VLBA Observational Status Summary 2018A

VLBA capabilities January 2018 - August 2018

1. Introduction, Older Versions of the OSS
2. New Developments
3. Antenna Sites
4. Frequency Bands & Performance
5. Station Signal Processing
   1. Primary Signal Path
   2. Frequency and Time Standard
   3. Calibration Signals
   4. Roach Digital Backend (RDBE)
   5. Programmable Network Switch
   6. Mark 5C Recorder
6. Correlator
   1. Introduction
   2. Spectral Resolution
   3. Integration Period
   4. Pulsar Gating and Binning
   5. Multiple Phase Centers
   6. Output Rate
7. Angular Resolution & u-v Coverage
8. Baseline Sensitivity
9. Image Sensitivity
10. Calibration Data
11. Amplitude Calibration
12. Phase Calibration & Imaging
    1. Fringe Finders
    2. The Pulse Cal System
    3. Fringe Fitting
    4. Editing
    5. Self-Calibration, Imaging, and Deconvolution
    6. Phase Referencing
13. Specialized Observational Techniques
    1. Polarimetry
    2. Spectral Line Observations
    3. Pulsar Observations
14. Extended "VLBA-Plus" Arrays
    1. Introduction
    2. The High Sensitivity Array (HSA)
    3. The Global 3mm VLBI Array (GMVA)
    4. The European VLBI Network (EVN) and Global cm VLBI
15. Proposal Preparation, Submission, & Review
16. Observation Preparation & Execution
17. Data Archive and Distribution
18. Post-Processing Software
19. References
20. Editor's Notes

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