Use when authoring or validating PAIDF augmentation YAML configs, or running remote Cosmos Transfer/Predict, image-edit, or image-to-video inference.
Scanned 9/3/2026
Install to Claude Code
npx -y skills add NVIDIA/skills --skill paidf-augmentation --agent claude-codeInstalls into .claude/skills of the current project.
Are you the author of Paidf Augmentation?
Add the live security badge to your README — it updates automatically with every re-scan.
[](https://www.skillsdirectory.com/skills/nvidia-paidf-augmentation)More formats (shields.io, HTML) on the badges page.
---
name: paidf-augmentation
description: >-
Use when authoring or validating PAIDF augmentation YAML configs, or running
remote Cosmos Transfer/Predict, image-edit, or image-to-video inference.
license: Apache-2.0
metadata:
owner: NVIDIA
service: physical-ai-data-factory
version: 1.1.0
reviewed: '2026-08-31'
author: NVIDIA
tags:
- physical-ai
- augmentation
- cosmos
- image-edit
---
# PAIDF Augmentation Pipeline Skill
Unified pipeline for augmenting camera data through NVIDIA generative AI models with automated captioning, generation, and quality evaluation. **BYOM (bring-your-own-model):** every model is reached over a remote HTTP endpoint described by one entry in the config's `endpoints:` list; adding a model is usually a config change, not code.
## Purpose
Use this skill to drive the PAIDF augmentation pipeline end to end:
- **Select the right model** — Cosmos Transfer 2.5 (transform a video), Cosmos Predict 2.5 (generate/extend video), image-edit (edit an image), or image-to-video (animate a first frame: Cosmos3 or Veo 3.1).
- **Author and validate YAML configs** against the `PipelineConfig` Pydantic schema.
- **Configure captioning** (VLM, LLM, deterministic VLM-template, text, or file) and **evaluators** (hallucination check, attribute verification, VLM verification).
- **Launch and run** inference inside the `paidf-augmentation:1.1.0` Docker container (remote-API only — no local model weights).
Use this skill when running inference, authoring or editing configs, debugging validation or runtime errors, adding data samples, configuring captioning, tuning generation parameters, registering BYOM endpoints/adapters, or setting up evaluators. Trigger keywords: augmentation, cosmos transfer, cosmos predict, image edit, image-to-video, veo, image attribute augmentation, defect image generation, captioning, attribute verification, config validation.
Do **not** use this skill for training or fine-tuning models, deploying clusters or NIM endpoints, or unrelated application/database development.
## Prerequisites
| Requirement | Detail |
|-------------|--------|
| **Docker** | `docker --version`. The image is **remote-API only** — it bundles no Cosmos/torch weights, so plain remote inference needs **no GPU and no `HF_TOKEN`**. |
| **NVIDIA GPU** (conditional) | Only for the `data_processing.alignment` post-processor (cupy) and **H.264** decode (evaluators, `data_processing.transcode`). See Limitations. |
| **Endpoint URLs** | One reachable URL per role the config uses: the model role (`video_transfer`/`video_predict`/`image_edit`/`image2video`) plus `vlm`/`llm` for captioning and evaluation. Defaults are local Qwen vLLM servers (`Qwen/Qwen3.6-27B-FP8` on `vlm`, `Qwen/Qwen2.5-14B-Instruct` on `llm`). If the user has none running, ask for URLs. |
| **API keys** (conditional) | Only for endpoints requiring auth. Passed by env var named in each endpoint's `api_key_env` — never hardcoded in YAML. Common: `VLM_API_KEY`, `LLM_API_KEY`, `VEO_API_KEY`, `BUILD_NVIDIA_API_KEY`. Local endpoints need none. |
| **Input media** | A video (transfer/predict) or image (edit/image2video) reachable by `multistorageclient` — local path, `s3://`, `gs://`, `az://`, or HTTP. |
## Inputs
Resolve each value in this precedence order: **state file → explicit prompt arguments → agent context → user prompt.** Ask the user only for what remains unresolved.
