VLBA Observational Status Summary 2019A

VLBA capabilities January 2019 - August 2019

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 & Mark 6 Recorders
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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