.. include:: ../../gcsubstitutions.txt

.. _PKGCOutputYAM:

Output - Yamamoto [Power Spectrum Multipoles and Window Product]
==================================================================

$SetSchemaPath le3/gc/euc-le3-gc-pkpf-yam.xsd

Data Product Name
__________________
.. DataProductNameStart

$PrintDataProductName

.. DataProductNameEnd

Data Product Custodian
________________________
.. DataProductCustodianStart

$PrintDataProductCustodian

.. DataProductCustodianEnd

Name of the Schema File
________________________
.. NameSchemaStart

$PrintSchemaFilename

.. NameSchemaEnd

Last Edited for DPDD Version
____________________________
.. DpddVersionlTagStart

1.1

.. DpddVersionTagEnd

Processing Elements Creating / Updating / Using the Product
___________________________________________________________
.. PECreatorStart

**Creators:**

* LE3_GC_PK

**Consumers:**

* LE3_GC_CMPK

.. PECreatorEnd

Processing function using the data product
____________________________________________
.. PFUsingStart

* LE3_GC_PowerSpectumCovariance
* This is a SGS pipeline final output product to be used by SWGs.

.. PFUsingEnd

Proposed for inclusion in EAS/SAS
___________________________________

.. IncludeInSASStart

This product is proposed for inclusion in the SAS: Yes

Is going to be used by the SWG-GC for their scientific analysis.

.. IncludeInSASEnd

Data Product Elements
______________________
.. DataProductElementsStart

$PrintDataProductElements

.. DataProductElementsEnd

Detailed Description of the Data Product
_________________________________________
.. DetailedDescStart

This output product is the power spectrum calculated over the input data catalog.
The product contains 2 FITS files relative to the Multipole 0 to 4, and Window Function Power Spectra

XML Keywords
^^^^^^^^^^^^
The product contains the following keywords:

**DataCatalog**
  Name of input DATA catalog
**RandCatalog**
  Name of input RANDOM catalog if used
**Statistics**
  Statistics used to evaluate PK
**NbarMethod**
  Method used for Nbar calculation
**NFT**
  Number of grid Points
**BoxSide**
  Side of the box containing the catalog objects
**MASscheme**
  Mass Assignment Schema used for density fields
**UseFKPweight**
  FKP weighting was enabled/disabled
**Pest**
  Estimated value for PK used for weighting
**UseInterlacing**
  Interlacing field usage enabled/disabled
**BinType**
  Binning scale: LIN/LOG
**BinNumDat**
  Number of bins in the Data Catalog spectrum
**KminDat**
  Minimum K value in output in the Data Catalog spectrum
**KmaxDat**
  Maximum K value in output in the Data Catalog spectrum
**DeltaKdat**
  Bin size in the Data Catalog spectrum
**BinNumWin**
  Number of bins in the Data Catalog spectrum
**KminWin**
  Minimum K value in output in the Random Catalog spectrum
**KmaxWin**
  Maximum K value in output in the Random Catalog spectrum
**DeltaKwin**
  Bin size in the Random Catalog spectrum
**BinNum2D**
  Number of bins in the 2D catalogs
**ReconstructionID**
  Identirfier for the reconstruction used
**CosmologyID**
  Cosmology used
**ReleaseName**
  Name of the release
**SpectrumFile**
  :ref:`FITS<gcpkspefileyam>` file with the Multipoles 0, 1, 2, 3, 4
**WindowFile**
  :ref:`FITS<gcpkspefilewinyam>` file with the Multipoles 0, 1, 2, 3, 4 for the window function


.. _gcpkspefileyam:

**SpectrumFile** FITS file
^^^^^^^^^^^^^^^^^^^^^^^^^^
The FITS type *le3.gc.pkpf.spe.1D* contains one binary table HDU named **SPECTRUM** with the following structure:

$PrintHDUTableContents fit/euc-le3-gc.xml le3.gc.pkpf.spe.1D SPECTRUM


.. _gcpkspefilewinyam:

**WindowFile** FITS file
^^^^^^^^^^^^^^^^^^^^^^^^
The window function data are stored in the same structure of the 1D :ref:`SpectrumFile<gcpkspefile>`


.. DetailedDescEnd