The Dwingeloo Radio Telescope
Audience: Operators and users of the Dwingeloo Radio Telescope
Purpose: To explain how to observe with the Dwingeloo Radio Telescope
Tony Foley
Introduction
The scope of this Document
A brief description of the Dwingeloo telescope
Frontends
Backends
Control
Hardware
Computer
Multiplexer
Correlator
Configurations
Bandwidth codes
Correlator modes
IF and A/D conversion
Receivers
21cm
Mixing scheme
18cm
Frontend
Mixing scheme
Motors and antenna limits
Limits
Dish surface and antenna gain
Clocks
Observing modes
Correlator modes
Single-bit
Two-bit
Split mode
Frequency switching
Position switching
Grid modes
RA/dec (apparent)
Galactic l/b
RA/dec (epoch B1950)
HA/dec
Azimuth/elevation
Scan mode
Track mode
Pointing mode
Nonstandard modes
Software
Schedule format
Bit options (Phase 1)
Letter codes (input phase 2)
Telescope parameters (input phase 3)
Operational software
Online software
Offline programs
Test software
Output files
Reduction software
Procedures
What to log
Daily check routine
Checking current observing status
Checking total power levels
Checking system temperature
Checking the clocks
Resetting the UT clock
At year change
Checking the synthesizer
Checking the multiplexer
Checking the correlator
Checking spectra
Stopping an observation
Moving the telescope for receiver change
What to do in case of storm
When to do this
Procedure
After a storm
Pointing the telescope by hand
Loading a schedule
Saving the data
Resetting the HP2621A terminal
Applying for observing time
Calibration Sources
Flux calibrators
Spectral line calibrators
Correction tables
Example schedule
References
NFRA ITRs
NFRA Notes
Others
RTE operating system
General
Dwingeloo-specific
Handleiding bij Storm
Program Index
Concepts Index
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