Results 31 to 40 of about 3,113 (292)
Spectral Templates Optimal for Selecting Galaxies at z > 8 with the JWST
The selection of high-redshift galaxies often involves spectral energy distribution (SED) fitting to photometric data, an expectation for contamination levels, and measurement of sample completeness—all vetted through comparison to spectroscopic redshift
Rebecca L. Larson +11 more
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Photometric Accuracy of Deconvolved Simulated Astronomical Images
A study of the photometric accuracy of deconvolved astronomical images was undertaken by processing two simulated images with several well-known algorithms. The simulations consisted of an image of a simple star field and an image of an active galactic nucleus (AGN).
Stephen R. McNeil, J. Ward Moody
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Kinematic Evidence of an Embedded Protoplanet in HD 142666 Identified by Machine Learning
Observations of protoplanetary disks have shown that forming exoplanets leave characteristic imprints on the gas and dust of the disk. In the gas, these forming exoplanets cause deviations from Keplerian motion, which can be detected through molecular ...
J. P. Terry +3 more
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Halted-pendulum Relaxation: Application to White Dwarf Binary Initial Data
Studying compact-star binaries and their mergers is integral to determining progenitors for observable transients. Today, compact-star mergers are typically studied via state-of-the-art computational fluid dynamics codes.
M. Alexander R. Kaltenborn +4 more
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Computer simulation of the growth of ice structures under astronomical conditions
James A. Miller
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Proceedings of the International Astronomical Union: Studying Magnetic Field Amplification in Interacting Galaxies Using Numerical Simulations [PDF]
Simon Selg, W. Schmidt
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We present the implementation of a two-moment-based general-relativistic multigroup radiation transport module in the G eneral-relativistic mu ltigrid nu merical ( Gmunu ) code.
Patrick Chi-Kit Cheong +3 more
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CMR Exploration. I. Filament Structure with Synthetic Observations
In this paper, we carry out a pilot parameter exploration for the collision-induced magnetic reconnection (CMR) mechanism that forms filamentary molecular clouds.
Shuo Kong +4 more
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We use large simulations of Ly α emitters with different fractions of ionized intergalactic medium to quantify the clustering of Ly α emitters as measured by the void probability function (VPF), and how it evolves under different ionization scenarios. We
Lucia A. Perez +3 more
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VLBI Network SIMulator: An Integrated Simulation Tool for Radio Astronomers
In this paper we introduce a software package, the Very Long Baseline Interferometry Network SIMulator (VNSIM), which provides an integrated platform assisting radio astronomers to design the Very Long Baseline Interferometry (VLBI) experiments and evaluate the network performance with a user-friendly interface. Though VNSIM is motivated to be designed
Zhao, Zhen, An, Tao, Lao, Baoqiang
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