Warp Opus Et

WARP/OPUS-ET Cryo-ET Processing Workflow

Agent Rules — read before acting

• Do only what the user asks. Don't anticipate, extend, or fix unreported issues — even obvious ones. One change at a time.
• Read before editing. Always read the current file/script before describing or modifying it. Don't rely on remembered content — the codebase changes.
• Verify before asserting; discover, don't guess. If uncertain how a tool, flag, or script behaves, confirm it before relying on it — in rough order of authority: run <tool> --help / --help | grep <flag>; read the tool's source (PyTom, cryodrgn/OPUS-ET, WarpTools, AreTomo are open — the source is the ground truth for undocumented conventions, e.g. the missing-wedge Angle1/Angle2 sign, which --help does not spell out); consult official/online docs (WebSearch/WebFetch) when the local tool is thin; or run the tool on a tiny synthetic input and inspect the output. Never infer a convention from a flag's name — a wrong assumption baked into a job runs silently and corrupts results. Wrong documentation is worse than no documentation.
• Enumerate scope before acting. For multi-file changes, use grep to find all affected files and confirm scope with the user before making any edits.
• Show before and after for every edit. Before modifying a script or config, quote the relevant current lines. After editing, summarize exactly what changed — not just "done."
• Don't chain changes. Renaming a variable in one place does NOT mean you should rename it everywhere — confirm scope first.
• Don't redesign. Apparent inconsistencies may be intentional. Respect the existing pattern unless the user asks to change it.
• When in doubt, show the current state and ask. "Here's what I see. Do you want me to change X, Y, or both?"

IMPORTANT: Gather Experimental Settings First

Before generating any commands, collect the parameters below. Do NOT use placeholder values — wait for actual answers. Only ask about phases the user needs.

Try to determine frame type automatically before asking (see Frame Type below).

Microscope & Detector

1. Pixel size (ANGPIX) — physical pixel size in Å (e.g., 1.085, 2.17, 3.37)

2. Exposure per tilt (EXPOSURE) — e⁻/Ų per tilt image (e.g., 2.36, 3.2)

3. Frame format + type — cannot be derived from filenames alone; determine from file extension first, then frame count.

   • Extension check (list the data dir):
     • *.eer → Falcon 4 EER movie (always fractionated; needs frame grouping)
     • *.tif / *.tiff → TIFF movie stack (fractionated)
     • *.mrc → could be either — inspect Z dimension (see Header Tools below): Z > 1 = fractionated, Z == 1 = single frame
   • Single-frame MRC → symlink to average/ + fs_ctf
   • Fractionated MRC/TIFF/EER → fs_motion_and_ctf (with format-specific flags)
   • File naming and MDOC NumberOfFrames are not reliable — don't trust them for detection

   Header tools — pick whichever is available:

   # Preferred (PyTOM env is already required by this skill):
   conda activate "$PYTOM_ENV" && headerPyTom <file.mrc>
   
   # Alternative (only if IMOD is on PATH):
   header <file.mrc>
   
   # Fallback (works in any conda env with mrcfile active, e.g. WARP_ENV):
   python -c "import mrcfile, sys; m = mrcfile.open(sys.argv[1], permissive=True); print('shape:', m.data.shape); m.close()" <file.mrc>
   

   The header (IMOD) command is not assumed available. Default to headerPyTom since PYTOM_ENV is already required by the skill; fall back to the mrcfile one-liner only if PyTOM is unavailable.

   Script-side MRC metadata readers:

   • warp_tiltseries_setup.slurm reads unbinned frame X/Y with Python mrcfile after activating WARP_ENV (m.header.nx, m.header.ny). If mrcfile is missing and AUTO_INSTALL_MRCFILE=1, the script installs it into WARP_ENV with python -m pip install mrcfile and re-checks the import.
   • warp_update_tomo_dims.slurm, gen_tm_jobs_aretomo.slurm, and gen_sphere_mask.slurm run in PYTOM_ENV and read MRC dimensions with headerPyTom; do not import OPUS-ET/cryodrgn in these scripts.
   • gen_training_mask.slurm, train_opuset.slurm, and train_opuset_fixed.slurm run in OPUSET_ENV; OPUS-ET training ANGPIX is inferred only from STAR _rlnDetectorPixelSize, and mask shape/radius is handled through dsdsh create_mask / OPUS-ET readers.

