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Results 601-650 of 1978 (1948 ASCL, 30 submitted)

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[ascl:1611.009] RHOCUBE: 3D density distributions modeling code

[ascl:1611.008] Transit Clairvoyance: Predicting multiple-planet systems for TESS

[ascl:1611.007] GRASP2K: Relativistic Atomic Structure Package

[ascl:1611.006] GalPot: Galaxy potential code

[ascl:1611.005] Exo-Transmit: Radiative transfer code for calculating exoplanet transmission spectra

[ascl:1611.004] PRECESSION: Python toolbox for dynamics of spinning black-hole binaries

[ascl:1611.003] MPDAF: MUSE Python Data Analysis Framework

[ascl:1611.002] tf_unet: Generic convolutional neural network U-Net implementation in Tensorflow

[ascl:1611.001] UltraNest: Pythonic Nested Sampling Development Framework and UltraNest

[ascl:1610.016] PyMC3: Python probabilistic programming framework

[ascl:1610.015] NuPyCEE: NuGrid Python Chemical Evolution Environment

[ascl:1610.014] Freddi: Fast Rise Exponential Decay accretion Disk model Implementation

[ascl:1610.013] MC³: Multi-core Markov-chain Monte Carlo code

[ascl:1610.012] Fourierdimredn: Fourier dimensionality reduction model for interferometric imaging

[ascl:1610.011] BXA: Bayesian X-ray Analysis

[ascl:1610.010] BurnMan: Lower mantle mineral physics toolkit

[ascl:1610.009] velbin: radial velocity corrected for binary orbital motions

[ascl:1610.008] cluster-in-a-box: Statistical model of sub-millimeter emission from embedded protostellar clusters

[ascl:1610.007] gatspy: General tools for Astronomical Time Series in Python

[ascl:1610.006] C³: Command-line Catalogue Crossmatch for modern astronomical surveys

[ascl:1610.005] GSGS: In-Focus Phase Retrieval Using Non-Redundant Mask Data

[ascl:1610.004] MUSE-DRP: MUSE Data Reduction Pipeline

[submitted] centerRadon: Center Determination Code in Stellar Images

[ascl:1610.003] DSDEPROJ: Direct Spectral Deprojection

[ascl:1610.002] CERES: Collection of Extraction Routines for Echelle Spectra

[ascl:1610.001] Piccard: Pulsar timing data analysis package

[ascl:1609.025] PYESSENCE: Generalized Coupled Quintessence Linear Perturbation Python Code

[ascl:1609.024] AdaptiveBin: Adaptive Binning

[ascl:1609.023] contbin: Contour binning and accumulative smoothing

[ascl:1609.022] PyPHER: Python-based PSF Homogenization kERnels

[ascl:1609.021] TIDEV: Tidal Evolution package

[ascl:1609.020] Askaryan Module: Askaryan electric fields predictor

[ascl:1609.019] SuperBoL: Module for calculating the bolometric luminosities of supernovae

[ascl:1609.018] SIP: Systematics-Insensitive Periodograms

[ascl:1609.017] spectral-cube: Read and analyze astrophysical spectral data cubes

[ascl:1609.016] PKDGRAV3: Parallel gravity code

[ascl:1609.015] FIT3D: Fitting optical spectra

[ascl:1609.014] Sky3D: Time-dependent Hartree-Fock equation solver

[ascl:1609.013] 21cmSense: Calculating the sensitivity of 21cm experiments to the EoR power spectrum

[ascl:1609.012] AIPY: Astronomical Interferometry in PYthon

[ascl:1609.011] Photutils: Photometry tools

[ascl:1609.010] CuBANz: Photometric redshift estimator

[ascl:1609.009] NSCool: Neutron star cooling code

[ascl:1609.008] GRASP: General-purpose Relativistic Atomic Structure Package

[ascl:1609.007] Weighted EMPCA: Weighted Expectation Maximization Principal Component Analysis

[ascl:1609.006] SCIMES: Spectral Clustering for Interstellar Molecular Emission Segmentation

[ascl:1609.005] FISHPACK90: Efficient FORTRAN Subprograms for the Solution of Separable Elliptic Partial Differential Equations

[ascl:1609.004] FISHPACK: Efficient FORTRAN Subprograms for the Solution of Separable Elliptic Partial Differential Equations

[ascl:1609.003] Kranc: Cactus modules from Mathematica equations

[submitted] pyLIMA: An Open Source Package for Microlensing Modeling

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