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: http://www.naic.edu/~astro/RXstatus/610.700/617.shtml
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610/700 MHz
Basic Information | Calibration & Beam Parameters RFI Situation Recent Events Receiver History Contact Info |
Frequency Range (GHz): |
(1) 607.6 - 611.8 MHz (HPW)* (2) 690.0 - 730.0 MHz
|
Name and Number:
610/700 MHz (610, 3)
|
Measured Sensitivity (K/Jy):
|
11 K/Jy*
|
Measured System Temp (K):
|
[102 + T(sky)] K* at 610 MHz
|
Native Polarization:
|
Linear
|
Beam Size (at 610 MHz):
|
7 x 8 arcmin
|
Available Filters:
|
click here |
|
2. Calibration & Beam Parameters:
Gain and Tsys | Cal Values | Beam Maps | Polarization | Misc. Info |
Only a single noise diode with a single intensity is available for this
receiver. This is denoted as "lcorcal", and gives measured temperature
steps of 42.49 K in Polarization A, and 41.09 in Polarization B for
linear polarization.
For detailed information on the magnitudes of the coma-lobe and
sidelobe
levels at 610 MHz, plus beam efficiencies, back to 01 May,
2001,
click here.
While the native polarization of the receiver is linear,
circular polarization can be produced using the 90-deg hybrid present
in the 10-GHz IF chain. If this is required, consult your Local
Friend.
BE WARNED that as there is only a "correlated"
calibration from the noise diode available with this receiver, the
"cal step" that results when using circular polarization with this
receiver is effectively unknown in degrees K.
To see an up-to-date plot of Tsys, just type tsys on your terminal after logging into Arecibo's computer network.
For detailed plots of the 610-MHz System Equivalent Flux Density (SEFD)
and
pointing
performance back to 01 May,
2001,
click
here .
The 610-MHz band is a protected band for radio astronomy between 608 and 614 MHz, (i.e. the purposely-vacant T.V. Channel 37). However, at Arecibo this band has historically suffered extreme RFI from out-of-band emissions originating from a nearby (spatially and in frequency) TV station. This is why the present relatively narrow-band filter is in the system at 610 MHz. It is hoped to obtain a wider-band filter in the near future to cover at least the complete protected band.
Daily RFI monitoring plots for the past several
years from the Observatory "hill-top" monitoring system can be found in
binders in either the telescope Control Room or by asking
the Arecibo Spectrum Manager.
For a full history of the 610-MHz receiver, click here.
For further information on this receiver, please contact Chris Salter at