Input - GC PFs Configuration Set

$SetSchemaPath le3/gc/inp/euc-le3-gc-conf-set.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:

• None: Created by hand

Consumers:

• 2PCF-GC case LE3_GC_TwoPointCorrelation

• 3PCF-GC case LE_GC_3PCF

• BK-GC case LE3_GC_BK

• CM-2PCF-GC case LE3_GC_CM2PCF

• CM-PK-GC case LE3_GC_CMPK

• PK-GC case LE3-GC

Processing function using the data product

• 2PCF-GC case LE3_GC_2PCF

• 3PCF-GC case LE3_GC_ThreePointCorrelation

• BK-GC case LE3_GC_Bispectrum

• CM-2PCF-GC case LE3_GC_TwoPointCovariance

• CM-PK-GC case LE_GC_PowerSpectrumCovariance

• PK-GC case LE3-GC-PK

Proposed for inclusion in EAS/SAS

This product is proposed for inclusion in the SAS: Yes

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

Data Product Elements

$PrintDataProductElements

Detailed Description of the Data Product

2PCF-GC

To compute the Galaxy Clustering Two-point Correlation Function, a parameter file specifying the configuration is needed. The configuration file contains all the information about the max/min scales to use in the computation, the number of output bins in the correlation function, the estimator to be used and information on the cosmology to be used for the coordinate transformation. The estimator selected in the configuration file defines the output product obtained.

XML Product

The product contains the following keywords:

PF

Name of the Processing function using this configuration

ConfigurationID

Identifier for the configuration Parameters+Cosmology used in this product

ParameterSetID

Identifier for the configuration Parameter set used in this configuration

CosmologyID

Identifier for the Cosmology used in this configuration

ReleaseName

Name of the release that uses this configuration

ParameterFile

ASCII file with PF parameters for this configuration

CosmologyFile

ASCII file with cosmological parameters to use in this configuration

Comment

[OPTIONAL] Comment to configuration

ParameterFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The 2PCF parameter file accepts the following keyword list:

[Path] section [used only in LOCAL configuration for code testing]

input

Input data path relative to current workdir

output

Output data path relative to current workdir

[Catalog.Galaxy] section [used only in LOCAL configuration for code testing]

filename

Name of input Data file

name

Name of catalog HDU in input file

coordinates

Coordinate system used by the catalog [CARTESIAN/EQUATORIAL/PSERUDO_EQUATORIAL]

angle_units

Angle units used for angular coordinates [DEGREE/RADIANS]

coord1

Position or name of the column to be used as 1st coordinate value

coord2

Position or name of the column to be used as 2nd coordinate value

coord3

Position or name of the column to be used as 3rd coordinate value

density

Position or name of the column to be used as density value

weight

Position or name of the column to be used as object weight value

filename2

Name of input Data file 2

[Catalog.Random] section [used only in LOCAL configuration for code testing]

filename

Name of input Random file

name

Name of catalog HDU in input file

coordinates

Coordinate system used by the catalog [CARTESIAN/EQUATORIAL/PSERUDO_EQUATORIAL]

angle_units

Angle units used for angular coordinates [DEGREE/RADIANS]

coord1

Position or name of the column to be used as 1st coordinate value

coord2

Position or name of the column to be used as 2nd coordinate value

coord3

Position or name of the column to be used as 3rd coordinate value

density

Position or name of the column to be used as density value

weight

Position or name of the column to be used as object weight value

filename2

Name of input Random file 2

filename_rec

Name of input Random reconstructed file

filename_rec2

Name of input Random reconstructed file 2

[2PCF] section

statistics

Correlation type [ONE_DIM, TWO_DIM_CART, TWO_DIM_POLAR]

method

Pair counting method [LINKED_LIST, KD_TREE]

bin1_type

Type of binning in the 1st dimension [LIN, LOG]

bin1_num

Number of bin channels in the 1st dimension

bin1_min

Minimum separation scale in the 1st dimension

bin1_max

Maximum separation scale in the 1st dimension

bin2_type

Type of binning in the 2nd dimension [LIN, LOG]

bin2_num

Number of bin channels in the 2nd dimension

bin2_min

Minimum separation scale in the 2nd dimension

bin2_max

Maximum separation scale in the 2nd dimension

pi_max

Maximum parallel separation up to which the 2D Cartesian correlation function is integrated to compute the projected correlation function

compute_RR

[true, false] Enable/disable RR pair counting in case of pair file re-use

compute_SS

[true, false] Enable/disable SS pair counting in case of pair file re-use

compute_R1R2

[true, false] Enable/disable R1R2 cross pair counting in case of pair file re-use

compute_S1S2

[true, false] Enable/disable S1S2 shifted cross pair counting in case of pair file re-use

