Directory https://webfiles.york.ac.uk/HFODD/Projects/dysprosium contains raw data corresponding to calculations performed within project dysprosium Files are organised within the following directories: dy149/ dy151/ dy153/ dy155/ dy157/ dy159/ dy161/ dy163/ dy165/ dy167/ dy167-106/ dy169/ dy171/ dy173/ dy175/ dy177/ dy179/ dy181/ dy183/ dy185/ dy187/ dy189/ dy191/ hf318j/ Pb208/ Directory hf318j contains all files of the full distribution of the code HFODD (v318j). The same files are also collected in one gziped tar file hf318j_distribution.viking.tar.gz Directries dybbb contain files pertaining to the calculations performed for the isotopes of dysprosium bbbDy for bbb=149-191 All files have the filenames with the following structure: [N00001x-L01R01-]aabbb-ccc-udd-170-HFT-fff-N16-siq-UDF1.318j.iii Sections above have the following meaning: aa = dy, name of the element bbb = mass number ccc = 000 for stage 3 calculations without blocking = 084 for the 84th orbital blocked = ... = 126 for the 126th orbital blocked u = 3 for calculations on the oblate side = 4 for calculations on the prolate side dd = 06 fixed-pairing gap constrained calculation starting from Pb208.oblate.rec = 66 initial unconstrained convergence calculation starting from 06 = 67 continuing unconstrained convergence calculation starting from 66 = 68 converging unconstrained SLOW=0.95 calculation starting from 67 fff = AMP for the angular-momentum-projection calculation; (for the convergence calculation, this section is omitted) iii = dat for the input data files = out for the output files = rec for the record files = ker for the kernel files. For the kernel files (and only for them), section N000010-L01R01- is present. In the subdirectories dybbb, the record files are included only for dd = 68, which allows for rerunning the angular-momentum-projection calculations. With the kernel files existing (not existing) in the execution directory, the kernel files are read (written) and the calculations take little (much) CPU time. Directory Pb208 contains all files generated for building the starting points for the dd = 06 calculations. Those for u = 3 (u = 4) start from the "oblate" ("prolate") files. Directory dy167-106 contains all files pertaining to runs dd = 06, 66, 67, and 68, including the corresponding iii = rec files. It illustrates the patterns used for all other 22 isotopes and 22 blocked states. All calculations were performed using the parity-conserved plus simplex-broken implementation of the code. They were performed in sequence of the following six stages: Stage 1, initialization. An HF run was performed to determine the ground-state of 208Pb (input data file Pb208.UDF1.dat). This run started from scratch and did not require any iii = rec file. Stage 2, polarization. Starting from the iii = rec file of Stage 1, two HF polarization runs were performed for 208Pb by using weak constraints on the axial quadrupole moments of: Q20 = +0.858 b (prolate shape, input data file Pb208.prolate.UDF1.dat) and Q20 = -0.858 b ( oblate shape, input data file Pb208.oblate.UDF1.dat). Exact values of the constrained quadrupole moments were irrelevant; the goal was to induce small axial deformations in 208Pb with the axial-symmetry axis oriented along the Cartesian "z" axis. Both runs used a weak cranking constraint of omega-z = -0.001 MeV oriented along the axial-symmetry axis.The goal of Stage 2 was to split the spherical orbitals into the deformed orbitals quantized according to the values of the total angular-momentum projections on the Cartesian "z" axis. The negative values of omega-z ensured that orbitals with positive projections of the angular momentum were obtained above those with negative projections. This allowed us to identify orbitals with tags 84(2)126 that would be used in the following runs to select the blocked quasiparticles. By using the even tags of the orbitals only, we picked those that had positive projections of the angular momentum. Stage 3, pairing. Starting from the oblate (u = 3) and prolate (u = 4) iii = rec files of Stage 2, the HFB pairing runs (dd = 06) were performed with fixed constant pairing gaps of Delta_P = 1 MeV and Delta_N = 1 MeV. In addition, for oblate (prolate) runs, large values of the quadrupole moments were constrained to Q20 = -10 b (Q20 = +10 b). In Stage 3, for all isotopes, quasiparticles were blocked according to the tags identified in Stage 2. The goal of Stage 3 was to obtain stable paired solutions (no pairing collapse) at large deformations that would be good starting points for the final convergence runs. In addition, for prolate shapes (u = 4), the false-vacuum calculations without blocking (ccc = 000) were also performed. Stage 4, convergence. Starting from the oblate (u = 3) and prolate (u = 4) iii = rec files of Stage 3, (i) the dd = 66 HFB pairing runs (eee = HFT) were performed with the pairing force replacing the fixed constant pairing gaps. All runs of Stage 4 were performed with constraints on the quadrupole moments released. In this way, for nuclei that would have both oblate and prolate minima, selfconsistent oblate and prolate solutions were obtained in the u = 3 and u = 4 runs. Otherwise, for nuclei that would have only one oblate, prolate, or spherical minimum, both u = 3 and u = 4 runs slided down to the common selfconsistent solution. As it turned out, some HFB runs needed to be re-converged at dd = 67 by using the iii = rec files obtained at dd = 66. For consistency, all HFB runs were re-converged, even if for those already converged at dd = 66 only a few iterations were performed. In addition, at dd = 68, by using the iii = rec files obtained at dd = 67, the final convergence was performed with the slowing-down parameters of SLOW=0.95 Stage 5, angular-momentum projection (fff = AMP). At Stage 5, the angular-momentum projection was performed for all converged and HFB (dd = 68) runs, and the spectroscopic magnetic-dipole and electric-quadrupole moments were determined.