{"url":"/dataset/high-cardinality-geometrically-shaped","name":"High-cardinality Geometrically Shaped Constellation for the AWGN channel and optical fibre channel","full_name":null,"description_markdown":"Optimised constellation for the paper High-Cardinality Geometrical Constellation Shaping for the Nonlinear Fibre Channel. Each file is a constellation optimised for the SNR in dB mentioned in the filename, containing the coordinates of the constellation points as comma-separated values. Each column represents a dimension and each row is a separate constellation point. The bit labels for the generalised mutual information (GMI) are implied and follow natural mapping, the first row is 0,..,0,0 the second 0,...0,1 the third 0,..,1,0 the fourth 0,...,1,1 etc and the last 1,...,1,1. The file named gmi.txt is the GMI for the resulting constellations. \r\n\r\n[source](https://doi.org/10.5522/04/20223963.v1)","description_withheld":null,"homepage":"https://doi.org/10.5522/04/20223963.v1","introduced_date":"2022-05-09","introduced_date_note":null,"introduced_by":{"paper":"/paper/high-cardinality-geometrical-constellation","title":"High-Cardinality Geometrical Constellation Shaping for the Nonlinear Fibre Channel","first_author":null,"url":null},"license":null,"modalities":[],"tasks":[],"languages":[],"variants":["High-cardinality Geometrically Shaped Constellation for the AWGN channel and optical fibre channel"],"data_loaders":[],"num_papers_in_archive":1,"source":{"archive":"pwc-archive (Hugging Face), CC BY-SA 4.0","snapshot":"2025-07-28"},"benchmarks":[],"papers_with_a_benchmark_row":[],"syntology_totals":{"read_at":"2026-09-24T18:15:14+00:00","papers_with_samples":0,"samples_harvested":0,"samples_ran":0,"samples_unverified":0,"pointer_only_for_licence":0,"papers_with_no_sample_that_ran":0,"note":"the per-paper counts above, summed; not a rate"},"papers_note":"The archive never published its papers-using-dataset list; these are papers with a leaderboard row on this dataset's benchmarks."}