4. Gain reference — required for most fractionated movies (EER, TIFF, raw MRC):

   • Path to gain MRC/DM4 (--gain <file>); ask user if present
   • Orientation flags (--gain_flip_x, --gain_flip_y, --gain_transpose) — ask only if the user already knows them; otherwise omit and let WARP's default apply
   • Skip entirely for already-gain-corrected single-frame MRC

5. EER frame grouping (EER only) — how many raw EER frames per dose fraction, e.g. --eer_ngroups 10. Ask user; typical: 10–20 groups per tilt.

6. Defects map (optional) — --defects <file.txt> for bad-pixel masking; only if user has one.

Tilt Series

7. Approximate tomo dimensions (TOMO_DIMS) — ask the user for cols×rows×Z in unbinned pixels before creating tilt-series settings (e.g. 3840x3712x2000).
   • cols × rows = detector size (fixed, from camera). If the user does not know it, derive X/Y from one unbinned frame or averaged tilt image: set SAMPLE_FRAME in warp_tiltseries_setup.slurm, or leave TOMO_DIM_X/Y blank so the script reads the first MRC under warp_frameseries/average. The script reads m.header.nx / m.header.ny with Python mrcfile in WARP_ENV; if mrcfile is missing, the script can auto-install it into WARP_ENV.
   • Z = an upper bound on sample thickness in unbinned pixels — only used to size AreTomo's reconstruction slab. Phase 3.5 rewrites it from the actual _ali.mrc output, so a rough estimate is fine. Defaults: 2000 for thin lamellae / thin cryo-ET, 3000–4000 for cells / thick specimens.
8. Binning factor (BINNING_FACTOR) — for ts_stack export and AreTomo (e.g. 4, 8). AreTomo runs on the binned stack, so it receives binned dims:
   • VOL_Z = TOMO_DIM_Z / BINNING_FACTOR → AreTomo -VolZ; 500 binned voxels is a practical starting value for many datasets, then adjust if the tomogram needs more or less Z margin
   • ALIGN_Z → AreTomo -AlignZ; set this close to the measured sample thickness in binned voxels, and always keep ALIGN_Z < VOL_Z
   • ALIGN_ANGPIX = ANGPIX × BINNING_FACTOR (stack export pixel size) The unbinned TOMO_DIMS stays in warp_tiltseries.settings; only AreTomo's CLI sees the binned values (computed inside the script). For ALIGN_Z, do not rely on a fixed fraction of VOL_Z when accuracy matters. A practical approach is to run global-only alignment / a quick 3D reconstruction at large binning, inspect an XZ slice, measure the specimen thickness, then set ALIGN_Z near that thickness. VOL_Z should remain larger to provide final-reconstruction Z margin.

Particle / Template Matching

9. Particle diameter (DIAMETER) — in Å (e.g., 320)

10. Box sizes — there are two distinct boxes, sized at different pixel sizes:

    • TM template / mask box (used in Phase 6 by gen_sphere_mask.slurm and consumed by gen_tm_jobs_aretomo.slurm): sized at ALIGN_ANGPIX, since TM runs on the binned reconstructions. Rule: box ≈ round_to_even(DIAMETER / 0.75 / ALIGN_ANGPIX) (particle occupies ~75% of box). Example: 320 Å at ALIGN_ANGPIX=13.48 Å → 32 px.
    • Subtomo export box (SUBTOMO_BOX_SIZE in warp_export_particles.slurm, warp_m_export.slurm, OPUS-ET training): sized at OUTPUT_ANGPIX. Rule: SUBTOMO_BOX_SIZE ≈ round_to_even(DIAMETER / 0.75 / OUTPUT_ANGPIX) (particle occupies ~75% of box), with DIAMETER / 0.5 / OUTPUT_ANGPIX for high-res / strong CTF cases. Example: 320 Å at OUTPUT_ANGPIX=2.5 Å → 171 px → round to 176.

    Both should be a multiple of 8 (preferably 16) for FFT efficiency. Box too small → CTF aliasing; too large → wasted memory and slower training.

11. Subtomogram export pixel sizes — OUTPUT_ANGPIX in warp_export_particles.slurm must be chosen by the user/agent for OPUS-ET training and is often binned after template matching. Do not derive it from warp_tiltseries.settings. COORDS_ANGPIX is the pixel size of coordinates in the input STAR; after this skill's PyTom→WARP conversion it is usually the unbinned ANGPIX. ⚠ Export is destructive: subtomos always land in the shared warp_tiltseries/subtomo/TS_XXX/TS_XXX_<index>_<OUTPUT_ANGPIX>A.mrc (fixed by --settings, not --output_star), so a second species/box/re-export at the same OUTPUT_ANGPIX silently overwrites the previous particles. Isolate each species in its own subtomo_<label>/ before re-exporting — see references/workflow.md §7.1 and item 22 (DATADIR).

