Euclid mock production v1.8.1

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Revision as of 14:49, 26 April 2019 by Jcarrete (talk | contribs) (Created page with "Goals: * Test new pipeline with some improvements in the SciPIC algorithm. * The catalog is a 2 redshift bins, 0.4 < z < 0.6 and 0.9 < z < 1.1. The catalog has been produced...")
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Goals:

  • Test new pipeline with some improvements in the SciPIC algorithm.
  • The catalog is a 2 redshift bins, 0.4 < z < 0.6 and 0.9 < z < 1.1.

The catalog has been produced using notebook:

> /hdfs/user/jcarrete/data/euclid/flagship_1_8_1/config/Euclid_mock_pipeline_production-v1.8.ipynb

The commit used in SciPIC is 4b08560

Some information about the changes:

  • Copy from 1.7.0 date(15/04/2019) but using the commit that includes the new NFW API (4b08560)
  • I "copy-paste" the way fluxes are estimated in the SciPIC flux autovalidation.ipynb notebook from Pau.
  • This version is the 1st try to integrate the NFW changes from Linda and the correct way of estimating the fluxes using the 1st octant of the new halo rockstar catalog.
  • Changes:
    • query to use the new rockstar dark matter halo catalog; the id for haloes changes: (bx, by, bz, id)
    • API change to use the NFW from Linda
    • file from Francisco mv to the scipic code: cp /software/astro/__to_delete__/src/castander/auxfiles/logflux_correction_hae_v1_3_1.csv /nfs/pic.es/user/j/jcarrete/src/mocks/scipic/mocks/fluxes/halpha_flux/logflux_correction_hae_v1_3_1.csv
    • New binning emmission lines
    • Changes in the way emission lines are called
    • Changes in the auxilary files path: "/nfs/pic.es/user/j/jcarrete/scipic_files"
    • I add a unique_gal_id using bx, by, bz and id
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