input_file_RR

Input RR pairs FITS file to skip RR calculation [used only in LOCAL configuration for code testing]

input_file_SS

Input SS pairs FITS file to skip SS calculation [used only in LOCAL configuration for code testing]

input_file_R1R2

Input R1R2 cross pairs FITS file to skip R1R2 calculation [used only in LOCAL configuration for code testing]

input_file_S1S2

Input S1S2 shifted cross pairs FITS file to skip S1S2 calculation [used only in LOCAL configuration for code testing]

use_weight

[true, false] Use objects weights

split_factor

Number of sub-catalogs in which the random catalog has been split for RR computation

reconstruction_id

TBD

use_cross

TBD

output_prefix

Output file name prefix

[Validation] section

grid_scale

LinkedList partitioning scheme grid scaling

observer_x

Position of the observer in direction x

observer_y

Position of the observer in direction y

observer_z

Position of the observer in direction z

periodic

[true, false] Use periodic boundaries conditions..TBD

plane_parallel

[true, false] Use parallel plane TBD

box_x_min

Catalog enclosing box minimum position x

box_x_max

Catalog enclosing box maximum position x

box_y_min

Catalog enclosing box minimum position y

box_y_max

Catalog enclosing box maximum position y

box_z_min

Catalog enclosing box minimum position z

box_z_max

Catalog enclosing box maximum position z

ascii_out

[true/false] Enable ASCII output filen in addition to FITS

CosmologyFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The cosmological accepted keywords are:

[Cosmology] section

cosmology_ID

Identifier for the cosmology

om_matter

Matter energy density parameter

om_radiation

Radiation energy density parameter

om_baryons

Baryon energy density parameter

om_vac

Vacuum energy density parameter

om_k

Curvature energy density parameter

Hubble

Hubble parameter in units of 100 Km /s /(Mpc /h)

hubble

Dimensionless Hubble parameter

spectral_index

Scalar index of primordial perturbations

w_eos

Dark energy equation of state

N_eff

Effective number of relativistic species

sigma8

Mass dipersion on sphers of 8 Mpc/h radius

Tcmb

CMB temperature

These parameters are read from the MDB.

3PCF-GC

To compute Galaxy Clustering Three Point Correlation Function, a parameter file specifying the configuration is needed. The configuration file contain all the information about the max/min scale to use in the computation, the number of output bins in the correlation function, the estimator to be used and information on the cosmology to be used for coordinate transformation. The estimator selected in the configuration file defines the output product obtained.

XML Product

The product contains the following keywords:

PF

Name of the Processing function using this configuration

ConfigurationID

Identifier for the configuration Parameters+Cosmology used in this product

ParameterSetID

Identifier for the configuration Parameter set used in this configuration

CosmologyID

Identifier for the Cosmology used in this configuration

ReleaseName

Name of the release that uses this configuration

ParameterFile

ASCII file with PF parameters for this configuration

CosmologyFile

ASCII file with cosmological parameters to use in this configuration

Comment

[OPTIONAL] Comment to configuration

ParameterFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The Bispectrum accepts the following keyword list:

[3PCF] section

correlation

correlation type [CONNECTED, REDUCED]

configuration

triangle configuration [SINGLE, ALL]

method

triplet method [DIRECT_COUNTING / SPHERICAL_HARMONICS_DECOMPOSITION]

binning

triplet binning [COSTHETA, THETA, SIDE]

n_orders

legendre polynomial order

use_weight

use object weights [true, false]

ASCII_out

enable ASCII output files defined below

reconstruction_ID

identifier for the reconstruction

[3PCF.SINGLE] section

r12

first side lenght

r12_binSize

first side shell size

r13

second side lenght

r13_binSize

second side shell size

n_bins

number of bins

[3PCF.ALL] section

rMin

minimum side lenght

rMax

maximum side lenght

shell_size

binsize

[3PCF.FILES] section

input_file_NNN

TBD

input_file_RRR

TBD

input_file_NNN_Legendre

TBD

input_file_RRR_Legendre

TBD

output_file_NNN

TBD [only for ASCII outputs]

output_file_RRR

TBD [only for ASCII outputs]

output_file_NNN_Legendre

TBD [only for ASCII outputs]

output_file_RRR_Legendre

TBD [only for ASCII outputs]

output_file_Corr

TBD [only for ASCII outputs]

[Cosmology] section

Cosmology

Cosmology configuration file [used ONLY in LOCAL run of the code]

CosmologyFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The cosmological accepted keywords are:

[Cosmology] section

cosmology_ID

Identifier for the cosmology

om_matter

Matter energy density parameter

om_radiation

Radiation energy density parameter

om_baryons

Baryon energy density parameter

om_vac

Vacuum energy density parameter

om_k

Curvature energy density parameter

Hubble

Hubble parameter in units of 100 Km /s /(Mpc /h)

hubble

Dimensionless Hubble parameter

spectral_index

Scalar index of primordial perturbations

w_eos

Dark energy equation of state

N_eff

Effective number of relativistic species

sigma8

Mass dipersion on sphers of 8 Mpc/h radius

Tcmb

CMB temperature

These parameters are read from the MDB.