12. Template generation / TM template — always ask the user for the source template map (INPUT_MRC) and its pixel size (MAP_ANGPIX); never guess or default to ribo.mrc. The default workflow is to run gen_template_from_mrc.slurm before template matching, using ANGPIX, BINNING_FACTOR, and TM_BOX_SIZE, then set TEMPLATE_MRC to the generated output (usually under templates/). Only skip template generation if the user confirms they already have a PyTom-ready template at exactly ALIGN_ANGPIX = ANGPIX × BINNING_FACTOR and the intended TM box size.

13. TM sphere mask (TM_MASK_MRC) — absolute path to the mask paired with the template; produced by gen_sphere_mask.slurm and consumed by gen_tm_jobs_aretomo.slurm. Default: $WORK_DIR/templates/${TM_LABEL}_mask.mrc. The mask box is read from the template MRC dimensions, and the default sphere radius is derived in pixels as round(DIAMETER / 2 / ALIGN_ANGPIX). Keep MASK_SIGMA=1 unless the user asks for a softer edge; the safety condition is MASK_RADIUS + MASK_SIGMA < TEMPLATE_DIM / 2, so the soft edge fits inside the template box. Both scripts must reference the same mask path — propagate one variable into both.

14. Extraction non-max suppression radius (EXTRACT_MASK_RADIUS, pixels) — in extract_tm_candidates_parallel.slurm (default 14, passed as --mask-radius). Intentionally larger than the sphere-mask MASK_RADIUS; do NOT derive it from round(DIAMETER / 2 / ALIGN_ANGPIX) (that formula yields the sphere radius ~11, not the NMS radius). Two peaks closer than this distance are merged. Wrong value → either duplicate hits (too small) or missed adjacent particles (too large).

15. Candidates per tomogram (NUM_CANDIDATES) — top-N peaks extracted per TS in extract_tm_candidates_parallel.slurm. Over-pick (5000–10000 for crowded specimens, lower for sparse) and filter by score in the resulting STAR.

16. Extraction reference/template name (TEMPLATE) — with this skill's default job layout, gen_tm_jobs_aretomo.slurm creates one job directory per tilt series/tomogram, and run_tm_sequential.slurm runs localization.py inside that directory. PyTom therefore writes scores_<template>.em and angles_<template>.em directly in each job directory (e.g. scores_ribo.em, angles_reference19.em), not under job_dir/<template>/. Always ask the user which template/reference suffix they want to extract, since users commonly run multiple TMs against the same tomograms. Set TEMPLATE to that suffix (e.g. TEMPLATE="ribo", TEMPLATE="26s", or TEMPLATE="reference19"). Only leave empty if the user confirms a single reference per job; the helper will otherwise auto-pick the first matched pair and warn if ambiguous. The extractor can also read per-reference subdirs for externally organized PyTom jobs, but that is not produced by gen_tm_jobs_aretomo.slurm.

17. TM label (TM_LABEL) — one species/template namespace, e.g. ribosome, 26s, hsp. For multiple species, run Phase 6 once per TM_LABEL and keep all intermediate files under template_matching/$TM_LABEL/. Do not share particles/, star_files/, or warp_star/ across species; it becomes impossible to know which picks belong to which template. Prefer keeping TM_LABEL, the generated template basename, and the PyTom extraction TEMPLATE suffix consistent unless the user has an existing naming convention.

