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Backends
The following four spectral line backends are available which can be
individually connected to any single pixel receiver and, if indicated,
also to HERA.
The 1 MHz filterbank consists of 4 units. Each unit has 256
channels with 1 MHz spacing and can be connected to different or
the same receivers giving bandwidths
between 256 MHz and 1024 MHz. The maximum bandwidth is available
for only one receiver, naturally one having a 1 GHz wide IF bandwidth.
Connection of the filterbank in the 1 GHz mode presently excludes the
use of any other backend with the same receiver.
Other configurations of the 1 MHz filterbank include
a setup in 2 units of 512 MHz connected to two different receivers, or 4 units
of 256 MHz width connected to up to four (not necessarily) different receivers.
Each unit can be shifted in steps of 32 MHz relative to the center frequency
of the connected receiver.
The 100 kHz filterbank consists of 256 channels of 100 kHz spacing.
It can be split into two halves, each movable inside the 500 MHz IF
bandwidth, and connectable to two different single pixel receivers
(must be set up in narrow band mode).
VESPA, the versatile spectrometric and polarimetric array,
can be connected either to HERA or to a subset of 4 single pixel receivers,
or to a pair of single pixel receivers for polarimetry.
The many VESPA configurations and user modes are summarized in a
Newsletter contribution
[14] and in a
user guide,
but are best visualised on a demonstration program which can be downloaded
from our web page
at URL ../IRAMFR/PV/veleta.htm.
Connected to a set of 4 single pixel receivers VESPA typically provides up to
12000 spectral channels (on average 3000 per receiver).
Up to 18000 channels are possible in special
configurations. Nominal spectral resolutions range from 3.3 kHz
to 1.25 MHz. Nominal bandwidths are in the range 10 -- 512 MHz.
When VESPA is connected to HERA, up to 18000 spectral channels can be used
with the following typical combinations
of nominal resolution (kHz) and maximum bandwidth (MHz):
20/40, 40/80, 80/160, 320/320, 1250/640.
The 4 MHz filterbank consists of nine units.
Each unit has 256 channels (spacing of 4 MHz, spectral resolution at 3 dB
is 6.2 MHz) and thus covers a total bandwidth of 1 GHz.
The 9 units are designed for connection to HERA, but a subset of 4 units
can also be connected to the backend distribution box which feeds
the single pixel spectral line receivers. All these receivers have a 1 GHz RF
bandwidth except for A100 and B100 (500 MHz only).
At the present time, a 4 MHz filterbank cannot be used simultaneously with
the autocorrelator or the 100 kHz filterbank on the same receiver.
The wideband autocorrelator WILMA consists of 18 units. They can
be connected to the 18 detectors of HERA. Each unit provides 512
spectral channels, spaced
out by 2 MHz and thus covering a total bandwidth of 1 GHz. Each band is sliced
into two 500 MHz subbands which are digitized with 2 bit/1 GHz samplers.
An informative technical overview of the architecture is
available at URL
../IRAMFR/TA/backend/veleta/wilma/index.htm.
Note that WILMA cannot presently be connected to any of the
single pixel receivers.
Next: Bibliography
Up: Call for Observing Proposals
Previous: Wobbling Secondary
Clemens Thum
2006-07-07