cband calibration
aug,2002
The cband receiver covers 3.95 to 6.05
Ghz.
It is a native linear receiver with the option to create circulars
using
a hybrid in the iflo cabinets.
Sections:
History
Recent
system performance measurements
Daily
monitoring of Tsys
Dewar
temperatures
Calibration measurements
Miscellaneous
cal values
History:
- 01nov10-17nov10
- : gortex cover comes loose, moisture gets into mouth of horn.
- Tsys goes up. repaired and back to normal on 17nov10.
- 28aug06: new cband
cal values installed (measured back in jul06).
- 06jul06: remeausured the cal values. Needed from the 25may06
tightening
of pola.
- 25may06: Found that sma connector for polA cal was loose. Cal had
jumped
back on 02feb06. After tightening, the Tsys did not jump back to the
pre
02feb06 value. So tightening changed the amount of cal that was getting
in before the jump.
- 02feb06: cal polA jumped (turned out to be loose sma connector
for cal).
- 10jun05: cal values measured using sky and absorber. backdated to
25may05
- 25may05: new amplifiers installed in cband receiver.
- 24may04 to 08oct04 pola tsys jumping around.. a bias line for the
led's
inside the dewar was shorting out.
- 16may03: cal values measured using sky and absorber. back dated
to
05may03.
- 05may03 cal cable tightened.
- 22apr03 new cal diodes installed.
- 28aug02 horn moved down 1.08" to put phase center at the correct
position.
- 22jan01: cal values measured using sky and absorber.
Calibration
measurements:
02jul09:
tsys vs freq for entire band.
may05-oct05: cband GAIN CURVES.
may05-oct05: System
performance
of data used for gain curves.
may03-mar04: cband GAIN CURVES.
may03-mar04: System
performance
of data used for gain curves.
Aug02-Dec02:
cband
GAIN CURVES.
aug02-dec02:
System performance: Gain,Tsys,Sefd.. using calibration runs.
08aug02:
horn moved down 1.08" to put phase center at focus.
sep01-aug02: cband
GAIN CURVES.
sep01-aug02:
System performance:Gain,Tsys,Sefd... using calibration runs.
22dec01:
cband sefd,pointing errors (preview)
02aug01:
gain/sefd after panels in the northern half of the dish adjusted
28jun01:
gain/sefd on 3C48 after SE quad of dish adjusted
27jun01:
gain/sefd with pitch,roll,focus correction after SE quad adjusted
jan01: calibration after 1st surface adjustment
sep00: calibration runs
Miscellaneous:
09feb11: look at
cband,iflo stability with the shutter closed.
19nov10: Tsys increases when horn gortex fabric
cover comes loose.
27sep04: oscillations/jumping around of
Tsys
in polA
29jul02:
resonances in the cband omt 29jul0
07jun02:
Polarized Tsys vs azimuth,za
19Nov10: Tsys increases when horn gortex
fabric cover
comes loose.
Tsys for the cband receiver increased from 30oct10
(polA 26K) to 13nov10 (polA 38K). It then decreased back to 26 K on
19nov10. After inspecting the feed it was found that the gortex fabric
horn cover had come loose. Water drops were found inside the horn. The
change in tsys was probably a function of how much water precipitated
on the the inside of the Horn. This would be a function of the horn
temperature and the dewpoint.
The top of the reciever is inside the gregorian dome
room which is air conditioned. The bottom part of the receiver
and the horn are under the rotary floor. This part is not air
conditioned.
The plots show the
Tsys and gain variations for this period (.ps) (.pdf):
- Page 1: Tsys vs data for Cband at 5Ghz
- black is polA, red is polb.
- Each minor tick mark is 5 days.
- There is some jumping around around 30oct10 to 04nov10
- It starts the steady increase on 07nov10 peaking on
12nov10 at polA=41.4K
- It decreases back to 25-26K on 19nov10.
- On 19nov10 the cover was placed back on the horn (after
cleaning out the water droplets).
- Page 2: cband calibration runs: 17oct,15nov,16nov10.
- The dates are color coded
- top: the gains for individual sources are not changing between
the dates.
- 2nd: Tsys vs za. the 17oct10 data is about 10k less that the
15,16Nov data.
- 3rd: SEFD: For the same source,the 16nov data is greater than
the 17oct10 data by the same amount that Tsys has increased. This shows
that the problem was really with the Tsys and not a change in the cal
values.
