Frequently Asked Questions (FAQ)
Using the Translator
How do I get started using the translator for my favorite spectrograph?
I have an instrument-specific translator question -or- I found a bug in an instrument translator. Who do I reach out to for help?
Translator Applications
Can I run a translator locally on my machine?
Can I use a translator for solar data? What about calibration data?
How does the translator handle different RV algorithms? What if, for example, I want a file that is a stellar template for template matching?
Adding a New Translator to the Data Standard
I want to develop a new instrument translator. How do I get started?
What does it mean to be compliant with the standard? E.g. Observatory required keywords vs Standard keywords
What version of Python should I be using? Is there Python version control?
The current data standard doesn’t accommodate a header keyword that is important for my instrument. What do I do?
Change Review Board
What is the Change Review Board?
How do I submit change requests for the data standard?
What is the process for assessing change requests?
How often are changes implemented?