STDWeb Documentation ==================== **STDWeb** (Simple Transient Detection for the Web) is a web-based tool for quick-look photometry and transient detection in astronomical images. It is based on the `STDPipe `_ library and implements a self-consistent, mostly automatic data analysis workflow. Features -------- - Upload your own FITS files or analyze files already on the server - Basic pre-processing and masking - Object detection with astrometric calibration (blind matching or WCS refinement) - Photometric calibration using multiple reference catalogs - Template subtraction with automatically downloaded or user-provided templates - Forced photometry for specified targets in original or difference images - Transient detection in difference images For details on the underlying routines, see the `STDPipe documentation `_ and `example notebooks `_. Supported Photometric Filters ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ - **Johnson-Cousins**: U, B, V, R, I - **Sloan/Pan-STARRS**: u, g, r, i, z, y - **Gaia**: G, BP, RP Reference Catalogs ~~~~~~~~~~~~~~~~~~ - Gaia DR3 synthetic photometry - Pan-STARRS DR1 - SkyMapper DR4 - SDSS DR16 - ATLAS-REFCAT2 - DES DR2 Template Sources ~~~~~~~~~~~~~~~~ - Pan-STARRS DR2 - Legacy Survey DR10 - SkyMapper DR4 - DES DR2 - DECaPS DR2 - ZTF DR7 Citation -------- If you use STDWeb in your work, please cite: Karpov, S. (2025). **STDweb: simple transient detection pipeline for the web**. *Acta Polytechnica*, 65(1), 50-64. https://doi.org/10.14311/AP.2025.65.0050 .. toctree:: :maxdepth: 2 :caption: Contents: installation configuration architecture api workflow handbook Indices and tables ================== * :ref:`genindex` * :ref:`search`