OPUS-ET Training

18. Latent dimension (ZDIM) — default 8; increase for more expressivity and more heterogeneous datasets
19. Number of epochs (NUM_EPOCHS) — default 40
20. Number of GPUs — for SLURM (--nproc_per_node)
21. Training decoder size (TEMPLATERES) — OPUS-ET --templateres; the decoder output size should be ~ SUBTOMO_BOX_SIZE × downfrac / 0.75 so the particle occupies ~75% of the decoder output. This is typically smaller than SUBTOMO_BOX_SIZE because the encoder downsamples.
22. Training subtomogram directory (DATADIR) — the subtomogram export directory (e.g. $WORK_DIR/warp_tiltseries/subtomo, or per-species like subtomo_ribo). The training scripts pass --datadir $(dirname "$DATADIR") to OPUS-ET because the STAR file's _rlnImageName entries already include the subdirectory prefix. For mask creation, $DATADIR is used directly to find a sample subtomogram.
23. Training mask (TRAINING_MASK_MRC) — required by OPUS-ET training. Default: $WORK_DIR/templates/${TM_LABEL}_training_mask.mrc. For template-matching filtering, a broad centered sphere mask is acceptable: run gen_training_mask.slurm with MODE="sphere" (the default, soft edge 2 voxels; the dilate/erode morphology applies only in MODE="density"), which samples an exported subtomogram from DATADIR for shape/header (so the output mask matches SUBTOMO_BOX_SIZE at OUTPUT_ANGPIX). The default sphere diameter is 85% of the box (MASK_RADIUS_FRACTION=0.85). Use MODE="density" only when a clean consensus map should define a tighter molecular mask. If the mask is missing at training time and AUTO_CREATE_TRAINING_MASK=1, train_opuset.slurm and train_opuset_fixed.slurm can still create a fallback spherical mask from an exported subtomogram using dsdsh create_mask --sphere-radius.
24. Training geometry overrides (ANGPIX, TILT_RANGE, TILT_STEP) — in train_opuset.slurm and train_opuset_fixed.slurm, leave ANGPIX blank to auto-detect only from _rlnDetectorPixelSize in the input particle STAR file. Do not infer training ANGPIX from OUTPUT_ANGPIX in warp_export_particles.slurm or from warp_tiltseries.settings. Tilt range/step are read from the first .tlt file under TILTSTACK_DIR, normally warp_tiltseries/tiltstack. Set them manually only when the auto-detected values are wrong or the dataset uses non-standard metadata.
25. Fixed-mode subset split — Phase 8c needs two independent particle halves for half-map reconstruction. The input is a selected subset of particles (e.g., from OPUS-ET analysis picking a specific conformational state), not a blind split of the full matching STAR. Once the user has a selected STAR (sel.star), split it with:

    # signature: dsdsh convert_star <starfile> <angpix> [--subset-label N] [--remove-symexp] [--rescale-angpix T]
    # angpix is POSITIONAL (the star's pixel size — OUTPUT_ANGPIX for an OPUS-ET sel.star);
    # there is NO --angpix and NO -o flag. Output is auto-named <starbasename>_subsetN.star.
    dsdsh convert_star sel.star <OUTPUT_ANGPIX> --subset-label 1   # → sel_subset1.star
    dsdsh convert_star sel.star <OUTPUT_ANGPIX> --subset-label 2   # → sel_subset2.star
    

    Run 8c twice, once per subset, with FIXED_SUBSET_LABEL=1 and FIXED_SUBSET_LABEL=2. If the particles were symmetry-expanded (e.g. D3 FAS), de-expand first with dsdsh convert_star sel.star <OUTPUT_ANGPIX> --remove-symexp (one row per rlnImageName), or the two halves each carry symmetry copies of the same particle and the FSC is inflated. You can then re-symmetry-expand each already-disjoint subset for fixed-mode training (relion_particle_symmetry_expand on sel_subset1.star and sel_subset2.star separately, never the pre-split star) → a symmetrized half-map while the two halves stay independent (see references/workflow.md §8.6).

Environment Paths

These are required for ALL phases — collect them first before anything else. 25. Project directory (WORK_DIR) — absolute path where data and scripts will run 26. WARP install path (WARP_DIR) — absolute path to publish/ dir, e.g. /home/user/warp/Release/linux-x64/publish. Must be the alncat fork on the alncat branch (https://github.com/alncat/warp), not upstream https://github.com/warpem/warp: this skill's ts_export_particles calls rely on --dont_correct_ctf_3d and --output_ctf_csv, both of which exist only in the fork (OPUS-ET ingests the per-particle CTF CSV and applies CTF correction internally). Verify with WarpTools ts_export_particles --help | grep dont_correct_ctf_3d — empty output means stock WARP. To install the fork: bash git clone https://github.com/alncat/warp.git cd warp git checkout alncat # Then follow the upstream WARP build instructions to produce # Release/linux-x64/publish/. Point WARP_DIR at that publish/ directory. 27. WARP conda env (WARP_ENV) — e.g. warp_build 28. OPUS-ET conda env (OPUSET_ENV) — e.g. opuset_env 29. PyTOM conda env (PYTOM_ENV) — e.g. pytom_env (template matching phases) 30. conda lib path (CONDA_LIB) — lib/ dir of WARP conda env; derive with: bash conda activate <WARP_ENV> && echo $CONDA_PREFIX/lib e.g. /home/user/.conda/envs/warp_build/lib 31. AreTomo cluster modules (MODULE_CUDA, MODULE_COMPILER) — only warp_aretomo_align_negate.slurm uses module load; set these only if AreTomo2 requires cluster modules on the user's system, otherwise set them to "". 32. SLURM partitions and GPU count — ask once, propagate into every script: - CPU_PARTITION — partition name for CPU-only jobs (scripts shipped as --partition=normal). Examples: normal, compute, cpu. - GPU_PARTITION — partition name for GPU jobs (scripts shipped as --partition=gpu or --partition=normal). Examples: gpu, gpu-a100, volta. - GRES_GPU — full --gres value, e.g. gpu:4, gpu:a100:4, gpu:1. Some sites require the GPU type (gpu:a100:4); check sinfo -o "%G". - NUM_GPUS — integer, must equal the count in GRES_GPU. Used by the training scripts (--nproc_per_node, --num-gpus). These default values in the scripts assume a generic SLURM setup — do not submit without confirming the partition names exist on the user's cluster (sinfo -s lists available partitions).

