The ASTROnomical POlarimetry and Photometry pipeline
-
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.
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.
Add a description, image, and links to the photometry-pipeline topic page so that developers can more easily learn about it.
To associate your repository with the photometry-pipeline topic, visit your repo's landing page and select "manage topics."