Project ID: plumID:25.029
Source: ./crys/4-reweight_crys.dat
Originally used with PLUMED version: 2.8
Stable: zipped raw stdout - zipped raw stderr - stderr
Master: zipped raw stdout - zipped raw stderr - stderr

Click on the labels of the actions for more information on what each action computes
tested onv2.10
tested onmaster
#RESTART

WHOLEMOLECULESThis action is used to rebuild molecules that can become split by the periodic boundary conditions. More details ENTITY0the atoms that make up a molecule that you wish to align=1-3922 #3832 ENTITY1=3833-3922 # prot0 lig1
DISTANCECalculate the distance/s between pairs of atoms. More details LABELa label for the action so that its output can be referenced in the input to other actions=d0 ATOMSthe pair of atom that we are calculating the distance between=1911,3857 # cat 160 SER OG vs UNK C19 DISTANCECalculate the distance/s between pairs of atoms. More details LABELa label for the action so that its output can be referenced in the input to other actions=d1 ATOMSthe pair of atom that we are calculating the distance between=3853,3885 # ext UNK C17 vs C39 DISTANCECalculate the distance/s between pairs of atoms. More details LABELa label for the action so that its output can be referenced in the input to other actions=h0 ATOMSthe pair of atom that we are calculating the distance between=1915,3858 # oxh 161 MET N vs O7 DISTANCECalculate the distance/s between pairs of atoms. More details LABELa label for the action so that its output can be referenced in the input to other actions=h1 ATOMSthe pair of atom that we are calculating the distance between=797,3858 # oxh 87 TYR N vs O7 DISTANCECalculate the distance/s between pairs of atoms. More details LABELa label for the action so that its output can be referenced in the input to other actions=s0 ATOMSthe pair of atom that we are calculating the distance between=1911,2991 # cat 237 HIS NE2 vs cat 160 SER OG DISTANCECalculate the distance/s between pairs of atoms. More details LABELa label for the action so that its output can be referenced in the input to other actions=x0 ATOMSthe pair of atom that we are calculating the distance between=1911,1915 # cat 160 SER OG vs oxh 161 MET N # autohinibition DISTANCECalculate the distance/s between pairs of atoms. More details LABELa label for the action so that its output can be referenced in the input to other actions=x1 ATOMSthe pair of atom that we are calculating the distance between=1911,797 # cat 160 SER OG vs oxh 87 TYR N # autohinibition
metad: METADUsed to performed metadynamics on one or more collective variables. More details ... ARGthe labels of the scalars on which the bias will act=h0,h1 # h0,h1 SIGMAthe widths of the Gaussian hills=0.05,0.05 # 0.5*fluctuation ~ 1A HEIGHTthe heights of the Gaussian hills=0.0 # standard ~0.1-1.0*kBT KJ/mol | ~0.02-1.20 d, ~1.0-2.0 a -> TAU??? PACEthe frequency for hill addition=10000000 # ~100-500 steps relax system before next hill add # change from 400 to 500!!! BIASFACTORuse well tempered metadynamics and use this bias factor=15 # barriers 20-30 KJ/mol need a bias factor of ~10-15 biol syst # change from 30 to 15!!! TEMPthe system temperature - this is only needed if you are doing well-tempered metadynamics=298 # well-tempered GRID_MINthe lower bounds for the grid=-1.0,-1.0 GRID_MAXthe upper bounds for the grid=2.0,2.0 # max min values cv, store hills in file, memory efficient ? FILE a file in which the list of added hills is stored=HILLS ...
