CSIRO Astronomy and Space Science
ATCA Users Guide
Preface
this Guide
Conventions
(1) The Australia Telescope Compact Array
/1./The Australia Telescope Compact Array
/1.1/The Australia Telescope National Facility
/1.2/Overview of the ATCA
/1.3/Centimetre Observations (16–3 cm bands)
/1.4/Millimetre-wave observations (15mm–3mm)
/1.5/Choosing an Observing Frequency
/1.6/Choosing Angular and Frequency Resolution
/1.7/Additional Observing Notes and Techniques
/1.8/High Time Resolution, Pulsars, Planets and VLBI
/1.9/Other Things to Consider
/1.10/Submitting a proposal
/1.11/Successful Proposals
(2) Preparing for Observations
/2./Preparing for Observations
/2.1/Scheduling Strategy
/2.2/Calibration Requirements
/2.3/How to Prepare a Schedule File
/2.4/How to Prepare a Mosaic File
/2.5/Observation Requirements
/2.6/Pre-observation Checklist
(3) Observing
/3./Observing
/3.1/Changeover
/3.2/Setting up
/3.3/Observing
/3.4/Troubleshooting
/3.5/cm Observing Startup Checklist
/3.6/mm Observing Startup Checklist
(4) After your Observations
/4./After your Observations
/4.1/Archiving Your Data
/4.2/Report Your Experiences
/4.3/Data Analysis
/4.4/Publishing Results
(A) caobs reference
/A./caobs reference
/A.1/Using caobs
(B) cacor reference
/B./cacor reference
/B.1/Cacor Status Panel
/B.2/Cacor Data Panel
/B.3/Cacor Timing Panel
/B.4/Cacor Log Panel
/B.5/Cacor Command Panel
/B.6/Cacor Commands
(C) SPD reference
/C./SPD reference
/C.1/Introduction to SPD
/C.2/SPD Commands
(D) vis
/D./vis
/D.1/VIS Commands
(E) Web Scheduler
/E./Web Scheduler
/E.1/Scheduler Fields
/E.2/Scheduler Actions
(F) Observatory Coordinates
/F./Observatory Coordinates
/F.1/Site Location
/F.2/Station Locations
(G) ATCA Configurations
/G./ATCA Configurations
/G.1/Array Configurations
/G.2/Shadowing Diagrams
(H) People to contact
/H./People to contact
Index
[Printable Guide] [Printable Chapter]

C.1 Introduction to SPD

The SPD (Spectra Display) program displays data from the ATNF correlators/spectrometers, either in the lag domain - the correlation function, as measured directly by a correlator - or in the frequency domain - the spectrum which results from the Fourier transform of the correlation function in the case of a correlator, or from direct measurement in the case of a spectrometer. The user can select which of the products contained within the correlator/spectrometer configuration to display and in what form to display them.

SPD can also display time bin profiles and time bin images for correlator/spectrometer configurations which provide time or pulsar binning. In the case of pulsar binning, the de-dispersed pulsar bin profile can be displayed.

Note: For the correlation function, the default action is to display only that part of the function which is actually measured in the correlator. For autocorrelations, this will generally be only be the positive lags. If negative lags are requested for autocorrelations with the ’lags’ command, the positive lag measurements are mirrored into the negative lags for display.


Users Guide last modified on 2011-04-27 15:49:06