# Enter input files to reset
#
cu2cl6_m1_std.inp
#
cu2cl6_m3_std.inp
#
cu2cl6_m1_clp6cud9.inp
#
cu2cl6_m3_clp6cud9.inp
#
cu2cl6_m1_std.inp
#
cu2cl6_m3_std.inp
#
cu2cl6_m1_clp6cud9.inp
#
cu2cl6_m3_clp6cud9.inp
# Numerics changes due to different distributions 
cu2cl6_m1_std.inp
# Numerics changes due to different distributions 
cu2cl6_m3_std.inp
# Numerics changes due to different distributions 
cu2cl6_m1_clp6cud9.inp
# Numerics changes due to different distributions 
cu2cl6_m3_clp6cud9.inp
# turned on dbcsr_multiply_fm_fm_t
cu2cl6_m1_std.inp
# turned on dbcsr_multiply_fm_fm_t
cu2cl6_m3_std.inp
# turned on dbcsr_multiply_fm_fm_t
cu2cl6_m3_clp6cud9.inp
# new general distribution
cu2cl6_m1_std.inp
# new general distribution
cu2cl6_m3_std.inp
# new general distribution
cu2cl6_m3_clp6cud9.inp
# Numerics change 
cu2cl6_m3_std.inp
# Different machines, different results
cu2cl6_m3_clp6cud9.inp
#
cu2cl6_m3_clp6cud9.inp
# numerics
cu2cl6_m1_std.inp
cu2cl6_m3_std.inp
#
cu2cl6_m1_clp6cud9.inp
# fm to dbcsr
cu2cl6_m1_std.inp
# fm to dbcsr
cu2cl6_m3_std.inp
# fm to dbcsr
cu2cl6_m1_clp6cud9.inp
# fm to dbcsr
cu2cl6_m3_clp6cud9.inp
# atomic code: unrestricted calculations 
cu2cl6_m1_std.inp
# atomic code: unrestricted calculations 
cu2cl6_m3_std.inp
# atomic code: unrestricted calculations 
cu2cl6_m1_clp6cud9.inp
# atomic code: unrestricted calculations 
cu2cl6_m3_clp6cud9.inp
# convert mo_derivs to dbcsr
cu2cl6_m1_std.inp
# convert mo_derivs to dbcsr
cu2cl6_m3_std.inp
#
cu2cl6_m1_clp6cud9.inp
#
cu2cl6_m3_clp6cud9.inp
#
cu2cl6_m1_std.inp
#
cu2cl6_m3_std.inp
#  
cu2cl6_m1_std.inp
#  
cu2cl6_m3_std.inp
# Numerics 
cu2cl6_m1_std.inp
# Numerics 
cu2cl6_m3_std.inp
#  
cu2cl6_m1_std.inp
#  
cu2cl6_m3_std.inp
#  
cu2cl6_m1_clp6cud9.inp
#  
cu2cl6_m3_clp6cud9.inp
# reset for numerics with a bunch of compilers/libs (all smaller than 1E-9)
cu2cl6_m1_clp6cud9.inp
cu2cl6_m1_std.inp
cu2cl6_m3_std.inp
# Numerics due to DBCSR images. 
cu2cl6_m1_std.inp
# Numerics due to DBCSR images. 
cu2cl6_m3_std.inp
# Numerics due to DBCSR images. 
cu2cl6_m1_clp6cud9.inp
# Numerics due to DBCSR images. 
cu2cl6_m3_clp6cud9.inp
# Numerics differences due to different distribution 
cu2cl6_m1_std.inp
# Numerics differences due to different distribution 
cu2cl6_m3_std.inp
# Numerics differences due to different distribution 
cu2cl6_m1_clp6cud9.inp
# Numerics differences due to different distribution 
cu2cl6_m3_clp6cud9.inp
# reset numerics, fix upper limits in multiply
cu2cl6_m1_std.inp
# reset numerics, fix upper limits in multiply
cu2cl6_m3_std.inp
# reset numerics, fix upper limits in multiply
cu2cl6_m1_clp6cud9.inp
# reset numerics, fix upper limits in multiply
cu2cl6_m3_clp6cud9.inp
#
cu2cl6_m1_std.inp
#
cu2cl6_m3_std.inp
#
cu2cl6_m1_clp6cud9.inp
#
cu2cl6_m3_clp6cud9.inp
# Numerics introduced by major QS refactoring 
cu2cl6_m1_std.inp
# Numerics introduced by major QS refactoring 
cu2cl6_m3_std.inp
# Numerics introduced by major QS refactoring 
cu2cl6_m1_clp6cud9.inp
# Numerics introduced by major QS refactoring 
cu2cl6_m3_clp6cud9.inp
# Numerics due to new local multiplication. 
cu2cl6_m1_std.inp
# Numerics due to new local multiplication. 
cu2cl6_m3_std.inp
# Numerics due to new local multiplication. 
cu2cl6_m1_clp6cud9.inp
# Numerics due to new local multiplication. 
cu2cl6_m3_clp6cud9.inp
# extended GTH pseudopotentials 
cu2cl6_m1_std.inp
# extended GTH pseudopotentials 
cu2cl6_m3_std.inp
# extended GTH pseudopotentials 
cu2cl6_m1_clp6cud9.inp
#  
cu2cl6_m1_std.inp
#  
cu2cl6_m3_std.inp
#  
cu2cl6_m1_clp6cud9.inp
#  
cu2cl6_m3_clp6cud9.inp
# reset numerics
cu2cl6_m3_std.inp
# more numerics
cu2cl6_m1_std.inp
#  
cu2cl6_m1_std.inp
#  
cu2cl6_m3_std.inp
#  
cu2cl6_m1_clp6cud9.inp