Summary:
- The gortex fabric cover coming loose at the mouth of the horn
caused Tsys to increase by up to 25%.
- The increase, decrease of Tsys was probably a function of the
horn temperature and the dew point.
- The receiver has shown other periods where the Tsys has increased
and then decreased. It would be interesting to correlate this with the
gregorian room temperature and the outside air dew point. It may be
that the cover had been loose for awhile.
processing: x101/101119/cbandTsys.pro
May05 to
oct05
fit GAIN CURVES to calib data. (top)
On 25may05 new amplifiers were installed in the
cband
dewar. Calibration data was then taken from 25may05 through 31oct05
(see
the
cband gain data ). Gain curves were then fit to the data. The
gain curves were installed in the system 22nov05.
The functional form used was:
gain= c0 + c1*(za-10) + c2*(za-10)^2 +
c3*(za-10)^3
Curves were fit separately to the frequencies:
4100,4400,4500,4700,4860,5000,5400,5690,
and 5900 Mhz. There were a total of 1774 points over the 9 frequencies
(average of 200 pnts/freq). There was no attempt to fit to the azimuth
dependence because of a lack of azimuth coverage.
The plots
show the gain data (black) and the fits (red) (.ps) (.pdf)
for the various frequencies:
- Fig 1 shows the az,za distribution for the data. This includes
all of
the
frequencies.
- Figs 2,3,4 plots the gain data and the fit to za. The freq,
fit
sigma,
and fit equation are printed below the plots.
- Figs 5,6,7 plot the fit residuals (data-fit) vs za.
The routine gainget() or corhgainget() will now
return
the cband gain for data after 25may05 from these equations. The
coefficients
can be found in the ascii file data/gain.datR9 (this is provided
in the AO
idl distribution for correlator routines). You can also find a copy
of it at AO in /pkg/rsi/local/libao/phil/data/gain.datR9.
processing: x101/cb/may05/dogainfit.pro
May05 thru oct05 :
System
performance data used to compute gain curves. (top)
Heiles calibration scans done from
25may05
(after the new amps were installed) thru 31oct05 were used to measure
the
system performance. This data was then used to compute the gain curves
for data taken after 25may05.
The first set of plots show the system
performance with all frequencies over plotted (.ps) (.pdf).
The sources are identified by symbol and the frequencies by color.
- Fig 1 shows the distributions on the dish of the measurements.
- Fig 2: Each frequency is in a different color. Symbols
differentiate
sources.
- Top: the Gain in Kelvins/Jansky.
- 2nd: Tsys in Kelvins
- 3rd: System Equivalent Flux Density (SEFD) in Jy. This is
the
size
of a source needed to equal the system temperature. The SEFD does not
depend
on the cal value (Tsys/Gain).
- Bottom: The average beam width in arc seconds.
- Fig 3 plots the coma parameter, first sidelobe height below the
peak,
the
main beam efficiency, followed by the main beam + 1st sidelobe beam
efficiency.
The coma parameter measures the asymmetry in the gaussian beam.
- Fig 3 has the pointing errors in az,za each plotted versus az and
za.
Color is used to identify different sources.
The second set of plots has the
system performance plotted separately for each frequency (.ps) (.pdf).
The figures are:
Fig 1 4100 Mhz Gain,Tsys,sefd,bmwid. 105 points
Fig 2 4100 Mhz coma,sidelobes, beam efficiencies
Fig 3 4400 Mhz Gain,Tsys,sefd,bmwid. 106 points
Fig 4 4400 Mhz coma,sidelobes, beam efficiencies
Fig 5 4500 Mhz Gain,Tsys,sefd,bmwid. 244 points
Fig 6 4500 Mhz coma,sidelobes, beam efficiencies
Fig 7 4700 Mhz Gain,Tsys,sefd,bmwid. 106 points
Fig 8 4700 Mhz coma,sidelobes, beam efficiencies
Fig 1 4860 Mhz Gain,Tsys,sefd,bmwid. 242 points
Fig 2 4860 Mhz coma,sidelobes, beam efficiencies
Fig 1 5000 Mhz Gain,Tsys,sefd,bmwid. 447 points. The source
B1645+174
looks
like it has a bad cal value. The gain is high, the Tsys is high, but
the
sefd was normal.