Optional

33. Output directory prefix (OUTPUT_DIR) — e.g., opuset/${TM_LABEL}/z${ZDIM}

M Refinement

34. Half-maps (M_HALF1, M_HALF2) — after Phase 8d, these default to opuset/<TM_LABEL>/half1.mrc and half2.mrc. User can also provide externally generated half-maps if skipping Phase 8c/8d.
35. Resample pixel size (ANGPIX_RESAMPLE) — MCore working pixel size for species creation. Defaults to $ANGPIX (unbinned detector pixel size). Set to a coarser value for faster refinement with lower memory usage.
36. Half-map mask (M_MASK) — defaults to opuset/<TM_LABEL>/halfmap_mask.mrc from Phase 8d. User can provide a custom mask.
37. Half-map mask threshold (M_HALFMAP_THRESHOLD) — density threshold for creating the half-map mask in Phase 8d. Only positive density above this value is kept. User must provide this.
38. RELION particles STAR (M_PARTICLES_STAR) — RELION-format particle STAR file for MTools create_species. User must provide this.
39. M mask threshold (M_MASK_THRESHOLD) — density threshold for MTools update_mask between MCore passes (optional, only needed if running Md).

Quick Start

1. Copy examples: cp pipeline.example.conf pipeline.conf && cp species.example.conf species.conf
2. Edit pipeline.conf and species.conf — fill all variables (paths, pixel sizes, labels, etc.)
3. Run bash validate.sh --phase 1 — checks placeholders, paths, tools, derived sanity
4. Submit Phase 1: sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_frameseries_import.slurm

Variables Reference

All variables are defined in pipeline.example.conf and species.example.conf — those files are the canonical reference. Copy them to .conf, edit, then run validate.sh to check them. Derived values (ALIGN_ANGPIX, directory paths, etc.) are computed automatically when the configs are sourced.

Configuration (pipeline.conf + species.conf)

Two config files — copy from examples, then edit:

cp pipeline.example.conf pipeline.conf
cp species.example.conf species.conf
vim pipeline.conf    # tilt-series-wide: paths, microscope, detector, cluster, binning
vim species.conf     # per-species: TM_LABEL, DIAMETER, box sizes, training params

pipeline.conf is shared by all species. species.conf is per-species — keep separate copies for different species (e.g. species_ribo.conf, species_26s.conf). Override via SPECIES_CONF=species_26s.conf sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/....

SLURM copies scripts to a temp directory, so $0 is not the original path. Always submit with SKILL_DIR so scripts can find their config files:

sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_frameseries_import.slurm

In scripts, SCRIPT_DIR falls back to $0 if SKILL_DIR is unset:

SCRIPT_DIR="${SKILL_DIR:-$(cd "$(dirname "$0")" && pwd)}"
source "${SCRIPT_DIR}/pipeline.conf" 2>/dev/null || { echo "ERROR: pipeline.conf not found..."; exit 1; }
SPECIES_CONF="${SPECIES_CONF:-${SCRIPT_DIR}/species.conf}"
source "$SPECIES_CONF" 2>/dev/null || { echo "ERROR: $SPECIES_CONF not found..."; exit 1; }

Pre-flight Validation (validate.sh)

Run before submitting any job:

bash validate.sh                        # full check
bash validate.sh --phase 1              # Phase 1 only
bash validate.sh --phase 6 --species species_ribo.conf  # Phase 6, specific species
bash validate.sh --phase 7 --dry-run    # resolve paths + print commands

All pre-submission checks are handled by validate.sh:

