Comments (1)
Hey Yuting!
So everything you're wanting should be relatively straightforward, given some forking and javascript work.
- You can increase the redshift accuracy by increasing the binning of the templates/input spectra by increasing the arraySize here: https://github.com/Samreay/Marz/blob/gh-pages/js/config.js#L62
- If you're looking at things in a lower redshift range, note that the startPower and endPower defined above the arraySize will determine the redshift range your xcors go to, so you could reduce the maximum wavelength if you're not needing higher redshift results.
- You can scrap templates and add your own simpy by editing https://github.com/Samreay/Marz/blob/gh-pages/js/templates.js
- In terms of redshift error, we found that usnig the width of the xcor peaks was not representative of the actual redshift error, and thats why its not used.
- But... if you want to do it anyway, the each spectra class has the xcor data stored in templateResults: https://github.com/Samreay/Marz/blob/gh-pages/js/classes.js#L77, where each template result is a dictionary of redshifts, xcor values, and the template weight (https://github.com/Samreay/Marz/blob/gh-pages/js/workerMethods.js#L256)
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Related Issues (20)
- Issue with some templates HOT 2
- Handle commas in comments HOT 11
- Issue with some templates, z = NaN HOT 2
- Scaling options
- Marz provides no feedback when loading results from previous versions in. HOT 14
- Merging feature request: more clearly label priorities of each redshifter
- Merging feature request: Default to default redshifter redshift
- Merging comments from from other redshifters
- "Previous" shotcut for best fit templates HOT 2
- Key bindings HOT 1
- Redshifting spectra with a redder spectral coverage than the standard OzDES setting HOT 3
- Problem in processing fits file HOT 3
- Give a way to report width of xcorr peak
- Additional templates HOT 9
- Uncertainties from Cross Correlation HOT 1
- Cross correlation peaks inverted for quasars HOT 5
- Redshift limit and adding templates HOT 2
- Air or Vacuum? HOT 2
- Vacuum/air wavelengths HOT 2
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