semvec/pypi-packages huggingface dataset:
peepfilt 0.1.4
Filter images without people using YOLOv8 (ultralytics).
Requires Python: >=3.12

# peepfilt

Filter images without people using YOLOv8 (Ultralytics). Supports CLI, FastAPI, and a minimal frontend. Auto-selects CUDA if available, otherwise CPU.

## Install

**For CPU only:**
```bash
pip install peepfilt[cpu]
```

**For GPU (CUDA 12.1):**
```bash
pip install peepfilt[gpu] --extra-index-url https://download.pytorch.org/whl/cu121
```

## CLI

```bash
peepfilt images/ \
  --no-people-dir images/no_people \
  --conf 0.25 \
  --batch-size 16
```

## Web UI

Start the API server with the web interface:

```bash
peepfilt-ui
```

Open `http://localhost:8090` in your browser to access the UI. Endpoints:

- GET `/health` – health check
- POST `/scan-dir` – scan a directory for images without people

## Notes
 
- Model: `yolov8n.pt` (Ultralytics)
- Person class only
- Image size: 640
- Defaults: conf 0.25, batch size 16
stpsf 2.2.0
Creates simulated point spread functions for Space Telescopes (James Webb, Roman)
Requires Python: >=3.10

STPSF: Simulated Point Spread Functions for the James Webb and Nancy Grace Roman Space Telescopes
===================================================================================================

.. image:: https://github.com/spacetelescope/stpsf/blob/stable/docs/readme_fig.png?raw=true

.. image:: https://img.shields.io/pypi/v/stpsf.svg
   :target: https://pypi.python.org/pypi/stpsf
   :alt: Badge showing current released PyPI version

.. image:: https://github.com/spacetelescope/stpsf/workflows/CI/badge.svg?branch=develop
   :target: https://github.com/spacetelescope/stpsf/actions
   :alt: Github Actions CI Status

.. image:: https://codecov.io/gh/spacetelescope/stpsf/branch/master/graph/badge.svg
  :target: https://codecov.io/gh/spacetelescope/stpsf

.. image:: https://zenodo.org/badge/DOI/10.5281/zenodo.15747364.svg
  :target: https://doi.org/10.5281/zenodo.15747364

.. |Documentation Status| image:: https://img.shields.io/readthedocs/stpsf/latest.svg?logo=read%20the%20docs&logoColor=white&label=Docs&version=latest
   :target: https://stpsf.readthedocs.io/en/latest/
   :alt: Documentation Status

.. image:: https://img.shields.io/badge/ascl-1504.007-blue.svg?colorB=262255
   :target: http://ascl.net/1504.007


**STPSF HAS BEEN MIGRATED FROM WEBBPSF**

STPSF produces simulated PSFs for the James Webb Space Telescope, NASA's
flagship infrared space telescope. STPSF can simulate images for any of the
four science instruments plus the fine guidance sensor, including both direct
imaging, coronagraphic, and spectroscopic modes.

STPSF also supports simulating PSFs for the upcoming Nancy Grace Roman Space Telescope (formerly WFIRST),
including its Wide Field Instrument and a preliminary version of the Coronagraph Instrument.

.. note::

   The current (Cycle 10) Roman WFI optical model was calculated by Goddard
   Space Flight Center in September 2024.

Documentation can be found online at https://stpsf.readthedocs.io

STPSF requires input data for its simulations, including optical path
difference (OPD) maps, filter transmission curves, and coronagraph Lyot mask
shapes. These data files are not included in this source distribution.
Please see the documentation to download the required data files.