• Unresolved placeholders in pipeline.conf, species.conf, and all SLURM scripts
• Environment paths (WORK_DIR, WarpTools, CONDA_LIB)
• Conda environments (WARP_ENV, OPUSET_ENV, PYTOM_ENV)
• Required tools (AreTomo2, dsdsh, etc.) — phase-aware
• Derived value sanity (CTF range ≥ 2×ANGPIX, box covers particle, mask fits template)
• Per-tomostar completion checks for the current phase
• SLURM script syntax (bash -n)
• --dry-run prints resolved paths and commands without submitting

WARP Environment Notes

⚠ ulimit -v unlimited is mandatory. WARP, MTools, MCore, and AreTomo allocate very large virtual address spaces. Without it they fail at startup with cryptic errors. Every shipped SLURM script already includes this line.

WARP_FORCE_MRC_FLOAT32=1 forces 32-bit float MRC outputs (set in every shipped script). Disk-space tradeoff: 32-bit floats ~2× the size of WARP's compact int16 default. Drop the export if downstream tools handle compressed format and disk is tight.

Full Pipeline (SLURM)

# All sbatch commands must pass SKILL_DIR so scripts find pipeline.conf:
#   sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/...

# Phase 1: Frame series
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_frameseries_import.slurm

# Phase 2: Tilt series setup
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_tiltseries_setup.slurm

# Phase 3: Export stacks + AreTomo2 alignment
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_export_stacks.slurm
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_aretomo_align_negate.slurm

# Phase 3.5: REQUIRED — update TOMO_DIMS from AreTomo output
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_update_tomo_dims.slurm

# Phase 4: Import alignments
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_import_alignments.slurm

# Phase 5: CTF + reconstruction
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_ts_ctf.slurm
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_ts_reconstruct.slurm

# 💡 Verify Phase 3–5 alignment chain: AreTomo vs WARP reconstruction dimensions
#    Both are at ALIGN_ANGPIX, so nx × ny × nz must match exactly:
#
#      TS=TS_026
#      headerPyTom warp_tiltseries/tiltstack/$TS/${TS}_ali.mrc | grep 'Number of columns'
#      headerPyTom warp_tiltseries/reconstruction/${TS}_*Apx.mrc | grep 'Number of columns'
#
#    Mismatch → Phase 3.5 skipped, or --alignment_angpix wrong in Phase 4,
#    or TOMO_DIMS X/Y incorrect. Fix the source, re-run from Phase 3.5/4.
#    Details: references/phases.md § sanity check.

# Phase 6: Template matching
# All shared variables are already in pipeline.conf + species.conf.
# Scripts source both automatically — no per-script CONFIG editing needed.
# Agent MUST fill these in species.conf before submitting:
#   TM_LABEL, DIAMETER, TM_BOX_SIZE, SUBTOMO_BOX_SIZE
#   INPUT_MRC, MAP_ANGPIX (template source)
#   NUM_CANDIDATES, EXTRACT_MASK_RADIUS, TEMPLATE (extraction)
# Agent MUST fill these in pipeline.conf:
#   ANGPIX, BINNING_FACTOR (→ ALIGN_ANGPIX derived automatically)
# Script-specific overrides (edit only if defaults don't fit):
#   gen_tm_jobs_aretomo.slurm: SEARCH_REGION=""  (full X/Y, z_start=20)
#   extract_tm_candidates_parallel.slurm: EXTRACT_MASK_RADIUS=14  (non-max suppression)
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/gen_template_from_mrc.slurm
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/gen_sphere_mask.slurm
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/gen_tm_jobs_aretomo.slurm
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/run_tm_sequential.slurm
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/extract_tm_candidates_parallel.slurm
# PyTom XML → per-tilt-series STAR. Canonical path: two SLURM steps below.
# Do not use a combined particles.star here.
# convert_to_star.slurm and convert_pytom_to_warp.slurm must use the same
# TM_LABEL, so they read/write template_matching/$TM_LABEL/star_files and warp_star.
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/convert_to_star.slurm
# convert_to_star.slurm sources pipeline.conf for ANGPIX (unbinned) and BINNING_FACTOR.
# These map to convert.py's --pixelSize and --binPyTom. Verify both are set in pipeline.conf.
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/convert_pytom_to_warp.slurm

# Phase 7: Export subtomograms
# All variables are in pipeline.conf + species.conf — no per-script editing needed.
# Verify in species.conf: TM_LABEL, SUBTOMO_BOX_SIZE, DIAMETER, OUTPUT_ANGPIX
# Verify in pipeline.conf: COORDS_ANGPIX (= ANGPIX)
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/warp_export_particles.slurm