BK-GC

To compute Galaxy Clustering Bispectrum, a parameter file specifying the configuration is needed.

The configuration file contain all the information about the max/min scale to use in the computation, the number of output bins in the output spectrum, the estimator to be used and information on the cosmology to be used for coordinate transformation.

XML Product

The product contains the following keywords:

PF

Name of the Processing function using this configuration

ConfigurationID

Identifier for the configuration Parameters+Cosmology used in this product

ParameterSetID

Identifier for the configuration Parameter set used in this configuration

CosmologyID

Identifier for the Cosmology used in this configuration

ReleaseName

Name of the release that uses this configuration

ParameterFile

ASCII file with PF parameters for this configuration

CosmologyFile

ASCII file with cosmological parameters to use in this configuration

Comment

[OPTIONAL] Comment to configuration

ParameterFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The Bispectrum accepts the following keyword list:

[Bk] section

statistics

Power spectrum estimator [DOAFFT, YBCFFT, YSCFFT, YDS]

use_random_catalog

[true/false] Enable random catalog usage (for estimators that use it)

Nft

Grid cube side

compute_box_side

[true/false] Enable enclosing box computation

box_side

Lenght of the box (Mpc/h) in configuration space if compute_box_side = false

catalog_center

X Y Z position of the catalog center

MAS_scheme

Mass Assignment Schema to be used to prepare the grid

use_FKP_weight

[true/false] Enable FKP weighting schema

Pest

Estimated power for FKP weights

cosmology

Cosmology configuration file [used ONLY in LOCAL run of the code]

output_prefix

Extre ID name in the output file

[Bk.meanDensity] section

method

Method used to calculate Nbar

name

string

format

string

[Bk.Binning] section

k_min

Minumum k in units of the fundamental frequency 2pi/Lbox for spectrum

k_max

Maximum k in units of the fundamental frequency 2pi/Lbox for spectrum

delta_k

Binning step

[Bk.Validation] section

compute_catalog_center

[true/false] Enable catalog center computation

use_MAS_correction

[true/false] Enable MAS correction

use_interlacing

[true/false] Enable interlaced grid usage

use_SN_correction

[true/false] Enable poisson shot-noise correction

use_ascii_output

[true/false] Enable ASCII output filen in addition to FITS

CosmologyFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The cosmological accepted keywords are:

[Cosmology] section

cosmology_ID

Identifier for the cosmology

om_matter

Matter energy density parameter

om_radiation

Radiation energy density parameter

om_baryons

Baryon energy density parameter

om_vac

Vacuum energy density parameter

om_k

Curvature energy density parameter

Hubble

Hubble parameter in units of 100 Km /s /(Mpc /h)

hubble

Dimensionless Hubble parameter

spectral_index

Scalar index of primordial perturbations

w_eos

Dark energy equation of state

N_eff

Effective number of relativistic species

sigma8

Mass dipersion on sphers of 8 Mpc/h radius

Tcmb

CMB temperature

These parameters are read from the MDB.

CM-2PCF-GC

To compute the Galaxy Clustering Two-point Correlation Covarance Matrix Function, a parameter file specifying the configuration is needed. The configuration file contains all the information about the max/min scales to use in the computation, the number of output bins in the correlation function, the estimator to be used and information on the cosmology used for the coordinate transformation. The parameters are used to cross-check the correctness of the input products of the 2PCF-GC provided.

XML Product

The product contains the following keywords:

PF

Name of the Processing function using this configuration

ConfigurationID

Identifier for the configuration Parameters+Cosmology used in this product

ParameterSetID

Identifier for the configuration Parameter set used in this configuration

CosmologyID

Identifier for the Cosmology used in this configuration

ReleaseName

Name of the release that uses this configuration

ParameterFile

ASCII file with PF parameters for this configuration

CosmologyFile

ASCII file with cosmological parameters to use in this configuration

Comment

[OPTIONAL] Comment to configuration

ParameterFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The 2PCF parameter file accepts the following keyword list:

[CM2PCF] section

only_even

In MULTIPOLE case, skip multipoles 1 and 3

CM-PK-GC

The configration product is neede to specify the ccompute Galaxy Clustering Power Spectrum, a Configuration file specifying the configuration is needed. The configuration file contain all the information about the max/min scale to use in the computation, the number of output bins in the output spectrum, the estimator to be used and information on the cosmology to be used for coordinate transformation. The estimator selected in the configuration file defines the output product obtained.

