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Several different types of spectrometers are/will be available at the SMTO:
- AOSs (Acousto-Optical Spectrometers)
- Filterbanks
- PI backends like the CHIRP.
Their characteristics are summarized in Table
1.4. The details of the spectrometers is discussed
further in Chapter 5.
Table 1.4:
SMTO Spectrometer Characteristics
Backend |
# Channels |
Res.[MHz] |
status |
AOSs |
|
|
|
MPIfR 1 GHz (AOS A) |
2048 |
1.021 |
online |
MPIfR 1 GHz (AOS B) |
2048 |
0.996 |
online |
MPIfR 250 MHz (AOS C) |
2048 |
0.4 |
online |
Filterbanks (FBS) |
|
|
|
256 MHz |
256 |
1.0 |
online |
64 MHz |
256 |
0.25 |
online |
8 MHz |
128 |
0.0625 |
online |
CHIRP |
|
|
|
3
180 MHz |
4100 |
0.044 |
expected late spring 2000 |
|
|
|
PI - Hofstadter |
|
Continuum data is processed with DRUMBEAT (Digital Recording Using
Multichannel Backend with AT), a 64 channel backend derived from
the Effelsberg 80-channel backend. See Chapter 3 for details.
The observer must tell OBST which backends to connect to which
frontends (see chapter 5). Various options
are possible, such as all backends going to one receiver or
having two backends attached to one receiver and the others
attached to a second receiver.
The software will keep track of the mode (line or continuum),
depending on the type of observation requested and use the appropiate
backend.
SMTO Manual Version 6.5, © May 2002, The SMTO Staff