| Input | Required | Description |
|-------|----------|-------------|
| `config_path` | Yes | Path to the pipeline YAML, e.g. `configs/cookbook/video-data-augmentation/config_video_transfer_CT25_nim.yaml`. If absent, pick a starting config from *Supported Models* and confirm with the user. |
| `input_media` | Yes | Source video/image → `data[].inputs.rgb`. Overridable at run time via `data.0.inputs.rgb=...`. |
| `output_paths` | Yes | `data[].output.{video,caption,metadata}`; `evaluation` optional. |
| `model_name` | Yes | `augmentation.model.name` — an endpoint `id`, a role, or a known model name. Free-form string, not an enum. |
| `endpoint_urls` | Yes | One `endpoints[]` entry per role in use. |
| `api_key_env` | If auth | Env-var *name* per endpoint; the value comes from the environment. |
| `target_attributes` | No | `captioning.llm.variables` (e.g. `weather_condition`, `lighting_condition`). |
| `generation_params` | No | `augmentation.parameters` — pass-through; only set knobs are sent. |
| `seed` | No | Under `augmentation.parameters`; `null` = random, re-rolled on retry. |
## BYOM model: endpoints, adapters, roles
The pipeline never embeds an SDK per model. Instead:
- **`endpoints:` is a list.** Each entry has `role`, `url`, `model` (the wire model string), an optional `id` (only to disambiguate 2+ endpoints sharing a role), an optional `adapter` (API contract; defaults from the role), `api_key_env`, and `timeout`.
- **Roles**: `vlm`, `llm` (captioning + evaluators), `image_edit`, `video_transfer` (Cosmos Transfer), `video_predict` (Cosmos Predict), `image2video` (Cosmos3 / Veo).
- **Adapters (API contracts)**: `openai.chat.completions`, `openai.images.edits`, `openai.video.sync`, `openai.video.async`, `nim`, `passthrough`. The same model can be served over different contracts by changing only the endpoint's `adapter` field.
- **Model selection**: `augmentation.model.name` resolves to an endpoint by `id`, else by `role`, else by the model-name→role map (`image-edit`→`image_edit`, `cosmos-transfer2.5`→`video_transfer`, `cosmos-predict`→`video_predict`, `cosmos3-image2video`→`image2video`).
## Supported Models
When the user hasn't specified a model, choose from their **input type and goal**:
| Input Type → Goal | `model.name` | Role / default adapter | Input → Output |
|-------------------|--------------|------------------------|----------------|
| Video — change scene attributes (weather, lighting, style) | `cosmos-transfer2.5` | `video_transfer` / `nim` | Video (+ controls) → Video |
| Video + text — extend or predict continuation | `cosmos-predict` | `video_predict` / `nim` | Video+Text → Video |
| Text only — generate video from scratch | `cosmos-predict` (`inference_type: text2world`) | `video_predict` / `nim` | Text → Video |
| Image — edit specific attributes | `image-edit` | `image_edit` / `nim` (or `openai.chat.completions`, `openai.images.edits`) | Image → Image |
| Image — animate a first frame | `cosmos3-image2video` (or your Veo endpoint id) | `image2video` / `openai.video.sync` (Veo: `openai.video.async`) | Image + prompt → Video |
**Key rule**: video in + scene-attribute change → **Cosmos Transfer**. Generate new video from text/image/video conditioning → **Cosmos Predict**. Single image edit → **image edit**. Still image → moving clip → **image-to-video**.
All models run via remote HTTP through one `BaseExecutor`; there is no local `torchrun` and no `executor_type` field.
## Usage
### Step 1: Launch the Docker Container
Set `PAIDF_IMAGE_ID` to the immutable `sha256:` image ID recorded from the
trusted local build (or supplied in trusted release metadata). The image ID is
build- and architecture-specific, so this repository cannot provide one
universal value. Verify that the mutable convenience tag still resolves to the
expected ID, then run the ID directly:
```bash
set -e
PAIDF_IMAGE_ID="sha256:<expected-image-id>"
test "$(docker image inspect --format '{{.Id}}' paidf-augmentation:1.1.0)" = "$PAIDF_IMAGE_ID"
docker network inspect paidf >/dev/null 2>&1 || \
docker network create paidf
docker run -it --rm \
--network paidf \
-v "$(pwd)/modules:/workspace/modules" \
-v "$(pwd)/configs:/workspace/configs" \
-v "$(pwd)/data:/workspace/data" \
--entrypoint /bin/bash \
"$PAIDF_IMAGE_ID"
```
Do not derive `PAIDF_IMAGE_ID` from the tag and immediately trust it; compare
the tag against the digest recorded when the image was built or published. If
a registry release provides a signed manifest, verify that signature before
pulling and use its `name:tag@sha256:<manifest-digest>` reference instead.
- **Networking:** augmentation only makes outbound requests, so it needs no
`-p`/`--publish` ports. Keep the shared `paidf` bridge shown above for remote
endpoints. For another model container, attach it to the same bridge and use
its container name in the endpoint URL. Run host-local models in a container
on that bridge, or use a remote endpoint; do not grant the augmentation
container access to the host network.
- **API keys:** prefer a platform secrets manager that injects the required
environment variables. Otherwise, export only the required keys and forward
their names with `-e VAR_NAME`; never mount or load a broad credential file.