Fig 2 5000 Mhz coma,sidelobes, beam efficiencies
Fig 1 5400 Mhz Gain,Tsys,sefd,bmwid. 341 points
Fig 2 5400 Mhz coma,sidelobes, beam efficiencies
Fig 1 5690 Mhz Gain,Tsys,sefd,bmwid. 98 points
Fig 2 5690 Mhz coma,sidelobes, beam efficiencies
Fig 1 5900 Mhz Gain,Tsys,sefd,bmwid. 98 points
Fig 2 5900 Mhz coma,sidelobes, beam efficiencies
processing: x101/cb/may05/doit.pro
27sep04
oscillations/jumping
of tsys in polA. (top)
The system temperature for polA has been
jumping around. On 24 sep04 data was taken with the radar interface
(ri). 40 Mhz around 4850 Mhz was detected with a 20 usecond time
constant and sampled at 10 useconds. 90 seconds of data was taken. The
plots show
the variations in pola.
- The top plot shows the total power time series. It has been
smoothed to
10 milliseconds. The black plot is polA while the blue plot is polB.
The
y axis units are Tsys. You can see that polA is jumping around a lot
more
than polb.
- The bottom plot is the magnitude of the spectrum of the time
series
(over
the entire 90 seconds). The first 20 hz of the spectrum is plotted. The
dashed green lines are placed every 1.2 hz. The spectrum has power at
harmonics
of this frequency.
The 1.2 hz power is probably coming from the
refrigerator
for the dewar. Somehow it is modulating the gain at this period. This
is
probably the culprit for the jumps in Tsys in polA.
note: When the dewar was brought down to the lab, one of the
cables in the dewar had lost its insulation and was intermitantly
shorting out. It may have been that the vibration of the refrigerator
caused
the cable to short.
processing: x101/040924/doit.pro
May03 to
Mar04
fit GAIN CURVES to calib data. (top)
link
to gain curve plot
Gain curves were fit to the
cband gain data from 05may03 through 29feb04. On 05may03
new
cals were installed and the cal cable was tightened. This data is
described
below.The plots
show the gain data (black) and the fits (red) for 4500, 4860,
5000,
5400,5690, and 5900 Mhz. These gain equations were installed on
08mar04.
- Fig 1 shows the az,za distribution for the data. The fit used a
3rd
order
polynomial in (za-10) and 1az, 2az, and 3az sin, cos terms.
- Fig 2,3 plots the gain data and the fit to za. The fit
equation
is
plotted with the sigma for the fit (in K/Jy). T
- Fig 4,5 plots the fit residuals (data-fit) vs za.
The only puzzling thing is that the gainfits for 4500Mhz and 4860 Mhz
are
almost identical..
The routine gainget() or corhgainget() will now
return
the cband gain for data after 05may03 from these equations. The
coefficients
can be found in the ascii file data/gain.datR9 (this is provided
in the AO
idl distribution for correlator routines). You can also find a copy
of it at AO in /home/phil/idl/data/gain.datR9.
processing: x101/cb/may03/dogainfit.pro
may03 thru feb04 :
System
performance data used to compute gain curves. (top)
Heiles calibration scans done from 05may03
(after
the cals installed) thru 29feb04 were used to measure the system
performance. This data was then used to compute the gain curves used
after
05may03.
The first set of plots show the system
performance with all frequencies overplotted. The sources are
identified
by symbol and the frequencies by color.
Fig 1 shows the distributions on the dish of the measurements.
Fig 2 has the Gain in Kelvins/Jansky. This relies on the cals and
the
source
flux. Ths next plot is Tsys vs za in Kelvins followed by the
SEFD
(System Equivalent Flux density) in Janskies / Tsys. At the bottom is
the
average beam width in arc seconds.
Fig 3 plots the coma parameter, first sidelobe height below the
peak,
the
main beam efficiency, followed by the main beam + 1st sidelobe beam
efficiency.
Fig 3 has the pointing errors in az,za, and total (added in
quadrature)
for the data.
The second set of plots has the
data plotted separately for each frequency. The colors and symbols
are used to differentiate the sources. The figures are:
Fig 1 4500 Mhz Gain,Tsys . 275 points
Fig 2 4500 Mhz sidelobes,beam efficiencies
Fig 3 4860 Mhz Gain,Tsys 275 points.
Fig 4 4860 Mhz sidelobes,beam efficiencies.
Fig 5 5000 Mhz Gain,Tsys 567 points.