XML Product

The product contains the following keywords:

PF

Name of the Processing function using this configuration

ConfigurationID

Identifier for the configuration Parameters+Cosmology used in this product

ParameterSetID

Identifier for the configuration Parameter set used in this configuration

CosmologyID

Identifier for the Cosmology used in this configuration

ReleaseName

Name of the release that uses this configuration

ParameterFile

ASCII file with PF parameters for this configuration

CosmologyFile

ASCII file with cosmological parameters to use in this configuration

Comment

[OPTIONAL] Comment to configuration

ParameterFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The Bispectrum accepts the following keyword list:

The configuration product specifies a ascii .ini file in the format keyword=value containing the following quantities:

[CMPK] section

only_even

use only even multipoles

PK-GC

The configuration product is needed to specify the compute Galaxy Clustering Power Spectrum, a Configuration file specifying the configuration is needed.

The configuration file contain all the information about the max/min scale to use in the computation, the number of output bins in the output spectrum, the estimator to be used and information on the cosmology to be used for coordinate transformation. The estimator selected in the configuration file defines the output product obtained.

XML Product

The product contains the following keywords:

PF

Name of the Processing function using this configuration

ConfigurationID

Identifier for the configuration Parameters+Cosmology used in this product

ParameterSetID

Identifier for the configuration Parameter set used in this configuration

CosmologyID

Identifier for the Cosmology used in this configuration

ReleaseName

Name of the release using this configuration

ParameterFile

ASCII file with PF parameters for this configuration

CosmologyFile

ASCII file with cosmological parameters to use in this configuration

Comment

[OPTIONAL] Comment to configuration

ParameterFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The Bispectrum accepts the following keyword list:

[Pk] section

statistics

Power spectrum estimator [DOAFFT, YBCFFT, YSCFFT, YDS]

use_random_catalog

[true/false] Enable random catalog usage (for estimators that use it)

compute_cross_power

[true/false] Enable cross spectrum computation

Nft

Grid cube side

compute_box_side

[true/false] Enable enclosing box computation

box_side

Lenght of the box (Mpc/h) in configuration space if compute_box_side = false

catalog_center

X Y Z position of the catalog center

MAS_scheme

Mass Assignment Schema to be used to prepare the grid

use_FKP_weight

[true/false] Enable FKP weighting schema

Pest

Estimated power for FKP weights

cosmology

Cosmology configuration file [used ONLY in LOCAL run of the code]

output_prefix

Extre ID name in the output file

[Pk.meanDensity] section

method

Method used to calculate Nbar

name

string

format

string

[Bk.Binning] section

type_of_binning

Type of bin scale: [LIN/LOG]

shift_to_bin_center

[true/false] Enable output scale referred on bin center

num_log_bins

Number of log-spaced bins if binning LOG

bin_width_dat

The shell-width in units of the fundamental frequency

bin_width_rand

The shell-width in units of the fundamental frequency for the random catalog

k_min_pk

Minumum k in units of the fundamental frequency 2pi/Lbox for spectrum

k_max_pk

Maximum k in units of the fundamental frequency 2pi/Lbox for spectrum

k_min_win

Minumum k in units of the fundamental frequency 2pi/Lbox for window

k_max_win

Maximum k in units of the fundamental frequency 2pi/Lbox for window

num_mu_bins

Number of mu-bins for 2D spectrum P(k,mu) (for estimators that use it)

[Pk.Validation] section

compute_catalog_center

[true/false] Enable catalog center computation

use_MAS_correction

[true/false] Enable MAS correction

use_interlacing

[true/false] Enable interlaced grid usage

use_SN_correction

[true/false] Enable poisson shot-noise correction

use_ascii_output

[true/false] Enable ASCII output filen in addition to FITS

CosmologyFile ASCII file

The ASCII .ini file has a keyword=value structure divided into [sections]. The cosmological accepted keywords are:

[Cosmology] section

cosmology_ID

Identifier for the cosmology

om_matter

Matter energy density parameter

om_radiation

Radiation energy density parameter

om_baryons

Baryon energy density parameter

om_vac

Vacuum energy density parameter

om_k

Curvature energy density parameter

Hubble

Hubble parameter in units of 100 Km /s /(Mpc /h)

hubble

Dimensionless Hubble parameter

spectral_index

Scalar index of primordial perturbations

w_eos

Dark energy equation of state

N_eff

Effective number of relativistic species

sigma8

Mass dipersion on sphers of 8 Mpc/h radius

Tcmb

CMB temperature

These parameters are read from the MDB.