# Phase 8: OPUS-ET training (sub-phases: 8a mask → 8b grad → 8c fixed)
# All variables are in pipeline.conf + species.conf — no per-script editing needed.
# Verify in species.conf: TM_LABEL, ZDIM, NUM_EPOCHS, BATCH_SIZE,
#   SUBTOMO_BOX_SIZE, TEMPLATERES, MASK_SOFT_EDGE, MASK_RADIUS_FRACTION
# Verify in pipeline.conf: NUM_GPUS
# For fixed-mode (Phase 8c): run dsdsh convert_star --subset-label 1 on the Phase 7 STAR first.
# Phase 8b auto-creates a fallback sphere mask if TRAINING_MASK_MRC is missing.
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/gen_training_mask.slurm  # Phase 8a — optional explicit mask
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/train_opuset.slurm        # Phase 8b — heterogeneity
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/train_opuset_fixed.slurm   # Phase 8c — fixed half-maps
sbatch --export=ALL,SKILL_DIR="$(pwd)" scripts/prepare_m_halfmaps.slurm    # Phase 8d — link half-maps + mask

For detailed per-phase commands: read references/phases.md

Phase Summary

SLURM Scripts Reference

For warp_m_update_mask.slurm and warp_m_export.slurm, SPECIES_BASE may be either the original species base name or the full hashed folder name. If m/species/<species>_* matches multiple folders, use the full folder name, e.g. SPECIES_BASE="ribosome_1199b7f2", so one species is selected unambiguously.

All scripts source pipeline.conf (and species.conf for Phase 6+). Fill the config files — not individual scripts. Run validate.sh before submitting to catch any remaining placeholders or path issues.

Cluster-specific SLURM directives (also do this for every script). Scripts ship with generic --partition, --gres, and --time defaults. Before the first submission on a new cluster:

• For scripts with no --gres=gpu:*, replace --partition=normal with --partition=$CPU_PARTITION. This includes CPU-only scripts such as convert_*, gen_*, extract_*, warp_tiltseries_setup, warp_m_setup, warp_m_create_species, warp_m_update_mask, warp_update_tomo_dims, and warp_import_alignments.
• For any script that has --gres=gpu:*, use --partition=$GPU_PARTITION even if the shipped partition is normal. This includes warp_frameseries_import.slurm and warp_export_stacks.slurm.
• Replace the shipped GPU request (--gres=gpu:1, --gres=gpu:4, etc.) with the cluster-specific GPU request and adjust --nproc_per_node / --num-gpus in the training scripts to match $NUM_GPUS.
• --time defaults are guesses (12h CTF, 24h recon, 48h TM, 120h training). If the user knows their cluster's max time or expected scale (e.g. 200 TS vs 20), bump or lower accordingly.

If sinfo -s lists no partition called normal or gpu, do not submit with the shipped defaults — SLURM will reject the job immediately.

Placeholders are caught by validate.sh (see Pre-flight Validation above). It scans pipeline.conf, species.conf, and all SLURM scripts for <placeholder> tokens and /path/to/ defaults.

Deployment Files

Setup: cp pipeline.example.conf pipeline.conf && cp species.example.conf species.conf, then edit both. Scripts exit with a clear error if the real .conf file is missing.

File Organization

Skill deployment files (shipped with the skill):

scripts/                        # SLURM phase scripts (one per phase/sub-phase) + manifest.yml
                                #   + Python helpers: tm_auto_mask.py, extract_candidates_parallel.py, format_slurm.py
references/                     # advanced.md, gotchas.md, phases.md, workflow.md
tests/                          # pytest — test_tm_auto_mask.py
validate.sh                     # Phase-aware pre-flight check (reads scripts/manifest.yml)
pipeline.example.conf           # Copy to pipeline.conf and edit
species.example.conf            # Copy to species.conf and edit (one per species)
pipeline_flowchart.html         # Visual reference
LICENSE

Pipeline runtime output under WORK_DIR:

