EVLA/VLBA/GBT Resources
NRAO Interactive Services Modification Request 2 T1 2010
1. Introduction
Any changes to the telescope specific resources
2. Background
3. Requirements
- EVLA
- We will either add the 74 MHz receiver for a special release (after June 1 deadline) or for the Oct 1 release.
- VLBA
- GBT
- GUPPI backend:
- Add an option to choose between "Coherent Dedispersion" and "Incoherent Dedispersion".
- Add K-band focal plane array (KFPA) as a new receiver. Call it "KFPA (shared risk)" in the menu.
- When selected only the Spectrometer backend should be available.
- Keep the following: Rest Frequencies, Sampling Level, and Desired Frequency Resolution
- Add the table below. Here are the constraints:
- The number of frequencies should match the number of spectral windows, except for when the number of beams is 7 whereby the user can input either the number of spectral windows or the number of spectral windows plus 1.
- The widest frequency separation is 1800 MHz.
- The sampling level works the same way as usual: if the bandwidth is either 200 MHz or 800 MHz then only 3-level is available, but if the bandwidth is either 12.5 MHz or 50 MHz then the user can choose either 3-level or 9-level.
4. Design
Technical lead should provide a brief description of how this will be implemented in the code.
5. Deployment Checklist
Documentation? Systems/hardware/networking things needed for deployment?
6. Test Plan
6.1 Internal Testing
6.3 Integration/Regression Tests
Signatures
APPROVED: I acknowledge that my request is fully contained in this MR, and if the Open Sky (or other NIS or PST developers) deliver exactly what I specified, I will be happy.
ACCEPTED: I acknowledge that I have validated the completed code according to the acceptance tests, and I am happy with the results.
Written |
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Checked |
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Approved by Scientific Sponsor |
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Accepted/Delivered by Sponsor |
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Discussion Area
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DanaBalser - 2010-02-18