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Results 3551-3600 of 3737 (3631 ASCL, 106 submitted)

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[ascl:1102.002] PBL: Particle-Based Lensing for Gravitational Lensing Mass Reconstructions of Galaxy Clusters
[ascl:1102.003] GRAVLENS: Computational Methods for Gravitational Lensing
[ascl:1102.004] LENSTOOL: A Gravitational Lensing Software for Modeling Mass Distribution of Galaxies and Clusters (strong and weak regime)
[ascl:1102.005] MRLENS: Multi-Resolution methods for gravitational LENSing
[ascl:1102.006] NBODY Codes: Numerical Simulations of Many-body (N-body) Gravitational Interactions
[ascl:1102.007] PixeLens: A Portable Modeler of Lensed Quasars
[ascl:1102.008] PMFAST: Towards Optimal Parallel PM N-body Codes
[ascl:1102.009] AHF: Amiga's Halo Finder
[ascl:1102.010] SEREN: A SPH code for star and planet formation simulations
[ascl:1102.011] Identikit 2: An Algorithm for Reconstructing Galactic Collisions
[ascl:1102.012] CPROPS: Bias-free Measurement of Giant Molecular Cloud Properties
[ascl:1102.013] Cactus: HPC infrastructure and programming tools
[ascl:1102.014] Einstein Toolkit for Relativistic Astrophysics
[ascl:1102.015] PMFASTIC: Initial condition generator for PMFAST
[ascl:1102.016] HERACLES: 3D Hydrodynamical Code to Simulate Astrophysical Fluid Flows
[ascl:1102.017] FARGO: Fast Advection in Rotating Gaseous Objects
[ascl:1102.018] Karma: Visualisation Test-Bed Toolkit
[ascl:1102.019] HOP: A Group-finding Algorithm for N-body Simulations
[ascl:1102.020] SKID: Finding Gravitationally Bound Groups in N-body Simulations
[ascl:1102.021] DIRT: Dust InfraRed Toolbox
[ascl:1102.022] PDRT: Photo Dissociation Region Toolbox
[ascl:1102.023] 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal
[ascl:1102.024] DiFX2: A more flexible, efficient, robust and powerful software correlator
[ascl:1102.025] LensPix: Fast MPI full sky transforms for HEALPix
[ascl:1102.026] CAMB: Code for Anisotropies in the Microwave Background
[ascl:1102.027] ZENO: N-body and SPH Simulation Codes
[ascl:1102.028] ZEUS-MP/2: Computational Fluid Dynamics Code
[ascl:1101.001] Second-order Tight-coupling Code
[ascl:1101.002] NDSPMHD Smoothed Particle Magnetohydrodynamics Code
[ascl:1101.003] IGMtransfer: Intergalactic Radiative Transfer Code
[ascl:1101.004] InterpMC: Caching and Interpolated Likelihoods -- Accelerating Cosmological Monte Carlo Markov Chains
[ascl:1101.005] CMHOG: Code for Ideal Compressible Hydrodynamics
[ascl:1101.006] NIRVANA: A Numerical Tool for Astrophysical Gas Dynamics
[ascl:1101.007] Galaxia: A Code to Generate a Synthetic Survey of the Milky Way
[ascl:1101.008] CRASH: A Block-Adaptive-Mesh Code for Radiative Shock Hydrodynamics
[ascl:1101.009] MasQU: Finite Differences on Masked Irregular Stokes Q,U Grids
[ascl:1101.010] TOPCAT: Tool for OPerations on Catalogues And Tables
[ascl:1011.013] EasyLTB: Code for Testing LTB Models against CosmologyConfronting Lemaitre-Tolman-Bondi Models with Observational Cosmology
[ascl:1011.014] CO5BOLD: COnservative COde for the COmputation of COmpressible COnvection in a BOx of L Dimensions with l=2,3
[ascl:1011.015] Geokerr: Computing Photon Orbits in a Kerr Spacetime
[ascl:1011.016] Non-LTE Models and Theoretical Spectra of Accretion Disks in Active Galactic Nuclei. III. Integrated Spectra for Hydrogen-Helium Disks
[ascl:1011.017] Microccult: Occultation and Microlensing
[ascl:1011.018] chrom_exact: Transit of a Spherical Planet of a Stellar Chromosphere which is Geometrically Thin
[ascl:1011.019] FLY: MPI-2 High Resolution code for LSS Cosmological Simulations
[ascl:1011.020] VisIVO: Integrated Tools and Services for Large-Scale Astrophysical Visualization
[ascl:1011.021] GRALE: A genetic algorithm for the non-parametric inversion of strong lensing systems
[ascl:1011.022] yt: A Multi-Code Analysis Toolkit for Astrophysical Simulation Data
[ascl:1011.023] HyRec: A Fast and Highly Accurate Primordial Hydrogen and Helium Recombination Code
[ascl:1011.001] Identikit 1: A Modeling Tool for Interacting Disk Galaxies
[ascl:1011.002] DAOSPEC: An Automatic Code for Measuring Equivalent Widths in High-resolution Stellar Spectra
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