WORK_DIR/
├── logs/                       # SLURM .out / .err files
├── mdoc/                      # MDOC files
├── tomostar/                  # Canonical tilt series list (*.tomostar)
├── warp_frameseries/          # Phase 1
│   └── average/               # Linked or motion-corrected tilt images
├── warp_tiltseries/           # Phases 2–5, 7
│   ├── tiltstack/TS_XXX/      # Exported stacks + AreTomo output
│   │   ├── TS_XXX.st          # Tilt stack
│   │   ├── TS_XXX.rawtlt      # Raw angles
│   │   ├── TS_XXX_neg.rawtlt  # Negated (for AreTomo)
│   │   ├── TS_XXX_ali.mrc     # AreTomo tomogram
│   │   ├── TS_XXX.xf          # Transforms (for WARP)
│   │   └── TS_XXX.tlt         # Refined angles (for WARP)
│   ├── reconstruction/        # CTF-corrected tomograms (TS_XXX_<apix>Apx.mrc)
│   ├── subtomo/               # Phase 7: exported subtomograms for OPUS-ET
│   │   └── TS_XXX/*.mrc        #   per-tilt-series subtomograms (at OUTPUT_ANGPIX)
│   ├── <TM_LABEL>_matching.star   # Phase 7 export STAR (warp_export_particles)
│   └── <species>_matching_refined.star  # M export STAR, one per species (warp_m_export)
├── templates/                  # Template generation + masks (Phase 6/8)
│   ├── <TM_LABEL>_tm.mrc        #   template at ALIGN_ANGPIX (gen_template_from_mrc)
│   ├── <TM_LABEL>_mask.mrc      #   TM sphere mask (gen_sphere_mask)
│   └── <TM_LABEL>_training_mask.mrc  # training mask (gen_training_mask)
├── template_matching/
│   └── <TM_LABEL>/            # One namespace per species/template
│       ├── jobs/              # PyTOM job XMLs + scores/angles
│       ├── particles/         # Extracted particle XMLs
│       ├── star_files/        # Per-tilt-series PyTom STAR files
│       └── warp_star/         # WARP-compatible STAR files
├── m/                         # Optional MTools / M refinement workspace
│   ├── <population>.population # Created by warp_m_setup.slurm
│   ├── <source>.source        # MTools data source (warp_m_setup.slurm)
│   └── species/
│       └── <species>_<hash>/  # Created by warp_m_create_species.slurm
│           ├── <species>.species
│           ├── *_particles.star
│           ├── *_relion.star  # Produced by warp_m_export.slurm before export
│           ├── <species>_half1.mrc      # M-refined half-maps (warp_m_refine → MCore)
│           ├── <species>_half2.mrc
│           └── <species>_filtsharp.mrc  # sharpened combined map (used for the in-cell render)
└── opuset/                     # Phase 8: OPUS-ET training + heterogeneity analysis
    └── <TM_LABEL>/               #   namespaced by species
        ├── z<ZDIM>/             #   heterogeneity training (e.g. z8; warm-start variant: z8_expanded)
        │   ├── weights.*.pkl
        │   ├── z.*.pkl
        │   ├── config.pkl
        │   ├── analyze.<epoch>/kmeans<numk>/   # Gate-3 states: labels.pkl, center maps, umap.pkl
        │   └── sel_<TM_LABEL>.star             # Gate-3 selected state (select_state.slurm)
        ├── fixed_subset<N>/     #   fixed-mode half-map reconstruction (N = 1, 2)
        │   ├── weights.*.pkl
        │   ├── config.pkl
        │   └── tmp0.mrc         #   the half-map reconstruction
        ├── half1.mrc            #   ← fixed_subset1/tmp0.mrc (prepare_m_halfmaps.slurm)
        ├── half2.mrc            #   ← fixed_subset2/tmp0.mrc
        └── halfmap_mask.mrc     #   molecule mask for M (optional)

Critical Issues (Quick Reference)

• CTF range max > Nyquist: reduce --range_max; must be ≥ 2× angpix
• GLIBCXX error: missing LD_LIBRARY_PATH — set ${CONDA_LIB}:${WARP_DIR}
• OutOfMemory: use 256 GB+, set ulimit -v unlimited, reduce --perdevice to 1
• Wrong tilt convention: WARP writes angles from positive max down to negative min (e.g. +54, +51, …, -54); AreTomo expects negative max up to positive max (e.g. -54, -51, …, +54). Fix: awk '{print -$1}' negates each angle — order is preserved in the respective sign convention.
• WARP tomo_dimensions must be UNBINNED: AreTomo output is binned — multiply by binning factor. Phase 2's initial TOMO_DIMS is only a guess; run Phase 3.5 (warp_update_tomo_dims.slurm) after AreTomo and before Phase 4 to rewrite settings with the true unbinned size. Skipping this silently corrupts coordinates in Phases 5–7.
• Verify after Phase 5 — AreTomo vs WARP reconstruction must agree: tell the user to compare headerPyTom warp_tiltseries/tiltstack/$TS/${TS}_ali.mrc against `headerPyTom warp_tiltseries/reconstru

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