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The package then defines the model likelihood and optimizes the physical galaxy reconstruction using target images across a range of wavelengths. 008) for fast prototyping with keras models (ascl:1806. Elise, Jake, Malik, and Xiao each solved the same - Gauthmath. GRUMPY (Galaxy formation with RegUlator Model in PYthon) models the formation of dwarf galaxies. Getsources is a powerful multi-scale, multi-wavelength source extraction algorithm. CuTEx analyzes images in the infrared bands and extracts sources from complex backgrounds, particularly star-forming regions that offer the challenges of crowding, having a highly spatially variable background, and having no-psf profiles such as protostars in their accreting phase. PGOPHER simulates and fits rotational, vibrational, and electronic spectra.

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SeeKAT is a Python implementation of a novel maximum-likelihood estimation approach to localising transients and pulsars detected in multiple MeerKAT tied-array beams at once to (sub-)arcsecond precision. WIMpy_NREFT also includes functionality to calculate directional recoil spectra, as well as signals from coherent neutrino-nucleus scattering (including fluxes from the Sun, atmosphere and diffuse supernovae). Elise jake malik and xiao each solved the same inequality in 5. RunDM can also extract the operator coefficients relevant for direct detection, namely low energy couplings to up, down and strange quarks and to protons and neutrons. PT-REX (Point-to-point TRend EXtractor) performs ptp analysis on every kind of extended radio source.

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The Medium Energy Gamma-ray Astronomy library (MEGAlib) simulates, calibrates, and analyzes data of hard X-ray and gamma-ray detectors, with a specialization on Compton telescopes. In addition, Comet provides a tool for publishing VOEvents to the global VOEvent backbone. IRSFRINGE is available as a stand-alone package and is also part of the Spectroscopic Modeling, Analysis and Reduction Tool (SMART, ascl:1210. Elise jake malik and xiao each solved the same inequality in terms. This framework is used as the basis for the flight software for satellite data systems and instruments, but can also be used on other embedded systems. 015), the speedy FFT library. Written in C, it samples halos from a mass function and assigns a profile, carries out ray-tracing simulations, and then counts peaks from ray-tracing maps. On average, EzTao is ten times faster than other tools relying on a Kalman filter for likelihood computation. MultiModeCode facilitates efficient Monte Carlo sampling of prior probabilities for inflationary model parameters and initial conditions and efficiently generates large sample-sets for inflation models with O(100) fields.

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The Fortran code has two major options for power spectrum calculations; -fast, which quickly computes the power spectrum at two-loop level (typically a few seconds) using the pre-computed data set of PT kernels for fiducial cosmological models, and -direct, in which the code first applies the fast method, and then follows the regularized expression for power spectrum to directly evaluate the multi-dimensional integrals. BRUCE writes out a time-sequence of perturbed surface models. The difference operator that can be used independently for detrending a light curve; it is also embedded in ARIMA (autoregressive integrated moving average) Box-Jenkins modeling. The code, written in C and MPI-parallelized, support the computation of power- and bispectra; it also supports higher-order polyspectra, but streamlining the input data is required. Slimplectic is appropriate for exploring cosmological or celestial N-body dynamics problems where nonconservative interactions, e. dynamical friction or dissipative tides, can play an important role. PyMF performs spatial filtering (matched filter, matched multifilter, constrained matched filter and constrained matched mutifilter) image processing that provides optimal reduction of the contamination introduced by sources that can be approximated by templates. CWITools analyzes integral field spectroscopy data from the Palomar and Keck Cosmic Web Imagers, and can be adapted for any three-dimensional integral field spectroscopy data. The wind is modeled as a set of streamlines originating on the surface of the AGN accretion disc, and evolved following their equation of motion, given by the balance between radiative and gravitational force. Elise jake malik and xiao each solved the same inequality math. GLEMuR (Gpu-based Lagrangian mimEtic Magnetic Relaxation) is a finite difference Lagrangian code which uses mimetic differential operators and runs on Nvidia GPUs. Pieflag has two core modes of operation (static and dynamic flagging) with an additional extend mode; the type of data largely determines which mode to choose. The type of mapping that can be expressed is very flexible, and PixelMaps can be compounded into chains of tranformations. For instance, it provides plugins and configuration files that understand HST and JWST data products. The models' parameters are optimised by using the Markov Chain Monte Carlo technique.

