The ASTROnomical POlarimetry and Photometry pipeline
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Updated
Dec 11, 2024 - Python
The ASTROnomical POlarimetry and Photometry pipeline
A pipeline for precise extraction of light curves through forward modelling of a region from time-series wide-field astronomical images
Python Scripts for Data Reduction and Analysis
An Easy GUI for Photometry: MYRaf V3.0!
The ASTROnomical POlarimetry and Photometry pipeline
RAPAS Photometry Pipeline
Web application to search, process, and visualizes the TESS data of any target cataloged in astronomical databases like SIMBAD.
A professional, modular Python library for exoplanet transit photometry analysis. Designed for graduate students, astronomers, and reproducibility-focused researchers.
This project is used to calculate flux level (uJy) at Signal-Noise-Ratio = 5 for faint objects in Spitzer IRAC images. Using IDL we simulate faint objects with IRAC PRF around target position in a grid manner, which could be a possible magnetar.
An opensource package for astronomical photometry
General astronomical image reduction pipeline.
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