Details
-
Feature
-
Not Assigned
-
None
Description
Input data: Spectra (frequency vs amplitude)
Output data: Spectra with marked positions of peaks above a (defined?) threshold. CSV file of frequency, peak, FHWM.
Software involved: Basic Python libraries. Also could be a CNN workflow.
Workflow steps: Very basic: run a script to find peaks after the user has defined thresholds. Plot peaks on the spectra. Extended: Run a CNN to classify optical spectra.
State of existing workflows: Alex has a very simple script that finds peaks. Would be very easy to reproduce. Distributing the data and creating a workflow that searches would be a moderate amount of work. A more detailed (science-ready) workflow needs to be implemented for this in general - Shari. Alex once had students that developed a CNN that classified millions of optical spectra (sub categories of stars and galaxies)
Architecture and hardware: Multithreaded CPU. Minimal RAM. Data can be distributed.
Attachments
Issue Links
- relates to
-
SP-3496 Consolidate naming and structure of SRC example workflow repository
- Done