Following packages are used for analysis of data sets from ALMA , EVLA, Parkes, VLA etc.
http://www.aips.nrao.edu/
http://casa.nrao.edu/
VLA data reduction: https://casaguides.nrao.edu/index.php/Karl_G._Jansky_VLA_Tutorials
Material and Jupyter notebooks associated with the Large Synoptic Survey Telescope Corporation (LSSTC) Data Science Fellowship Program (DSFP). The LSSTC DSFP is a two year training program designed to teach skills required for LSST science that are not easily addressed by current astrophysics programs.
Tutorial notebooks for the Rubin Observatory LSST Science Pipelines
Access to all ZTF data products is through the online (GUI-based) web-tools and API services of the NASA/IPAC Infrared Science Archive (IRSA) linked from: https://irsa.ipac.caltech.edu/Missions/ztf.html.
To visualize, analyze, and retrieve any of the file-based products (single-exposure science or reference images, and/or their catalogs or other files), use the following GUI: https://irsa.ipac.caltech.edu/applications/ztf/. You can supply a sky position, a list of positions, or names of objects that can be resolved, including Solar System objects or an orbital ephemeris. The query returns the CCD-quadrant images touching these positions and metadata for additional filtering.
Quick data reduction code for ALFOSC spectra. This code reduces ALFOSC@NOT spectra, obtained with the grism #4 (ver 0.1) and provides a flux-calibrated spectrum using old calibration files.
1D extraction of long-slit spectroscopy
https://keheintz.github.io/PyReduc/
PypeIt is a Python package for semi-automated reduction of astronomical, spectroscopic data. Its algorithms build on decades-long development of previous data reduction pipelines. Support for 20+ Spectrographs;
From HST directly
An all-in-one script for downloading, registering, and drizzling HST images, running dolphot, and scraping data from dolphot catalogs. This script is optimized to obtain photometry of point sources across multiple HST images.
Galaxy Evolution Explorer (GALEX) mission surveyed the sky in the ultraviolet for approximately ten years between April 2003 and June 2013. The gPhoton database and associated software tools now give researchers the means to use photon-level GALEX data up through General Release (GR) 6/7. The gPhoton command line tools permit users to search for coverage within this database and create calibrated light curves, images, or movies, with the flexibility to set time and spatial ranges or cuts across the entire mission. This enables studies of variability at timescales shorter than the GALEX visit files, customization or refinement of the calibration, and simplifies the fusion of data across mission phases, surveys and modes. When imported as Python modules, gPhoton permits even more detailed work with the data, including analysis at the level of individual photons.
https://swift.gsfc.nasa.gov/analysis/UVOT_swguide_v2_2.pdf
CIAO is the software package developed by the Chandra X-Ray Center for analysing data from the Chandra X-ray Telescope. It can also be used with data from other Astronomical observatories, whether ground or space based.
Marx is a suite of programs created and maintained by the MIT/CXC/HETG group group and is designed to enable the user to simulate the on-orbit performance of the Chandra X-ray Observatory.
The Science Analysis System (SAS) is a collection of tasks, scripts and libraries, specifically designed to reduce and analyze data collected by the XMM-Newton observatory.
https://www.cosmos.esa.int/web/xmm-newton/download-and-install-sas
Analysis threads: https://www.cosmos.esa.int/web/xmm-newton/sas-threads
ISIS, the Interactive Spectral Interpretation System, is designed to facilitate the interpretation and analysis of high resolution X-ray spectra. It is being developed as a programmable, interactive tool for studying the physics of X-ray spectrum formation, supporting measurement and identification of spectral features, and interaction with a database of atomic structure parameters and plasma emission models. A collection of useful ISIS scripts: http://www.sternwarte.uni-erlangen.de/isis/
SPEX is a software package optimized for the analysis and interpretation of high-resolution cosmic X-ray spectra. The software is especially suited for fitting spectra obtained by current X-ray observatories like XMM-Newton, Chandra, Suzaku, and Hitomi.
An X-Ray Spectral Fitting Package
https://heasarc.gsfc.nasa.gov/xanadu/xspec/
Quickstart: https://github.com/fermi-lat/Fermitools-conda/wiki
Analysis threads: https://fermi.gsfc.nasa.gov/ssc/data/analysis/scitools/