List of parameters

SRoll parameters

NAME

DESCRITPION

bolo

List of detectors name

nbolo

Size of the list ‘bolo’

BeginRing

First ring to consider (included)

EndRing

Last ring to consider (included)

RSTEP

Ring step. If set to 1, all the input rings are processed by sroll,if set to 10, 1 ring out of 10 is used, and so on. Useful to quick check some parameter combinations, as run time is significantly reduced.Use RSTEP=1 for actual productions.

Nside

Indice of pixelization of the sphere healpix

D_NOPOL

NORM_GAIN

Flag for normalise the gain

REMOVE_CAL

Flag for remove calibration

ADDDIP

Flag for add the dipole

KCMBIN

TESTPOL

If set to 0, activates the sroll simulation code (without stim),where colored noise and ADCNL residuals are added to the input signal HPR.If set to 4, only the ADCNL residuals part is added (?). Other values allowed in the code are: 3 (commented), 7 (?). Ignored (forced to -1) if stim_paramfiles is set.

XI2STOP

Threshold for the XI2 calcul

seuilcond

Threshold used for cond matrix

NITT

Number of iterations

FITANGLE

FITPOLEFF

saveCOV

saveCO

delta_psi

Angle in degrees to add to all bolometers psi pointing ({dbpath}/{pixname}_REP6_ptg_TUPLE_2) to simulate an entire focal plane rotation.Omit or set to 0.0 for default/legacy behavior (no focal plane rotation)

verbose

TEMPLATE_NSIDE

Indice of pixelisation for the template

BUILDTF

SEED

GAINSTEP

Number of gain values to fit over the whole mission. If set to 1, only one gain value will be fitted, thus no variable gains. RD12 values are GAINSTEP=128 for 100GHz to 217GHz and GAINSTEP=32 for 353GHz to 857GHz.

NADU

NADUSTEP

Number of setp used in fit_adu ( function no longer use in sroll4)

DOCNN

Bolean list of size NITT, run the CNN or not at each iteration

val_mean

w_mean

do_mean

CALLCNN

Path for CNN

CNN_START

Define at wich iteration start to use CNN

Calibration

NEP

White noise for each detectors

CrossPol

Table of Polarization efficiency [%] for each detectors

Monop

OUT_NOPOL

bolomask

Mask that define which bolometer to use.

beg_surv

Array that define the start ring for each survey

end_surv

Array that define the end ring for each survey

name_surv

Array that define the name of each survey

MAPRINGS

Mask

Binary map that is used to indicate which pixels or regions of a spherical map are considered valid or usable. ( Example

projectionType

Projection use for the output map : example for cosmology ‘I,Q,U’ for intensity and polarized map and for oceanography ‘spline3’ to project signal in 0,6,180 degrees.

in_template_map

Signal_noPS

Input signal

ADU

Badring

List of flagged rings that wont be process

HPR_Calib

List of HPRs containing the component that will be subtracted,not fitted, from Signal_noPS.

Hit_noPS

Ptg_noPS

Pointing

Theo_HPR

Theo_MAP

phase

Input phase of the HPR to be projected to maps. Used for advance denoising

rgcnn

bolo_map

List of name for the output (len(bolo_map) == len(MAPRING))

Out_MAP

Path to save maps ouput

Out_VEC

Path to save vectors ouput