Pinned Repositories
bib
my library
corv
Compact Object Radial Velocities
hsl_python
research code from the Human Spaceflight Lab at the Johns Hopkins School of Medicine.
hsltools
a multipurpose package for all your physiological signal processing needs.
merlin
end-to-end reduction and analysis pipeline for magE spectra
mpms
searching for cool population iii stars disguised as white dwarfs
starwave
modeling resolved stellar populations with bayesian inference
wdtools
computational tools for the spectroscopic analysis of white dwarfs
vedantchandra's Repositories
vedantchandra/wdtools
computational tools for the spectroscopic analysis of white dwarfs
vedantchandra/corv
Compact Object Radial Velocities
vedantchandra/merlin
end-to-end reduction and analysis pipeline for magE spectra
vedantchandra/starwave
modeling resolved stellar populations with bayesian inference
vedantchandra/hsl_python
research code from the Human Spaceflight Lab at the Johns Hopkins School of Medicine.
vedantchandra/hsltools
a multipurpose package for all your physiological signal processing needs.
vedantchandra/bib
my library
vedantchandra/mpms
searching for cool population iii stars disguised as white dwarfs
vedantchandra/chandra
my code
vedantchandra/doppler
General radial velocity determination software
vedantchandra/isochrones
Pythonic stellar model grid access; easy MCMC fitting of stellar properties
vedantchandra/marcc
code backup for astronomy work on the Blue Crab computing cluster at MARCC
vedantchandra/prospector
Python code for Stellar Population Inference from Spectra and SEDs
vedantchandra/pydis
A simple longslit spectroscopy pipeline in Python
vedantchandra/Sequencer
An algorithm that detects one-dimensional sequences in complex datasets
vedantchandra/spaceflight-adaptation
multidimensional analysis of human health and performance in relation to long-duration spaceflight
vedantchandra/vedantchandra.github.io
my website
vedantchandra/WD_models
I provide a python module for transformations between WD photometry (Gaia, SDSS, Johnson, and 2MASS passbands) and physical parameters, based on interpolation of existing atmosphere grid and cooling models. If you use this tool, please cite this website and the corresponding papers of atmosphere grid (synthetic colors) and cooling models.