UPPER_WALLSDefines a wall for the value of one or more collective variables, More details ARGthe arguments on which the bias is acting=h0 ATthe positions of the wall=0.6 KAPPAthe force constant for the wall=5000 EXP the powers for the walls=2 EPS the values for s_i in the expression for a wall=1 OFFSET the offset for the start of the wall=0 LABELa label for the action so that its output can be referenced in the input to other actions=h0_uwall # 6A max distance from hole UPPER_WALLSDefines a wall for the value of one or more collective variables, More details ARGthe arguments on which the bias is acting=h1 ATthe positions of the wall=0.6 KAPPAthe force constant for the wall=5000 EXP the powers for the walls=2 EPS the values for s_i in the expression for a wall=1 OFFSET the offset for the start of the wall=0 LABELa label for the action so that its output can be referenced in the input to other actions=h1_uwall # 6A max distance from hole #UPPER_WALLS ARG=s0 AT=0.6 KAPPA=5000 EXP=2 EPS=1 OFFSET=0 LABEL=s0_uwall # 6A max distance from hole #UPPER_WALLS ARG=d0 AT=0.6 KAPPA=5000 EXP=2 EPS=1 OFFSET=0 LABEL=d0_uwall # 6A max distance from ser #LOWER_WALLS ARG=x0 AT=0.6 KAPPA=5000 EXP=2 EPS=1 OFFSET=0 LABEL=x0_uwall # 6A max distance from hole #LOWER_WALLS ARG=x1 AT=0.6 KAPPA=5000 EXP=2 EPS=1 OFFSET=0 LABEL=x1_uwall # 6A max distance from hole
LOWER_WALLSDefines a wall for the value of one or more collective variables, More details ARGthe arguments on which the bias is acting=d1 ATthe positions of the wall=4.0 KAPPAthe force constant for the wall=2550 EXP the powers for the walls=2 EPS the values for s_i in the expression for a wall=1 OFFSET the offset for the start of the wall=0 LABELa label for the action so that its output can be referenced in the input to other actions=d1_lwall # crystalline stretch
PRINTPrint quantities to a file. More details ARGthe labels of the values that you would like to print to the file=* STRIDE the frequency with which the quantities of interest should be output=1 FILEthe name of the file on which to output these quantities=colvar.reweight #print less
### reweight histograms as: REWEIGHT_BIASCalculate weights for ensemble averages that negate the effect the bias has on the region of phase space explored More details ARG the biases that must be taken into account when reweighting=metad.bias TEMPthe system temperature=298 hd0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=d0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00667 GRID_MIN the lower bounds for the grid=0.2 GRID_MAX the upper bounds for the grid=1.0 GRID_BINthe number of bins for the grid=120 fd0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hd0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fd0 FILE the file on which to write the grid=fd0.dat hx1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=x1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00500 GRID_MIN the lower bounds for the grid=0.2 GRID_MAX the upper bounds for the grid=0.8 GRID_BINthe number of bins for the grid=120 fx1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hx1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fx1 FILE the file on which to write the grid=fx1.dat hx0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=x0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00250 GRID_MIN the lower bounds for the grid=0.2 GRID_MAX the upper bounds for the grid=0.5 GRID_BINthe number of bins for the grid=120 fx0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hx0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fx0 FILE the file on which to write the grid=fx0.dat hs0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=s0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00333 GRID_MIN the lower bounds for the grid=0.2 GRID_MAX the upper bounds for the grid=0.6 GRID_BINthe number of bins for the grid=120 fs0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hs0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fs0 FILE the file on which to write the grid=fs0.dat hh1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417 GRID_MIN the lower bounds for the grid=0.2 GRID_MAX the upper bounds for the grid=0.7 GRID_BINthe number of bins for the grid=120 fh1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh1 FILE the file on which to write the grid=fh1.dat hh0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417 GRID_MIN the lower bounds for the grid=0.2 GRID_MAX the upper bounds for the grid=0.7 GRID_BINthe number of bins for the grid=120 fh0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh0 FILE the file on which to write the grid=fh0.dat hh0h1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h0,h1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00417 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,0.7 GRID_BINthe number of bins for the grid=120,120 fh0_h1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh0h1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh0_h1 FILE the file on which to write the grid=fh0_h1.dat hh0d0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h0,d0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00667 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,1.0 GRID_BINthe number of bins for the grid=120,120 fh0_d0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh0d0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh0_d0 FILE the file on which to write the grid=fh0_d0.dat hh0s0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h0,s0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00333 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,0.6 GRID_BINthe number of bins for the grid=120,120 