Fig 6 5000 Mhz sidelobes,beam efficiencies
Fig 7 5400 Mhz Gain,Tsys 566 points.
Fig 8 5400 Mhz sidelobes,beam efficiencies
Fig 9 5690 Mhz Gain,Tsys 292 points.
Fig 10 5690 Mhz sidelobes,beam efficiencies
Fig 11 5900 Mhz Gain,Tsys 292 points.
Fig 12 5900 Mhz sidelobes,beam efficiencies
Use the second set of plots to identify the sources.
processing: x101/cb/may03/doit.pro
Aug02
to Dec02 fit GAIN CURVES to calib data. (top)
link
to gain curve plot
Gain curves were fit to the
cband gain data from 28aug02 (after horn focus change) to 30nov02.
This data is described below.The plots
show the gain data (black) and the fits (red) for 4500, 4860,
5000,
and 5400 Mhz.
- Fig 1 shows the az,za distribution for the data. The fit used a
3rd
order
polynomial in (za-10) and 1az, 2az, and 3az sin, cos terms.
- Fig 2 plots the gain data and the fit to za. The fit
equation is
plotted with the sigma for the fit (in K/Jy). T
- Fig 3 plots the fit residuals (data-fit) vs za.
The routine gainget() or corhgainget() will now
return
the cband gain for data after 28aug02 from these equations. The
coefficients
can be found in the ascii file data/gain.datR9 (this is provided
in the AO
idl distribution for correlator routines). You can also find a copy
of it at AO in /home/phil/idl/data/gain.datR9.
processing: x101/cb/dec02/dogainfit.pro
aug02-dec02: System
performance:Gain,Tsys,Sefd...
using calibration runs. (top)
Heiles calibration scans done from 28aug02
(after
the horn focus) were used to show the system performance after the horn
focus.
The first set of plots show the system
performance with all frequencies overplotted. The sources are
identified
by symbol and the frequencies by color.
Fig 1 shows the distributions on the dish of the measurements.
Fig 2 has the Gain in Kelvins/Jansky. This relies on the cals and
the
source
flux. Ths next plot is Tsys vs za in Kelvins followed by the
SEFD
(System Equivalent Flux density) in Janskies / Tsys. At the bottom is
the
average beam width in arc seconds.
Fig 3 plots the coma parameter, first sidelobe height below the
peak,
the
main beam efficiency, followed by the main beam + 1st sidelobe beam
efficiency.
Fig 3 has the pointing errors in az,za, and total (added in
quadrature)
for the data.
The second set of plots has the
data plotted separately for each frequency. The colors and symbols
are used to differentiate the sources. The figures are:
Fig 1 4500 Mhz Gain,Tsys 241points.
Fig 2 4500 Mhz sidelobes,beam efficiencies
Fig 3 4860 Mhz Gain,Tsys 245 points.
Fig 4 4860 Mhz sidelobes,beam efficiencies.
Fig 5 5000 Mhz Gain,Tsys 279 points.
Fig 6 5000 Mhz sidelobes,beam efficiencies
Fig 7 5400 Mhz Gain,Tsys 273 points.
Fig 8 5400 Mhz sidelobes,beam efficiencies
Fig 9 5690 Mhz Gain,Tsys 35 points.
Fig 10 5690 Mhz sidelobes,beam efficiencies
Fig 11 5900 Mhz Gain,Tsys 35 points.
Fig 12 5900 Mhz sidelobes,beam efficiencies
Use the second set of plots to identify the sources.
processing: x101/cb/dec02/doit.pro
28aug02 horn moved down
1.08"
to put phase center at focus. (top)
link to new
plot:
system performance before and after the horn move.
The cband horn was lowered 1.08" toward the
tertiary
to place the phase center at the focus (this is explained on the lband
focus change page). The source J0738+177 was tracked on 26aug02
before
the horn was moved and then again on 28aug02 after the horn
positioning.
The plots
show
the results of the focus change.
- Fig 1 shows the gain (K/Jy) before (black) and after (red). The
absolute
gain values depends on the source flux and the cal. The relative change
does not rely on these values. The lower plot shows the relative change
in gain (after-before)/before.
- Fig 2 has the gain, Tsys, Sefd, and average beam width for before
and
after.
- Fig 3 plots the coma, 1st sidelobe level, main beam efficiency,
and
mainbeam
+1st sidelobe efficiency.
