eazy-py
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Pythonic photometric redshift tools based on EAZY
On Mac systems using Python 3.8 and later, the process start method defaults to "spawn" which raises a RuntimeError if `mp.Pool` is not called within a `if __name__ == '__main__':`...
I am trying to use my own catalog using fluxes I calculated from the magnitudes I got from the B,V,g',I',r, sdss filtered pictures I took. I have been having issues...
Possible alternative to including `eazy-photoz` as a submodule would be to just download the filters and templates from that repo and put them in the `eazy` site-packaged directory. This allows...
See the `update-setup` branch. TBD: - how to include the pieces from the `eazy-photoz` submodule that are currently symlinked in `eazy/data` - how to include the dependencies of my github...
1) How does eazy-py account for non detections (upper limits)? If I have one source that is out of the field for one specific observed band I have to put...
When fitting some simulated HST+JWST fluxes, comparing the original EAZY to eazy-py, where I've fit the same data set with the same templates (and template error function), without using a...
Hi @gbrammer I'm trying to understand why there are differences between outputs in the legacy way of running EAZY vs eazypy. Since both run the same C code, I'm bit...
The `fit_catalog` method that replaced `fit_parallel` in 2b3caf870d7ec8f95d6ae52e8e7cade9cab84675 has a serious bug in the [iteration over redshift steps](https://github.com/gbrammer/eazy-py/blob/2b3caf870d7ec8f95d6ae52e8e7cade9cab84675/eazy/photoz.py#L1440) in that it evaluates the TEF at the unit index of the...
does this function exist, or would it be easy to implement?
Hello, I noticed an error in the calculation of the pivot wavelength. The first and second arguments for `np.trapz` need to be swapped to fix this.