fh0_s0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh0s0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh0_s0 FILE the file on which to write the grid=fh0_s0.dat hh0x0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h0,x0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00250 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,0.5 GRID_BINthe number of bins for the grid=120,120 fh0_x0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh0x0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh0_x0 FILE the file on which to write the grid=fh0_x0.dat hh0x1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h0,x1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00500 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,0.8 GRID_BINthe number of bins for the grid=120,120 fh0_x1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh0x1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh0_x1 FILE the file on which to write the grid=fh0_x1.dat hh1d0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h1,d0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00667 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,1.0 GRID_BINthe number of bins for the grid=120,120 fh1_d0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh1d0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh1_d0 FILE the file on which to write the grid=fh1_d0.dat hh1s0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h1,s0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00333 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,0.6 GRID_BINthe number of bins for the grid=120,120 fh1_s0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh1s0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh1_s0 FILE the file on which to write the grid=fh1_s0.dat hh1x0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h1,x0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00250 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,0.5 GRID_BINthe number of bins for the grid=120,120 fh1_x0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh1x0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh1_x0 FILE the file on which to write the grid=fh1_x0.dat hh1x1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=h1,x1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00417,0.00500 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.7,0.8 GRID_BINthe number of bins for the grid=120,120 fh1_x1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hh1x1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fh1_x1 FILE the file on which to write the grid=fh1_x1.dat hd0s0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=d0,s0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00667,0.00333 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=1.0,0.6 GRID_BINthe number of bins for the grid=120,120 fd0_s0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hd0s0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fd0_s0 FILE the file on which to write the grid=fd0_s0.dat hd0x0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=d0,x0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00667,0.00250 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=1.0,0.5 GRID_BINthe number of bins for the grid=120,120 fd0_x0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hd0x0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fd0_x0 FILE the file on which to write the grid=fd0_x0.dat hd0x1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=d0,x1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00667,0.00500 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=1.0,0.8 GRID_BINthe number of bins for the grid=120,120 fd0_x1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hd0x1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fd0_x1 FILE the file on which to write the grid=fd0_x1.dat hs0x0: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=s0,x0 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00333,0.00250 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.6,0.5 GRID_BINthe number of bins for the grid=120,120 fs0_x0: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hs0x0 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fs0_x0 FILE the file on which to write the grid=fs0_x0.dat hs0x1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=s0,x1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00333,0.00500 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.6,0.8 GRID_BINthe number of bins for the grid=120,120 fs0_x1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hs0x1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fs0_x1 FILE the file on which to write the grid=fs0_x1.dat hx0x1: HISTOGRAMAccumulate the average probability density along a few CVs from a trajectory. More details ARGthe quantities that are being used to construct the histogram=x0,x1 LOGWEIGHTSthe logarithm of the quantity to use as the weights when calculating averages=as BANDWIDTHthe bandwidths for kernel density esimtation=0.00250,0.00500 GRID_MIN the lower bounds for the grid=0.2,0.2 GRID_MAX the upper bounds for the grid=0.5,0.8 GRID_BINthe number of bins for the grid=120,120 fx0_x1: CONVERT_TO_FESConvert a histogram to a free energy surface. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=hx0x1 TEMPthe temperature at which you are operating=298 MINTOZERO set the minimum in the free energy to be equal to zero DUMPGRIDOutput the function on the grid to a file with the PLUMED grid format. More details GRIDYou should use ARG instead of this keyword which was used in older versions of PLUMED and is provided for back compatibility only=fx0_x1 FILE the file on which to write the grid=fx0_x1.dat