ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

Browsing Codes

Results 1-100 of 3860 (3759 ASCL, 101 submitted)

Previous

12 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 Next

Order

Title Date

▲ ▼

Mode

Abstract Compact

Per Page

50100250 All

[submitted] SOAP: A Python Package for Calculating the Properties of Galaxies and Halos Formed in Cosmological Simulations

[submitted] QUIDS: Q/U Integrated Dust Shells

[ascl:2507.018] ysoisochrone: Python package to estimate masses and ages for young stellar objects

[ascl:2507.017] spectool: Spectral data processing and analysis toolkit

[ascl:2507.016] spinifex: Ionospheric corrections

[ascl:2507.015] nGIST: The new Galaxy Integral-field Spectroscopy Tool

[ascl:2507.014] SAUSERO: Software to AUomatize in a Simple Environment the Reduction of Osiris+

[ascl:2507.013] Sapphire++: Interaction of charged particles with a background plasma simulator

[ascl:2507.012] arctic_weather: High Arctic meteorological conditions analyzer

[ascl:2507.011] COBRA: Optimal Factorization of Cosmological Observables

[ascl:2507.010] show_cube: Show reduced spectra for Gemini NIFS

[ascl:2507.009] Coniferest: Python package for active anomaly detection

[ascl:2507.008] tayph: Cross-correlation analysis of high resolution spectroscopy

[ascl:2507.007] Nii-C: Automatic parallel tempering Markov Chain Monte Carlo framework

[ascl:2507.006] OW: Opacity Wizard

[ascl:2507.005] SysSimPyMMEN: Infer the minimum-mass extrasolar nebula

[ascl:2507.004] SysSimPyPlots: Functions for plotting galleries of systems

[ascl:2507.003] SysSimExClusters: Clustered planetary system model for SysSim

[ascl:2507.002] LSCS: High-contrast space telescopes simulator

[ascl:2507.001] ExoplanetsSysSim: Exoplanet System Simulation

[submitted] spherimatch: A Python package for cross-matching and self-matching in spherical coordinates

[submitted] Modified Teukolsky Framework for Environmentally- Coupled Black Hole Ringdown: A Physics-Informed Neural Network Approach for Improved Gravitational Wave Analysis

[ascl:2506.025] Procoli: 1D profile likelihood extractor

[ascl:2506.024] CAMEL: Cosmological parameters estimator

[ascl:2506.023] pinc: Compute profile likelihoods in cosmology

[submitted] OK Binaries Interactive Catalog

[ascl:2506.022] CLUES: Clustering tool for analyzing spectral data

[ascl:2506.021] Bjet_MCMC: Model multiwavelength spectral energy distributions of blazars

[ascl:2506.020] pynchrotron: Synchrotron emission from cooling electrons

[ascl:2506.019] astromodels: Spatial and spectral models for astrophysics

[ascl:2506.018] 3ML: Framework for multi-wavelength/multi-messenger analysis

[ascl:2506.017] hydromass: Hydrostatic mass profile reconstruction

[ascl:2506.016] SBI++: Simulation-based (likelihood-free) inference for astronomical applications

[ascl:2506.015] Octofitter: Bayesian inference against exoplanet and binary star data

[ascl:2506.014] M_-M_K-: Estimate masses and uncertainties from M_Ks (2MASS Ks + distance)

[ascl:2506.013] OCSVM-Transit-Detection: One-Class SVM model for exoplanet transit detection

[ascl:2506.012] pyTPCI: Python version of The Pluto-Cloudy Interface

[ascl:2506.011] TPCI: The PLUTO CLOUDY interface

[ascl:2506.010] easyCHEM: Chemical abundances in exoplanet atmospheres calculator

[ascl:2506.009] GRIP: Generic data Reduction for nulling Interferometry Package

[ascl:2506.008] DART-Vetter: Convolutional Neural Network to distinguish planetary transits from false positives

[ascl:2506.007] excalibuhr: High-resolution spectral data reduction

[ascl:2506.006] Gen TSO: Graphical interface to simulate JWST exoplanet time-series observations

[ascl:2506.005] VBMicrolensing: Microlensing computations for single, binary, and multiple lenses

[ascl:2506.004] TESS-cont: TESS contamination tool

[ascl:2506.003] SMART: Forward-modeling framework for spectroscopic data

[ascl:2506.002] MAGIC: Automatic analysis of realistic microlensing light curves

[ascl:2506.001] CTD: Cumulative Time Dilation

[ascl:2505.020] Hibridon: Time-independent non-reactive quantum scattering calculations

