximum temperature on surface
temp(7) -
minimum temperature on surface
tgain(2) -
telescope gain in forward direction at center of main beam( units=0.001 )
tint -
integration time(sec)
tpave -
total power dvm reading averaged over observation
tpdev -
max percentage deviation of tp from tpave(unit=.01
ts(8) -
system temperature (units=1k)
tsid -
sidereal time at start of observation
utd -
mean universal time date
vcal(2) -
dual channel contiuum v/f calibration constants
vclsr -
velocity correction to lsr s.t. vtotal=vlsr+vclsr
vcsun -
velocity correction to heliocentric as for lsr
vlsr -
center velocity used when observation was made
xch1 -
channel number of in1
xfr1 -
frequency of in1 (GHz)
xlabel -
x-axis label (8 characters )
xmax -
channel, vleocity, or frequency(GHz) for ymax
xmean -
mean channel, velocity, or frequency(GHz) from line measuring function. In the case of a continuum mapping observation, this parameter and the ones which follow are the parameters of the gaussian fit.
xmerr -
formal error to mean channel, velocity, or frequency (GHz) from line function
xoff(16) -
x offset of the 16 quarry elements in quarry coordinates (units=1e-4 degrees)
xsigma -
sigma(width) in channel, velocity, or frequency(GHz)
xsky1 -
sky coordinate of in1 (used during mapping )
xtype -
three digit code specifying types of x coords in header variables xvel1, dvdin, xfr1, dfrdin, and xsky1, dskydin 1st-digit: ( 0=vlsr, 1=vsun ) 2nd-digit: ( 0=flsr, 1=fsky ) 3rd-digit: (0=ra, 1=dec, 2=az, 3=el, 4=none of the
xvel1 -
velocity of in1
xwerr -
formal error to xwidth from line function
xwidth -
full width in x to first crossing to y >ymax/2
yint -
integrated y values from line measuring function
ylabel -
y-axis label (8 characters )
ymax -
maximum y value from line measuring function
yoff(16) -
y offset of the 16 quarry elements in quarry coordinates (units=1e-4 degrees)
ysb -
subreflector y axis lvdt
ysigma -
rms noise in spectra measured by baseline or wave
ysky -
continuum raster map y offset
yterr -
formal error to integrated y values from line function


next up previous contents
Next: SPA Functions Up: SPA User's Manual Previous: MSDOS SPA

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Tue May 14 18:00:20 EDT 1996