cpinte
I am an astrophysicist working at Monash University, Melbourne, Australia and at Institute for Planetary sciences and Astrophysics, Grenoble, France.
Pinned Repositories
adda
ADDA - light scattering simulator based on the discrete dipole approximation
ads2bibdesk
ads2bibdesk helps you add astrophysics articles listed on NASA/ADS to your BibDesk database using the new ADS Developer API
aggregate
Some python codes to generate various aggregate particles (e.g. ballistic particle cluster, and cluster-cluster).
Analytical_Kinks
casa_cube
python tool to display and analysis astronomical data cubes
disksurf
Measure the molecular emission surface of protoplanetary disks. Based on Pinte et al. (2018).
dynamite
DYNamical Analysis and MultIscale Tomography of line Emission
mcfost
MCFOST radiative transfer code
pymcfost
python interface to the 3D radiative transfer code mcfost
yomcfost
yorick interface to the 3D radiative transfer code mcfost
cpinte's Repositories
cpinte/mcfost
MCFOST radiative transfer code
cpinte/pymcfost
python interface to the 3D radiative transfer code mcfost
cpinte/aggregate
Some python codes to generate various aggregate particles (e.g. ballistic particle cluster, and cluster-cluster).
cpinte/casa_cube
python tool to display and analysis astronomical data cubes
cpinte/dynamite
DYNamical Analysis and MultIscale Tomography of line Emission
cpinte/yomcfost
yorick interface to the 3D radiative transfer code mcfost
cpinte/adda
ADDA - light scattering simulator based on the discrete dipole approximation
cpinte/csalt
Circumstellar Spectral Analysis with Line Tomography
cpinte/get_moments
Fortran 90 module for maximum entropy based reconstruction of a function from its moments
cpinte/astrochem
A code to compute the abundances of chemical species in the interstellar medium
cpinte/Awesome-CV
:page_facing_up: Awesome CV is LaTeX template for your outstanding job application
cpinte/celeritas
Celeritas is a new Monte Carlo transport code designed to accelerate scientific discovery in high energy physics by improving detector simulation throughput and energy efficiency using GPUs.
cpinte/disc_fitting
Fitting disc parameters with MCFOST models
cpinte/elias2-24
cpinte/exojax
🐈 Automatic differentiable spectrum modeling of exoplanets/brown dwarfs using JAX, compatible with NumPyro and JAXopt
cpinte/GMM-Aggregates
calculations of optical properties of dust grain. used for creating aggregates and calculating the optical properties via the generalised multi-wavelength Mie theory
cpinte/idefix
A new finite volume code designed to run on many architectures, such as GPU, CPU and manycores, using Kokkos.
cpinte/miepy
Python module to solve Maxwell's equations for a cluster of particles using the generalized multiparticle Mie theory (GMMT)
cpinte/MSTM
Multiple Sphere T Matrix code
cpinte/phantom
Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code
cpinte/phantom-build
phantom-build is designed to make building Phantom easier
cpinte/phantom-setup
phantom-setup: generate initial conditions for Phantom simulations
cpinte/planet-disk-modes-cooling
Solve the linear perturbation equations for planet-disk interaction with cooling
cpinte/sarracen
cpinte/SHIFT
Fourier transforms in polar and spherical polar coordinates.
cpinte/spiralmoments
cpinte/StringiFor
Strings Fortran Manipulator with steroids
cpinte/UVMultiFit
UVMULTIFIT is a versatile library for fitting models directly to visibility data, currently implemented in CASA. These models can depend on frequency and fitting parameters in an arbitrary algebraic way.
cpinte/visread
Small tools to help export and process visibilities.
cpinte/wakeflow
Implementation of semi-analytic method for modelling planetary wakes in protoplanetary disks.