Favorable conditions for Raman scattering with atomic hydrogen are easily met in symbiotic stars, young planetary nebulae, and active galactic nuclei. 003) and a flexible R interface to a large number of likelihood samplers. Pomegranate builds probabilistic models in Python that is implemented in Cython for speed. FERRE holds this array in memory, or in a direct-access binary file, and interpolates in it. The same median filtering procedure applied to an image of standard deviations derived from a background-subtracted image results in a flattening image. Elise jake malik and xiao each solved the same inequality math. Witten in python, CosmoSIS consolidates and connects existing code for predicting cosmic observables and maps out experimental likelihoods with a range of different techniques. The pycraf Python package provides functions and procedures for spectrum-management compatibility studies, such as calculating the interference levels at a radio telescope produced from a radio broadcasting tower.
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It implements stellar evolution using SSE (ascl:1303. Elise jake malik and xiao each solved the same inequality in two. SORA optimally analyzes stellar occultation data. ASKAPsoft provides data processing functionality for Australian Square Kilometre Array Pathfinder, including calibration, spectral line imaging, continuum imaging, source detection and generation of source catalogs, and transient detection. DECA can be applied to large samples of galaxies with different orientations with respect to the line of sight (including edge-on galaxies) and requires minimum human intervention.
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BMarXiv scans new (i. e., since the last time checked) submissions from arXiv, ranks submissions based on keyword matches, and produces an HTML page as an output. 017), which can be used with VPFIT to set up the fits, fit the profiles, and examine the result in interactive mode for setting up initial guesses; vpguess (ascl:1408. The cold part of the EOS is modeled after the Varpoly EOS. Elise jake malik and xiao each solved the same inequality in 2. 012) NDF data format. The time step is chosen adaptively in such a way that particles are not allowed to cross more than one radial cell during one step. PUMA (Positional Update and Matching Algorithm) cross-matches low-frequency radio catalogs using a Bayesian positional probability with spectral matching criteria.
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It includes 3-D functionality and several other additional geometries and features. Stretched periodic boxes, and special cases such as simulations with two periodic dimensions and one non-periodic dimension are supported as well. The PyKat wrapper (ascl:2004. 0, a generic point source radiometric model, interfaces with any instrument to provide an estimate of several Payload performance metrics. Because of its generic utility, this package provides a stand-alone implementation that contains the core components of the source separation algorithm. Fastrometry is a Python implementation of the fast world coordinate solution solver for the FITS standard astronomical image. Though Quickclump is primarily intended for decomposing observations of interstellar clouds into individual clumps, it can also be used for finding clumps in any 3D rectangular data. DaMaSCUS-CRUST determines the critical cross-section for strongly interacting DM for various direct detection experiments systematically and precisely using Monte Carlo simulations of DM trajectories inside the Earth's crust, atmosphere, or any kind of shielding. Bmcmc is a general purpose Markov Chain Monte Carlo package for Bayesian data analysis. Elise, Jake, Malik, and Xiao each solved the same - Gauthmath. Users can add effects from a list of pre-implemented astrophysical forces or contribute new ones. Getsf extracts sources and filaments in astronomical images by separating their structural components, and is designed to handle multi-wavelength sets of images and very complex filamentary backgrounds. This black hole can be either Schwarzschild (nonrotating) or Kerr (rotating) by choice of the user.
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The code integrates the hydrostatic equation in order to determine the correct planet radius given the mass in each layer. BlackJAX is a sampling library designed for ease of use, speed, and modularity and works on CPU as well as GPU. These open source libraries can be included in either C++ or Python codes. EqTide calculates the evolution of 2 bodies experiencing tidal evolution according to the "equilibrium tide" framework's "constant-phase-lag" and "constant-time-lag" models. It is built using Keras for developing ML models to run on CPU and GPU seamlessly. RadVel models Keplerian orbits in radial velocity (RV) time series. Though written for K2, EVEREST can be applied to additional surveys, such as the TESS mission, to correct for instrumental systematics and enable the detection of low signal-to-noise transiting exoplanets. Eigentools is a set of tools for studying linear eigenvalue problems. It creates a datacube in FITS format that can be processed with a data reduction package (such as GILDAS, ascl:1305. In both modes of operation PHOTOM performs photometry using either the traditional aperture method or via optimal extraction.
The code has been significantly rewritten and expanded; please see ascl:1812.