Improving Test Coverage for the TARDIS Plasma Module
Contributor: Rishmita Rao
The plasma module is used to determine the ionization and excitation states of the supernova ejecta using the basic structure of the supernova...
Exploring supernovae made easy
Contributor: Rishmita Rao
The plasma module is used to determine the ionization and excitation states of the supernova ejecta using the basic structure of the supernova...
Contributor: Shreyans Saraf
Currently, TARDIS relies on IPyWidgets for its visualization modules. While effective within Jupyter environments, these widgets have limited...
Contributor: Haille Perkins
This project will result in functionality for both TARDIS and STARDIS to identify and display a user provided list of atomic and molecular lines to...
Contributor: Riddhi Gangbhoj
TARDIS implements a regression testing framework which is used to compare the current output of TARDIS to a saved data repository to validate code....
Contributor: Asish Kumar
The first half of the project which is writing benchmarks and improving the webpage for storing it. In order to achieve this goal I will be using...
Contributor: Sumit_Gupta
TARDIS provides ways to simulate and analyze supernovae. Currently, as a visualization tool, we have the "Spectral element DEComposition (SDEC)...
Contributor: Sarthak Srivastava
Understanding photon-ion interactions within ejecta is crucial for interpreting astronomical spectra. While the TARDIS SDEC plot visualizes which...
Contributor: Ansh_49
TARDIS operates on a “photospheric” inner boundary approximation. A hard inner boundary in velocity is set from which radiative packets are emitted...
Contributor: Ayushi Daksh
TARDIS generates synthetic observations of stellar explosions that can be compared to real observations. With such comparisons, we can learn more...
Contributor: light2802
Most of the functions in STARDIS generate and loop over huge numpy arrays, that are over a million elements. Initializing the array requires...
Contributor: Shikha Rathi
Carsus generates an HDF file by combining data from various sources. This HDF file can be used by Tardis to generate Atomic Spectra. However, when a...
Contributor: Shreyas Singh
TARDIS has a new module that transports gamma rays created by nuclear decay. The NNDC stores nuclear decay data in a format that is difficult to read...
Contributor: smokestacklightnin
The main goal for this project is to improve the speed of STARDIS, a Python library that generates synthetic spectra for stars. An easy way to...
Contributor: Satwik Kambham
Currently, TARDIS simulations run quickly and thus pausing and resuming a simulation is not necessary. However, future additions to the code may...
Contributor: Jayant bhakar
TARDIS uses a monte carlo method to propagate photon packets through a model of an exploded star. As these virtual packets move through the ejecta...
Contributor: Atharva Arya
This project aims to improve the current Carsus testing framework and add a version key to Carsus output format. Along with this, the project would...
Contributor: Rohith Varma Buddaraju
Tardis is an open-source project designed for rapid spectral modelling of supernovae. Astrophysicists widely use it to model supernovas. When new...