- **No GPU needed for remote inference** — add `--gpus` for `data_processing.alignment` and any **H.264** decode; pick a GPU not shared with a busy model server. Container runs as uid 10000; ensure `data/` is writable (or `--user "$(id -u):$(id -g)"`).
> **Security:** Host networking is prohibited for this workflow, especially
> when API keys are present. Review
> [pipeline-operations.md](references/pipeline-operations.md#security-notes).
### Step 2: Run the Pipeline (Inside the Container)
```bash
uv run --no-sync modules/cli.py --config configs/<config_file>.yaml
# With OmegaConf CLI overrides (dot-list syntax)
uv run --no-sync modules/cli.py --config configs/cookbook/video-data-augmentation/config_video_transfer_CT25_nim.yaml \
data.0.inputs.rgb=/workspace/data/input.mp4 \
augmentation.parameters.seed=42
```
Environment variables: keys resolve as the `api_key_env` var → the role's default env var. If `api_key_env` names an **unset** var, resolution falls back to the role default; leave it off for unauthenticated endpoints. `LOG_LEVEL` sets logging.
## Configuration Schema
Configs are validated against `PipelineConfig` (`modules/aug_utils/schema/`) and have seven top-level sections: `data`, `endpoints` (a **list**), `pipeline`, `captioning`, `augmentation`, `data_processing`, and `evaluators`. Full per-section YAML is in [configuration-schema.md](references/configuration-schema.md); runtime flow and common editing tasks are in [pipeline-operations.md](references/pipeline-operations.md).
## Examples
> Configs live under `configs/cookbook/<use-case>/`. See the [cookbook index](../../configs/cookbook/README.md) for the folder layout.
| Use case | Config(s) |
|----------|-----------|
| Video scene-attribute transfer (CT2.5, `nim`) | `config_video_transfer_CT25_nim.yaml` |
| Image → video | `config_image2video_cosmos3.yaml` (VLM→LLM) · `config_image2video_cosmos3_vlm_template.yaml` (VLM→template) · `config_image2video_veo31.yaml` (Veo 3.1, async) |
| Image Attribute Augmentation | `config_image_edit_attribute_{chat_api,images_api,nim}.yaml` · `…_gemma_llm.yaml` (hosted-Gemma LLM swap) |
| Defect Image Generation + MI alignment | `config_image_edit_defect_{chat_api,images_api}.yaml` |
| Batch config generation | `workflow_example.yaml` · `attribute_distribution_1000_v1.yaml` |
| Smart-space seed image / event video | `config_seed_image_gen_cosmos3_super_t2i_smart_spaces.yaml` · `config_event_video_gen_cosmos3_smart_spaces.yaml` |
Per-config captioning / evaluator / adapter details are in [config-decision-tree.md](references/config-decision-tree.md).
## Troubleshooting
Run all inference and schema validation **inside the Docker container** for a consistent environment. For config-validation errors, runtime/endpoint errors, and typical per-stage timings, see [troubleshooting.md](references/troubleshooting.md).
## Limitations
- **Remote inference only.** All models run behind remote HTTP endpoints; no local weights, no `torchrun`, no `executor_type`, no Gradio executor.
- **GPU for alignment and H.264 decode.** Remote inference needs no GPU. A CUDA GPU is required by `data_processing.alignment` (cupy) and by anything decoding H.264 — the evaluators and `data_processing.transcode` — because the image ships only the hardware `h264_cuvid` decoder (software AVC decode is off for licensing). VP9 decodes in software. Video **output** is VP9-only.
- **Inference only.** This pipeline augments and generates media — it does not train or fine-tune models.
- **Auth varies by endpoint.** Hosted endpoints (e.g. Veo) need a key via `api_key_env`; local endpoints (e.g. vLLM) need none.
## Reference files
- [configuration-schema.md](references/configuration-schema.md) — full per-section YAML for every config section.
- [config-decision-tree.md](references/config-decision-tree.md) — which config to start from, model/captioning selection, alignment override rules.
- [pipeline-operations.md](references/pipeline-operations.md) — pipeline flow, worked example, common tasks, storage, security notes.
- [captioning-strategy-guide.md](references/captioning-strategy-guide.md) — all 6 captioning modes with complete YAML.
- [evaluator-setup-guide.md](references/evaluator-setup-guide.md) — hallucination tuning, attribute verification, MCQ wiring.
- [troubleshooting.md](references/troubleshooting.md) — validation/runtime errors and per-stage timings.
- [image-attribute-augmentation.md](references/image-attribute-augmentation.md) — Image Attribute Augmentation image-edit workflow and dataset packaging.
- [event-video-gen.md](references/event-video-gen.md) — smart-space image-to-video event generation.
Is this your skill, or is something wrong with this listing? Request removal or report an issue. Author removals are honored within 72 hours.
No comments yet. Be the first to comment!