- Fig 4 is the pointing error for this source before and after.
- Fig 5 plots the change in pointing error before and after.
Above 8 degrees za the gain improved. Below 6
degrees
it degraded. The za pointing error for the source setting is up to 25
asecs.
The change in pointing because of the move was up to 10 asecs for
rising
azimuth.
The focus
curves done by moving the platform (bottom plot. cband is
bright
red color) show that the cband horn was in focus (platform
height=1256.35
feet) at za=5 degrees. Below za=5 the platform focused higher (the ray
path is too short) while for za > 5 the platform was focusing below
1256.35
(the ray path is too long). Making the ray path shorter by 1 " should
have
hurt the gain below za=5 and helped it above za=5.
The model
of the focus height using AO9 as the reference agrees with the
platform
focus curves and the data we took here. The model
of the focus height with the reflector at the origin (about 2"
difference
in focus) does not.
sep01 to
27aug02 fit GAIN CURVES to calib data. (top)
link
to gain curve plot
Gain curves were fit to the
cband gain data from 01sep01 (after dish adjusted) to 27aug02
(before
horn focus changed). This data is described below.The plots
show the gain data (black) and the fits (red) for 4500, 4860,
5000,
and 5400 Mhz.
- Fig 1 shows the az,za distribution for the data. Because of the
incomplete
az coverage, the fit was only done to za.
- Fig 2 plots the gain data and the fit to za. The fit
equation is
plotted with the sigma for the fit (in K/Jy). The quadratic and cubic
terms
of the fit should only be used for za >= 14 degrees.
- Fig 3 plots the fit residuals (data-fit) vs za.
The routine gainget() or corhgainget() will now
return
the cband gain for data after 01sep01. The coefficients can be found in
the ascii file data/gain.datR9 (this is provided in the AO
idl distribution for correlator routines). You can also find a copy
of it at AO in /home/phil/idl/data/gain.datR9.
processing: x101/cb/aug02/dogainfit.pro
sep01-aug02:
System performance:Gain,Tsys,Sefd... using calibration runs. (top)
All of the heiles calibration scans sept01 to aug02
for the cband receiver were used to plot the system performance. This
includes
dedicated calibration runs and individual calibration scans done by
observers.
Scans with pointing errors greater than 30 Asecs, extended sources,
tsys
greater than 46K, or uncertain flux at 5 Ghz were not used. This data
was
taken under differing weather conditions. After the above selection,
there
were 1697 points (all frequencies) and 30 different sources.
The first set of plots show the system
performance with all frequencies overplotted. The sources are
identified
by symbol and the frequencies by color.
Fig 1 has the Gain in Kelvins/Jansky. This relies on the cals and
the source
flux. Ths next plot is Tsys vs za in Kelvins followed by the
SEFD
(System Equivalent Flux density) in Janskies / Tsys. At the bottom is
the
average beam width in arc seconds.
Fig 2 plots the coma parameter, first sidelobe height below the
peak,
the
main beam efficiency, followed by the main beam + 1st sidelobe beam
efficiency.
Fig 3 has the pointing errors in az,za, and total (added in
quadrature)
for the data.
The second set of plots has the
data plotted separately for each frequency. The colors and symbols
are used to differentiate the sources. The figures are:
Fig 1 4500 Mhz Gain,Tsys 355 points.
Fig 2 4500 Mhz sidelobes,beam efficiencies
Fig 3 4860 Mhz Gain,Tsys 353 points.
Fig 4 4860 Mhz sidelobes,beam efficiencies.
Fig 5 5000 Mhz Gain,Tsys 427 points.
Fig 6 5000 Mhz sidelobes,beam efficiencies
Fig 7 5400 Mhz Gain,Tsys 420 points.
Fig 8 5400 Mhz sidelobes,beam efficiencies
Fig 9 5600 Mhz Gain,Tsys 71 points.
Fig 10 5600 Mhz sidelobes,beam efficiencies
Fig 11 5900 Mhz Gain,Tsys 71 points.
Fig 12 5900 Mhz sidelobes,beam efficiencies
Use the second set of plots to identify the sources.
processing: x101/cb/aug02/doit.pro
22dec01: sefd,
pointing
errors. (top)
A calibration run was done on 22dec01 using the
heiles
scans. The plots
show the sefd and pointing errors. A more detailed analysis of this
data is included in the sep01 to aug02
system
performance.
home_~phil