Output Product: Covariance of Tomographic Cosmic Shear EB Power Spectra¶
$SetSchemaPath le3/wl/cmtwopcf/out/euc-le3-wl-cmtwopcf-PEBShearShear2D.xsd
Data Product Name¶
$PrintDataProductName
Data Product Custodian¶
$PrintDataProductCustodian
Name of the Schema File¶
$PrintSchemaFilename
Last Edited for DPDD Version¶
1.1
Processing Elements Creating / Updating / Using the Product¶
Creators:
LE3_CM_2PCF_WL_ShearShear_Pipeline
Consumers:
WL-SWG
Processing Function using the products¶
SGS pipeline output product to be used by LE3 and SWGs
Proposed for inclusion in EAS/SAS¶
This product is proposed for inclusion in the SAS: Yes
The covariance matrix gives the error estimates of the shear-shear real-space second-order statistics PE-PE, PB-PB, PEB-PEB, PE-PB, PE-PEB, PB-PEB functions.
Data Product Elements¶
$PrintDataProductElements
Detailed Description of the Data Product¶
This product contains the covariance matrix for tomographic cosmic shear E/B power spectra.
This output product is a fits binary table containing important input parameters as keywords in primary HDU, and a binary table in the next HDU with the covariance for cosmic shear E/B modes, as described in
SpatialCoverage a description of the spatial footprint [optional, cot:spatialFootprint],
CatalogSelection: describing the selection in the input catalogues [optional, up to 4 elements]
CatalogFileName: the name of the input catalogue [sys:dataFileName]
Selection: selection associated to catalogue [string]
CatalogUse: for which use case the catalog is employed (=[“ShearShear”]) [string among “PosPos”, “PosShear”, “ShearShear”]
CatalogInfo: whether position or shear information is used in this catalogue (=[“Shear”]) [string among “Pos”, “Shear”]
CatalogOrder: order associated to catalogue for reporting (e.g. BIN_ID1)[int32]
Keywords¶
This fits table is expected to contain the following keywords in primary HDU, characterizing the important parameters of the product:
$PrintPrimaryHeader fit/euc-le3-wl.xml le3.wl.cm2pcf.output.pebshearshear2d
Covariance table¶
The table (first HDU, EXTNAME=”RS_COVAR_EB_SHEARSHEAR2D”) will contain the following columns:
$PrintCatalog fit/euc-le3-wl.xml le3.wl.cm2pcf.output.pebshearshear2d
Note
Under discussion is the possibility in the future of having as first HDU an estimate for Shot Noise :
ELL1: first mean multipole [D, float64]
ELL2: second mean multipole [D, float64]
BIN_COMB1: first index for combination of redshift bins [J, int32]
BIN_COMB2: second index for combination of redshift bins [J, int32]
PE_PE_SH: covariance between E band power spectrum (shape/shot noise) [D, float64]
PB_PB_SH: covariance between B band power spectrum (shape/shot noise) [D, float64]
PEB_PEB_SH: covariance between EB band power spectrum (shape/shot noise) [D, float64]
PE_PB_SH: covariance between E and B band power spectra (shape/shot noise) [D, float64]
PE_PEB_SH: covariance between E and EB band power spectra (shape/shot noise) [D, float64]
PB_PEB_SH: covariance between B and EB band power spectra (shape/shot noise) [D, float64]
Warning
We have discussed to add later in the primary header
<IntegerKeyword name="SHE_SEL"/> <!-- ID of selection made (e.g. tomographic redshifts, stellar mass…) -->