Allowing the users to append their filters into the existing BEAST filter library #756
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Codecov Report
@@ Coverage Diff @@
## master #756 +/- ##
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- Coverage 43.31% 43.26% -0.06%
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Files 101 101
Lines 9811 9825 +14
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+ Hits 4250 4251 +1
- Misses 5561 5574 +13
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| if __name__ == "__main__": | ||
| parser = argparse.ArgumentParser() | ||
| parser.add_argument( | ||
| "filter_throughput_curve", | ||
| type=str, | ||
| default=None, | ||
| help="filename of filter throughput curve to be added into the BEAST filter library", | ||
| ) | ||
| parser.add_argument( | ||
| "--tablename", | ||
| type=str, | ||
| help="Table name for the filter", | ||
| ) | ||
| parser.add_argument( | ||
| "--observatory", | ||
| type=str, | ||
| help="Observatory for the filter (e.g., HST, GALEX)", | ||
| ) | ||
| parser.add_argument( | ||
| "--instrument", | ||
| type=str, | ||
| help="Instrument associated with the filter (WFC3, ACS, ...)", | ||
| ) | ||
| parser.add_argument( | ||
| "--filtername", | ||
| type=str, | ||
| help="Name for the filter", | ||
| ) | ||
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| args = parser.parse_args() | ||
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| if args.filter_throughput_curve: | ||
| lamb, throughput = numpy.loadtxt(args.filter_throughput_curve, usecols=(0, 1), | ||
| unpack=True) | ||
| append_filter(lamb, throughput, args.tablename, args.observatory, args.instrument, | ||
| args.filtername) | ||
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| if not any(vars(args).values()): | ||
| parser.print_help() |
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I think this should be a separate script in the tools subdir instead of added to phot.py. For consistency with how similar capabilities are handled in the BEAST.
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That makes sense. Will start a separate script for this functionality.
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This task could be merged with the outstanding WIP PR #646!
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Need to add this script to this PR.
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This PR supersedes PR #646, right? If so, please confirm that it provides the same capabilities or that those are not needed desired anymore. |
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Ping. |
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Ping. ;-) |
Sorry!! Yes. |
This PR is to allow the users to add any filters that are not in the default BEAST filter library into the filter library from command line. An input ascii file for a filter throughput curve should have two columns: wavelength in angstrom and throughput.