[ascl:2505.019] AIRI: Algorithms for computational imaging

[ascl:2505.018] SCATTERING: Solve the coupled equations for a given scattering system

[ascl:2505.017] TD-CARMA: Estimates of gravitational lens time delays with flexible CARMA processes

[ascl:2505.016] iSLAT: Interactive Spectral-Line Analysis Tool

[ascl:2505.015] CETRA: Cambridge Exoplanet Transit Recovery Algorithm

[ascl:2505.014] afterglowpy: Compute and fit GRB afterglows

[ascl:2505.013] tBilby: Transdimensional inference for gravitational-wave astronomy with Bilby

[ascl:2505.012] ExoLyn: Multi-species cloud modeling in atmospheric retrieval

[ascl:2505.011] eclipsoid: Transit models for ellipsoidal planets in Jax

[ascl:2505.010] Exo-MerCat: Exoplanet Merged Catalog with Virtual Observatory connection

[ascl:2505.009] BEM: Random forest for exoplanets

[ascl:2505.008] Aeolus: Object-oriented analysis of atmospheric model output

[ascl:2505.007] Jitter: RV jitter prediction code

[ascl:2505.006] jnkepler: Differentiable N-body model for multi-planet systems

[ascl:2505.005] NumPyro: Probabilistic programming with NumPy

[ascl:2505.004] Eureka!: Data reduction and analysis pipeline for JWST and HST time-series observations

[ascl:2505.003] pyGCG: Python Grism Classification GUI

[ascl:2505.002] SWIFTGalaxy: Galaxy particle analyzer

[ascl:2505.001] speclib: Tools for working with stellar spectral libraries

[submitted] Fourier Power Spectrum Pipeline for Multitracer Fisher Forecasting.

[submitted] infrared_comparison: Compare the thermal-infrared sky brightness of polar and mid-latitude sites

[submitted] arctic_mass_dimm: Estimate seeing conditions measured with MASS/DIMM at Eureka/PEARL, compare to other sites

[submitted] allsky: Estimate atmospheric transparency via photometry with PASI at Eureka/PEARL, compare to other sites

[submitted] astromorph: self-supervised machine learning pipeline for astronomical morphology analysis

[ascl:2504.035] SHELLFISH: SHELL Finding In Spheroidal Halos

[ascl:2504.034] JOFILUREN: Wavelet code for data analysis and de-noising

[ascl:2504.033] Vela.jl: Bayesian pulsar timing and noise analysis

[ascl:2504.032] DMCalc: In-band dispersion measure of pulsars calculator

[ascl:2504.031] TempoNest: Bayesian analysis tool for pulsar timing

[ascl:2504.030] kotekan: High performance radio data processing pipeline

[ascl:2504.029] GNURadio: Software Radio Ecosystem

[ascl:2504.028] jaxoplanet: Astronomical time series analysis with JAX

[ascl:2504.027] picasso: Painting intracluster gas on gravity-only simulations

[ascl:2504.026] Flax: Neural network library for JAX

[ascl:2504.025] RFIClean: Mitigation of periodic and spiky RFI from filterbank data

[ascl:2504.024] PDQ: Predict Different Quasars

[ascl:2504.023] AstroPT: Transformer for galaxy images and general astronomy

[ascl:2504.022] MultiREx: Massive planetary spectra generator

[ascl:2504.021] GalClass: Visual Galaxy Classification tool

[ascl:2504.020] ChromaStarPy: Python stellar atmosphere and spectrum modeling code

[ascl:2504.019] ExoInt: Devolatilization and interior modeling package for rocky planets

[ascl:2504.018] tpfplotter: TESS target pixel file plotter

[ascl:2504.017] Pytmosph3R: Compute transmission spectra of planets with a 1D, 2D, or 3D atmospheric structure

[ascl:2504.016] TROPF: Tidal Response Of Planetary Fluids

[ascl:2504.015] DYNAMITE: DYNAmical Multi-planet Injection TEster

[ascl:2504.014] CHIMERA: CaltecH Inverse ModEling and Retrieval Algorithms

[ascl:2504.013] VSPEC: Variable Star PhasE Curve

[ascl:2504.012] Turbospectrum_NLTE: Turbospectrum 2020 with NLTE capability

[ascl:2504.011] TriArc: Detecting trace gases in exoplanet atmospheres

[ascl:2504.010] tglc: TESS full-frame image light curves

[ascl:2504.009] SWAMPE: 2D spectral-core shallow-water exoplanet atmosphere model

Previous

12 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 Next

Would you like to view a random code?