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Starduster contains two specific generative models, which explicitly take into account the features of the dust attenuation curves and dust emission spectra. ProFit is a Bayesian galaxy fitting tool that uses the fast C++ image generation library libprofit (ascl:1612. Pygad provides a framework for dealing with Gadget snapshots. Given some data and uncertainties, the code determines the posterior distribution of a model. MARGE (Machine learning Algorithm for Radiative transfer of Generated Exoplanets) generates exoplanet spectra across a defined parameter space, processes the output, and trains, validates, and tests machine learning models as a fast approximation to radiative transfer.

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ArtPop can build stellar populations independently from generating mock images, as one might want to do when interested only in calculating integrated photometric properties of the population. The R package Hyper-Fit fits hyperplanes () and creates 2D/3D visualizations (ot2d / ot3d) to produce robust 1D linear fits for 2D x vs y type data, and robust 2D plane fits to 3D x vs y vs z type data. It aims to mark the abrupt changes in the corresponding wavelength distribution of the emission automatically. Cactus is a software framework for solving time-dependent partial differential equations on block-structured grids, and Carpet acts as driver layer providing adaptive mesh refinement, multi-patch capability, as well as parallelization and efficient I/O. GSSP (Grid Search in Stellar Parameters) is based on a grid search in the fundamental atmospheric parameters and (optionally) individual chemical abundances of the star (or binary stellar components) in question. Lenstronomy reconstructs the lens mass and surface brightness distributions of strong lensing systems using forward modelling and supports a wide range of analytic lens and light models in arbitrary combination. In some cases, the planet can eject the small body from the solar system; in these cases, the program estimates the mean time for the ejection. Mo'Astro sets up a MongoDB collection of a survey's image set, keeping FITS metadata readily available, and providing a place in the reduction pipeline to persist metadata. This method opens up the possibility of recovering more information from existing and future imaging data. It is multi-threading parallel. Model parameters of interest may include neutron star mass and radius (useful to constrain the properties of ultradense nuclear matter) or the system geometry and properties of the hot emitting surface-regions.

The CubeFactory class creates a large image cube from a list of FFI files, which allows the cutout operation to be performed efficiently. 22 arcseconds for 65 Cybele, and the uncertainty in the mean motion varies from 0. Diffstar fits the star formation history (SFH) of galaxies to a smooth parametric model. Given an initial distribution, myRadex evolves the system towards equilibrium using an ODE solver. Self-Interacting Dark Matter (SIDM) is a hypothetical model for cold dark matter in the Universe. The routines in ktransit create and fit a transiting planet model. The values returned by the tool are in units of 10^-6 counts/second/arcminute^2. It uses the REBOUND (ascl:1110. At the simple end of the spectrum a Held-Suarez case is available. It has two basic modes of operation: using an interactive display to specify the positions for the measurements, or obtaining those positions from a file.

It makes a first guess at the shapes of all sources through object recognition techniques; it then allows for departure from such idealized "seeds" through an iterative growing procedure and derives photometric corrections for spatially coincident diffuse emission from a low-order surface fit to the background after exclusion of all detected sources. The kozai package can represent and evolve hierarchical triples using either the Delaunay orbital elements or the angular momentum and eccentricity vectors. The Astrocut package has two parts: the CubeFactory and the CutoutFactory. 019), it provides end-to-end simulation and processing of radio survey data. It uses a U-Net architecture to learn the waveform features of a dataset. SPEX's next generation software is available in OSPEX (ascl:2007.

STAR-MELT is also useful for different applications of spectral analysis where emission line identification is required. PRISM analyzes scientific models using the Bayes linear approach, the emulation technique, and history matching to construct an approximation ('emulator') of any given model. SEVN also provides an up-to-date formalism for pair-instability and pulsational pair-instability supernovae, and is designed to interface with direct-summation N-body codes such as STARLAB (ascl:1010. SIP (Systematics-Insensitive Periodograms) extends the generative model used to create traditional sine-fitting periodograms for finding the frequency of a sinusoid by including systematic trends based on a set of eigen light curves in the generative model in addition to using a sum of sine and cosine functions over a grid of frequencies, producing periodograms with vastly reduced systematic features. Support for HST and JWST is available through the extension stsynphot (ascl:2010. 4 Vesta (new mass determination). 011) to parallelize a Barnes-Hut tree algorithm for a memory-distributed supercomputer. Working in the range of 3, 650-10, 200 Angstroms, the automatic spectral typing algorithm compares important spectral lines to template spectra and determines the best matching spectral type, ranging from O to L type stars.