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Releases: foglienimatteo/GaPSE.jl

Version 0.8.0

23 Feb 12:20
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Now you can work with an arbitrary window function.

Version 0.7.0

07 Mar 09:36
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Version 0.7.0 Pre-release
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With the notebook ipynbs/Computations_b1p5-sb0-fevo0.ipynb you can compare now the contribution of the Galaxy Number Counts to the Primordial Non-Gaussianities in the Power Spectrum.

Version 0.6.0

16 Jan 15:51
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Version 0.6.0 Pre-release
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  • Made the docstrings for almost all the functions in the code; only the LD, GNCxLD and LDxGNC TPCFs are huge holes in this picture

  • Improved the structure of the functions that manage the Integrated Window Function (print_map_F and WindowF in particular); some options have changed name

  • Improved the structure of the functions that manage the Integrated Window Function (print_map_IntegratedF and WindowFIntegrated in particular); some options have changed name

  • Improved the code for PS_multipole and associated functions; some options have changed name

Version 0.5.0

09 Dec 16:17
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You can now compute the PNG contributions to the PS at large scales. Still need to be fully tested, so it's not 100% reliable.

Version 0.4.0

03 Jun 22:12
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Version 0.4.0 Pre-release
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Implementation of the following features:

  • relativistic Galaxy Number Counts TPCFs;
  • cross correlations between Luminosity Distance perturb and Galaxy Number Counts;
  • code for the computation of the Doppler and the matter TPCFs in the Plain-Parallel approximation;
  • tests for all of them;

Version 0.3.0

06 Apr 19:03
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Version 0.3.0 Pre-release
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Improved docs, tests and PS computation. Implemented the functions necessary for the evaluation of the Doppler auto-CF in the Plane Parallel approximation.

Version 0.2.0

17 Mar 11:38
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Version 0.2.0 Pre-release
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Resctructuration of CosmoParams and many other things; check the file CHANGELOG.md.

Version 0.1.0

07 Mar 16:06
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Version 0.1.0 Pre-release
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First release of the code. The following functionalities are implemented:

  • read an arbitrary input matter power spectrum, produced by CLASS
  • write and read a map of the window F function
  • read an arbitrary input background data file, produced by CLASS
  • calculate all the GR effects two-point auto-correlation and cross-correlation multipole functions, for an arbitrary multipole order
  • calculate the sum of all these TPCFs